Blowtorch of the Gods Captured by Black Hole Image Makers – The New York Times

Dr. Kims group has now reprocessed the observations from those four nights. In addition the group used two other sets of radio telescopes at different frequencies and different resolutions on other days. They did this to study the structure of the quasars jet and zoom in on its source, like opening a set of Matryoshka dolls, in Dr. Kims words.

The results can be seen in the movie above. As viewed from afar at the lowest magnification, the jet bends down from a bright spot at the top of the frame, which corresponds to the center of the quasar, where the black hole is presumably working its grinding magic. Seen closer up, the jet decomposes into a series of blobs or hot spots shooting out. They form a line that bends slightly.

Under the highest magnification, the viewer is left with two blobs one at the top of the image, which is source of the jet, and the lower feature, which is one of the jets outbursts of energy. The source of the jet looks like a bar turned sideways, nearly perpendicular to the direction of the blowtorch.

That, Dr. Kim said in a statement, was a surprise, because they found this unexpected, perpendicular form where they expected to find only the source of the jet.

This is like finding a very different shape by opening the smallest Matryoshka doll, he said.

The perpendicular structure, the astronomers said in their paper, could be the accretion disk itself, the doughnut of fiery doomed material that circles the black hole. Enormous pressures and magnetic fields in that realm squeeze energy out the top and bottom of the doughnut at nearly the speed of light.

Dr. Doleman ventured, however, that it could just be the beam twisting again to make life difficult for the observers.

In the second half of the movie, the astronomers compared images from the Event Horizon Telescope at a single wavelength over the course of a week to see how the knots in the jet were moving.

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Blowtorch of the Gods Captured by Black Hole Image Makers - The New York Times

E. Margaret Burbidge, Astronomer Who Blazed Trails on Earth, Dies at 100 – The New York Times

She joined the University of California, San Diego, in the early 1960s and went on to become the first director of its Center for Astrophysics and Space Sciences. At her death, she was universityprofessor emeritus there.

With her husband, the American physicist William Fowler and the English astronomer Fred Hoyle, Dr. Burbidge wrote a 1957article that is considered one of the most influential scientific papers of its era. Titled Synthesis of the Elements in Stars, but known in astronomical circles simply as B2FH, it was published in the journal Reviewsof Modern Physics.

In it, the authors argued that nearly all of the chemical elements, from aluminum to zinc, are forged in the bodies of stars, a process nowcalled stellar nucleosynthesis.

It was already known that the lightest elements, like hydrogen and helium, had been created amid theBigBang. But the origin of the heavier elements, including the carbon that makes up plants and animals, the oxygen in the atmosphere and the gold and silver mined from the ground in sum, the very matter of the universe was the subject of longstanding debate.

The thesis of B2FH, now widely accepted,isthat the heavier elements are synthesized from the lighter ones by thermonuclear reactions within stars. Loosed into space, these elements can also recombine to form new stars, beginning the cycle once more.

As the article describes it, we are all, in essence, made from stars.

That work laid the foundations for all of modern nuclear astrophysics, and particle astrophysics as well, Dr. Fowler said. It gave a blueprint for how the elements were formed in the cosmos.

(For work on the evolution of stars in general, Dr. Fowler shared the 1983Nobel Prize in Physics with the Indian-American astrophysicist SubrahmanyanChandrasekhar.)

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E. Margaret Burbidge, Astronomer Who Blazed Trails on Earth, Dies at 100 - The New York Times

Astronomers are hoping to see the very first stars and galaxies in the Universe – Universe Today

Sometimes its easy being an astronomer. When your celestial target is something simple and bright, the game can be pretty straightforward: point your telescope at the thing and just wait for all the juicy photons to pour on in.

But sometimes being an astronomer is tough, like when youre trying to study the first stars to appear in the universe. Theyre much too far away and too faint to see directly with telescopes (even the much-hyped James Webb Space Telescope will only be able to see the first galaxies, an accumulation of light from hundreds of billions of stars). To date, we dont have any observations of the first stars, which is a major bummer.

So, astronomers engage in a little bit of cosmic peek-a-boo.Before the first stars formed (the exact date is uncertain, because we havent observed it yet, but we suspect it happened about thirteen billion years ago), the universe was composed almost entirely of pure, unadulterated neutral hydrogen: single electrons bound to single protons in perfect harmony.

But then the first stars appeared, and poured their high-energy radiation throughout the cosmos, flooding the universe with copious X-rays and gamma rays. That intense radiation ripped apart the neutral hydrogen, converting it into the thin but hot plasma that we see in the present-day universe. This process, known as the Epoch of Reionization, started in little patches that eventually grew to engulf the cosmos, like a bunch of weird bubbles.

All this is fascinating, but how can astronomers actually detect this process? They can do it through a little trick of neutral hydrogen: it emits radiation at a very specific frequent, 1420 MHz, which corresponds to a wavelength of 21 centimeters. Before the first stars came online, the neutral gas pumped out this 21cm radiation by the bucketload, with the signal gradually diminishing as the universe became a plasma.

Sounds like a plan, except a) this signal is incredibly weak, and b) a bajillion other things in the universe emit radiation at similar frequencies, including our radios on Earth.

Disentangling the annoying noise from the juicy cosmological signal requires takes mountains of data and sifting through the astronomical haystack for the 21cm needle. We currently dont have the capabilities to make the detection that will have to wait for next-generation radio telescopes like the Square Kilometer Array but current observatories like the Murchison Widefield Array in Western Australia are laying all the necessary groundwork.

Including delivering 200 TB of data in its first pass, which is currently under analysis by some of the most powerful supercomputers in the world.

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Marvel at the universe with the free Northeast Astronomy Forum Virtual Experience today! – Space.com

Each year around this time, thousands of skywatchers, scientists and telescope manufactures flock to Suffern, New York for a weekend reveling at the stars the Northeast Astronomy Forum. This year, due to the coronavirus pandemic, the event has gone virtual and you can watch it live for free today (April 6), no tickets needed.

The Northeast Astronomy Forum, or NEAF, is organized by the Rockland Astronomy Club and has been held for nearly three decades at SUNY Rockland Community College. NEAF 2020 was originally scheduled for this weekend, April 4-5, but the coronavirus pandemic forced organizers to postpone the live event to help curb the spread of COVID-19, the disease caused by the virus.

Instead, NEAF 2020 will hold a one-day free event from 10 a.m. to 8 p.m. EDT (7 a.m. - 5 p.m. PDT). You can tune in to the livestream event here directly from NEAF. It is also being streamed live on YouTube here.

Related: Free space projects for kids at home during the coronavirus outbreakMore: Coronavirus pandemic: Full space industry coverage

The event promises to be packed "featuring product demonstrations, fantastic vendor discounts, door prizes, and amazing speakers that have made the Northeast Astronomy Forum legendary," organizers said in a statement."

Among the speakers in today's forum will be Thomas Zurbuchen, NASA Associate Administrator for science missions; C. Alex Young, the agency's associate director for science, heliophysics division; Samuel Hale, executive director of the Mount Wilson Observatory in California; Dianna Colman, chair of the Yerkes Foundation to Save Yerkes; and planetary scientist Janni Radebaugh, who will discuss Dragonfly, a mission to send a helicopter to Saturn's moon Titan.

Today's one-day livestream is not the end for NEAF 2020. Organizers and CUNY Rockland Community College have rescheduled the event for Sept. 12 and 13.

Email Tariq Malik attmalik@space.comor follow him@tariqjmalik. Follow us@Spacedotcom, Facebook and Instagram.

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Marvel at the universe with the free Northeast Astronomy Forum Virtual Experience today! - Space.com

Here’s the best way to enjoy the ‘Super Pink Moon,’ according to a NASA astronomer – Space.com

Tonight (April 7), the moon will be at its brightest and largest for the whole year during the "Super Pink Moon."

This extraordinary astronomical event is surely not one to miss. Space.com spoke with NASA astronomer Michelle Thaller, the assistant director of science communications at NASA's Goddard Space Flight Center in Greenbelt, Maryland, about tonight's highly-anticipated skywatching event to get a better idea of what to expect and how people can best observe this special supermoon.

"It's just kind of a fun astronomical thing," Thaller said about tonight's full moon. Supermoons, or full moons that appear bigger than usual, occur because our moon does not orbit in a perfect circle around Earth. Rather, it circles our planet in an elliptical-shaped orbit. This means that sometimes the moon is closer to Earth and sometimes it is farther away, causing it to appear bigger or smaller from our perspective on Earth.

Webcast info: How to watch the 'Super Pink Moon' online tonight!Video:Pink supermoon? Astronomer explains what it is

"Tonight the moon is 17,000 miles [27,000 kilometers] closer than average," Thaller said, adding that not only will the moon look bigger in the sky tonight, it will also be about 30% brighter than the average full moon.

Luckily, because it will be so big, bright and obvious in the sky "it's a very simple and easy thing to observe," Thaller said.

This is good news for people who are self-isolating to "flatten the curve" and reduce the spread of the novel coronavirus. Even if you are inside, there is a high likelihood that you'll be able to spot the supermoon through a window.

"All you really need is to be able to look to the eastern horizon at sunset," Thaller said, adding that you have a huge window of time to look at the moon as well. "The wonderful thing about a full moon is that full moons are up all night long, they rise at sunset then they cross over the sky and set at sunrise, so at any point in the night you can go outside and actually see this wonderful big, bright moon."

However, despite how easy it will be for people around the world to check out tonight's supermoon, Thaller added that she has a favorite time to watch a full moon moonrise. "Sometimes it just knocks my socks off to see a full moon rising in the sky," she said.

"When you can see it against the horizon, it looks gigantic. It looks like it's coming in for a landing," she added. "To me, that's the best part."

So, whether you're inside looking out a window or out in your backyard at sunset waiting for a "giant" supermoon to beam up over the eastern horizon, make sure that tonight you look up!

Editor's note:If you have an amazing supermoon photo you'd like to share for a possible story or image gallery, you can send images and comments in tospacephotos@space.com.

Follow Chelsea Gohd on Twitter @chelsea_gohd. Follow us on Twitter @Spacedotcom and on Facebook.

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Here's the best way to enjoy the 'Super Pink Moon,' according to a NASA astronomer - Space.com

Astronomers spot never-before-seen gravitational wave source from binary white dwarf stars – Space.com

Astronomers have detected two stellar corpses whirling around each other, and they might be producing gravitational waves.

White dwarf stars are what become of stars like our sun after they run out of fuel and turn into leftover hot cores. For many years, researchers have predicted that there should be binary, or two-object, systems made up of white dwarf stars. According to general relativity, two such masses orbiting each other should emit energy in the form of gravitational waves, which are ripples or disturbances in the fabric of spacetime.

Now, this is not the discovery of gravitational waves, rather it is the discovery of this binary which may be a source for gravitational waves. But, not only will this study advance our understanding of these systems and gravitational wave sources, it will also be important in validating the efficiency of an instrument that will launch in 2034.

Video:Double star system is a 'cosmic Jekyll and Hyde'Related:Is life possible around binary stars? (Podcast)

The instrument, LISA (the Laser Interferometer Space Antenna) gravitational wave observatory, will use the J2322+0509 system to essentially train with. Because they already know they exist, it's a good test to make sure the instrument can correctly spot it.

"Verification binaries are important because we know that LISA will see them within a few weeks of turning on the telescopes," Mukuemin Kilic, a co-author on this study from the University of Oklahoma, said in the statement. "There's only a handful of LISA sources that we know of today. The discovery of the first prototype of a new class of verification binary puts us well ahead of where anyone could have anticipated."

In a new study identifying and exploring this binary, researchers at the Center for Astrophysics (CfA) at Harvard have detected, for the first time, a binary white dwarf system made up of two white dwarf stars (with helium cores) that are clearly separate stars. This system, known as J2322+0509, has a short orbital period of 1,201 seconds (just over 20 minutes) and is the first gravitational wave source of its kind ever identified.

"Theories predict that there are many double helium-core white dwarf binaries out there," Warren Brown, CfA astronomer and lead author on the study, said in a statement. "This detection provides an anchor for those models, and for doing future experiments so that we can find more of these stars and determine their true numbers."

This system, whose orbital period is the third shortest period of all detached binaries ever found, was fairly tough to spot. "This binary had no light curve," Brown said in the statement. "We couldn't detect a photometric signal because there isn't one." So instead of using a photometric study, which looks at light itself, the team used spectroscopic studies, which observe how matter interacts with electromagnetic radiation like visible light, to identify the star's orbital motion.

But, while the system was tricky to spot, it turns out that this type of binary is an extremely strong source of gravitational waves, the team found using theoretical calculations, according to the statement and the study. The researchers determined that because of the system's alignment with respect to Earth, instruments should pick up a signal 2.5 times stronger than from the same system twisted a different direction.

This binary won't be a binary forever, though, as a consequence of the very gravitational waves the scientists hope to someday detect. "The orbit of this pair of objects is decaying," Brown said. "The gravitational waves that are being emitted are causing the pair to lose energy; in six or seven million years they will merge into a single, more massive white dwarf."

This work is described in a paper posted to the preprint server arXiv.org on April 3 that has been accepted by the journal Astrophysical Journal Letters.

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Astronomers spot never-before-seen gravitational wave source from binary white dwarf stars - Space.com

Interview: Jim Lovell relives the successful failure of Apollo 13 – Astronomy Magazine

Lovell: Well, it did become more famous in the beginning, at least in the eyes of NASA. I have to tell you an interesting story. We came back. Its a failure. So the spacecraft, the command module, which was the only thing left of Apollo 13, really, was in a warehouse down in Florida for about six months. Then, they tried to forget about it. They wanted to go on to Apollo 14 and everything like that.

Then France called up, Paris called up, [the] museum at Le Bourget, which was where Lindbergh landed. They asked the Smithsonian, Do you have any space artifacts that we could have in this museum? Then the lights came on in the Smithsonian and also NASA, Well, we can get rid of this spacecraft. So they exiled Apollo 13 to Le Bourget, and it stayed there for 20 years.

About 18 years after that, I had a classmate that went out there and he saw it and he wrote me a letter. He said, Do you know where your spacecraft is? I didnt at that time. No one told me it was in Le Bourget.Then, later on, a year or so later, my wife [Marilyn] and I were in Paris and we went out to this museum, which was at the airfield there, and there we saw it. We walked up to it. It was still on the cradle that they had rolled it in on. It was all by itself, just about, nothing else around it. The hatch was missing. The instrument panel was missing. The seats were missing. The only thing I saw was a piece of paper that was stuck on the side that said, Apollo 13, and gave the names of the three crew members. And then Ron Howard made the movie. Of course they made the movie that was shown in France, and all those French people said, Oh, its out there in Le Bourget. Lets go see it.

Meanwhile, NASA was so embarrassed and the Smithsonian, that a museum out of Hutchinson, Kansas, called the Cosmosphere, offered to go get [it] and bring it back and pay for it and they did. And all those Frenchmen now were mad because they had kept it for 20 years, and now it came back here. [Laughs.]

Astronomy: Do you recall what the first thing you and Marilyn talked about once you returned after Apollo 13? What did that conversation go like? Did [she] encourage you to find a different career path maybe?

Lovell: Well, I have to tell you another interesting story along those lines. About a week or two weeks after we got picked up in Hawaii and then we came back, we had a big press conference of course. All the NASA people came in and all the reporters came in, and TV people and stuff like that, and a lot of the families came in to listen to the whole thing. We were in the auditorium down in the Johnson Space Center. So we started talking about that.

At the beginning of the conference, a reporter asked, Jim, are you gonna ask for another flight? Obviously, this was not successful. Before that, on Apollo 11 [and] 12, management said, Look, if theres a problem with this flight, well get you back and well give you the very next one.

So when that question came up from the reporter, I thought to myself, because management was right behind us, here was the perfect opportunity to put them on the wall and say yes, because they had not talked to us, the 13, just 11 and 12. I was about ready to say something like that when, out in the audience, I saw a hand go up. Then I saw it go down like this. [Jim gives a thumbs down gesture.] It was my wife. [Laughs.] I could tell. I said, No. I think this is the last flight Im gonna make. [Laughs.]

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Interview: Jim Lovell relives the successful failure of Apollo 13 - Astronomy Magazine

See the waning crescent Moon meet the dawn planets, 1516 April 2020 – Astronomy Now Online

At civil dawn (approximately 40minutes before sunrise in the British Isles) on the mornings of 15 and 16April 2020, let the old crescent Moon be your guide to three naked-eye planets Jupiter, Saturn and Mars. Both the red and the ringed planet lie in the constellation of Capricornus, while Jupiter lies in Sagittarius. This looping animation depicts the view very low to the horizon between southeast and south-southeast around 5:30amBST on the mornings in question. Note that the Moons apparent size is enlarged for clarity. Dabih, otherwise known as BetaCapricorni, is a third-magnitude multiple star. AN animation by Ade Ashford.If youre an early riser in the British Isles fortunate enough to experience clear skies at the start of civil twilight on 15 and 16April, why not venture out at 5:30amBST to see the waning crescent Moon guide you to not just one, but three naked-eye planets Jupiter, Saturn and Mars. Typical 750 or 1050 binoculars will enable you to better appreciate these attractive conjunctions, while the smallest of telescopes also reveal some of Jupiters bright Galilean moons.

What to look for on 15April 2020 at5:30amBSTAt the onset of civil twilight some 40minutes before sunrise in the UK, the waning last quarter lunar crescent lies in Sagittarius just 8degrees slightly less than the span of a fist at arms length above the south-southeast horizon for an observer in the heart of the British Isles.AN graphic by Ade Ashford.At 5:30amBST on 15April, magnitude+0.6 Saturn lies 4degrees to the Moons upper left, while magnitude-2.2 Jupiter 13 times brighter than the ringed planet is 4degrees the upper right of the Moon. Whats more, this attractive celestial triumvirate comfortably fits within the field of view of typical 750 binoculars. Owners of small telescopes can also see Jovian moons Callisto, Europa and Ganymede at this time, but Io is transiting the face of its parent planet.

If your skies are particularly clear, can you glimpse third-magnitude star beta () Capricorni, better known as Dabih, some 5degrees (slightly more than a 1050 binocular field of view, but easily encompassed by 750 instruments) to the upper left of Saturn? If so, can you see that its a double star?

What to look out for on 16April 2020 at5:30amBSTThe almost 23-day-old Moon lies in the constellation of Capricornus at UK civil dawn, some 3degrees to the lower right of magnitude+0.6 planet Mars. The lunar crescent is just 5degrees high in the southeast, so can you glimpse the Red Planet and Moon in the same field of view of 1050 binoculars this morning?

Caution: never sweep with binoculars close to the horizon near sunrise lest you accidentally view the Sun with disastrous consequences for your eyesight. Consult our interactive online Almanac to find the precise time of sunrise for your location. (Clickhere for a users guide to the Almanac.)

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See the waning crescent Moon meet the dawn planets, 1516 April 2020 - Astronomy Now Online

View On Astronomy: Want to see Betelgeuse supernova? You’ll have to wait a bit longer – The Independent

As 2019 came to a close, the news media sensationalized a story about Orions bright star Betelgeuse. The headlines were certainly designed to get ones attention. Betelgeuse was about to go supernova. However, the stars behavior was really old news that was recently enhanced by new observational data. You see, Betelgeuse is a red super giant star (20 times more massive than our Sun and approximately 1,000 times larger) that is indeed nearing the end of its life cycle. And with a star this massive, the result will someday be a supernova event.

Betelgeuse is a known variable star, which pulsates back and forth about one full magnitude (brightness scale) in a 425-day period. What happened more recently is that the star dimmed a little more than usual, by about .2 of a magnitude. An imaging technique using radio waves revealed Betelgeuse appeared to be lopsided, but this discovery turned out to be a huge dust cloud blocking some of the stars light from reaching us. In fact, Betelgeuse has shed off great shells of its outer surface several times in the past, typical activity for these stars as they burn through their supply of nuclear fuel. Speculation arose that Betelgeuses grand finale was soon at hand.

However, every article I read succinctly stated the event could happen soon, or 100,000 years from now. While it is inevitable that Betelgeuse will go supernova in the future, we neednt worry. Fortunately, at its distance of about 700 light years from the Earth, we will not suffer from any hard radiation effects. The supernova will be at least as bright as a full moon and will be visible in broad daylight. About a day before we see the visible light from the supernova event our Earth will be bombarded by a harmless hail of neutrinos and gamma rays. That onslaught will be our advance warning system that Betelgeuse the star has met its demise.

Just as I began to write about Betelgeuses potential imminent demise, new data revealed that Betelgeuse began to brighten once again during mid-to-late February (much like it has in the past). Astronomers will certainly keep monitoring Betelgeuse with their instruments in the hope of capturing the death of a star. If it happens within our lifetime, I hope it occurs when the constellation of Orion is above our horizon. The sight will be spectacular.

Easter Observance Determination

Many religious celebrations are determined by astronomical circumstances. Easter is no exception. But because our secular calendar is not in sync with the motion of the heavens, Easter can occur as early as March 22 or as late as April 25. The general rule is: Easter will fall on the first Sunday after the full moon on or next after the vernal equinox (springMarch 19, 20 or 21). However, if the full moon occurs on a Sunday, Easter is celebrated on the following Sunday. This scenario happened in 2001.

However, there is a caveat to that rule that I only learned about back in 2018. Because the date of the vernal equinox does vary year-to-year, the determination for the Easter date depends on the ecclesiastical approximation of March 21 for the vernal equinox according to https://www.timeanddate.com. This stipulation holds true even if the vernal equinox falls on the 19th or 20th of March.

Therefore, for 2020, using March 21 as the date for the vernal equinox, the next Full Moon after March 21 will be on April 7 at 10:35 pm EDT (Eastern Daylight Time) this year. Therefore, Easter will be celebrated on the following Sunday, April12.

April Lyrids Meteor Shower

Its been a while since Mother Nature has afforded us a decent display of shooting stars. Clouds or bright moonlight have often conspired to prevent us from watching burning rocks falling from the sky. However, on the night of April 22-23, between midnight and dawn, the annual April Lyrids meteor shower will reach its peak of activity. The Lyrids are actually the oldest known shooting star display, having been observed by Chinese astronomers on March 16, 687 BCE. Being such an old display, the number of meteors populating this stream of particles has greatly diminished. However, with good sky conditions and no interfering moonlight, perhaps up to 20 meteors per hour can be counted from dark sky locations.

These swift and bright meteors disintegrate after hitting our atmosphere at a moderate speed of 29.8 miles per second. They often produce luminous trains of dust that can be observed for several seconds. The Moon will be new on the 23rd, so it will not interfere whatsoever with this years shooting star display.

The Lyrids appear to radiate outward from an area of sky on the Lyra-Hercules border near the bright star Vega, which will be about 45 degrees (halfway between the horizon and zenith) above the eastern horizon at midnight and well placed for observing. Let your eyes roam the heavens while facing this general direction. Remember, even though you can trace the dust train left by a Lyrid meteor back to the radiant point, members of this shower can appear anywhere in the sky. The Lyrids are a fairly narrow stream of particles, so dont expect many to be seen before or after peak night. It is produced by dust particles left behind by comet C/1861 G1 Thatcher,

Keep your eyes to the skies!

The author has been involved in the field of observational astronomy in Rhode Island for more than 35 years. He serves as historian of Skyscrapers Inc., the second oldest continuously operating amateur astronomical society in the United States.

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View On Astronomy: Want to see Betelgeuse supernova? You'll have to wait a bit longer - The Independent

Comets Are Breaking Apart in Our Cosmic Backyard, and Astronomers Are Stoked – Popular Mechanics

At the end of August 2019, an amateur astronomer named Gennadiy Borisov made a remarkable discovery. He'd spotted an interstellar comet zipping through our solar system. In December, that comet, newly named 2I/Borisov, made its closest approach to the sunperhaps its first close encounter with any star.

Astronomers have since used Earth's many telescopesboth terrestrial and orbitalto observe the comet. Last week, astronomers reported in a series of posts to the website Astronomer's Telegram that 2I/Borisov showed signs of breaking up. On March 28 and March 30, the Hubble Space Telescope snapped pictures of the interstellar comet and it seemed to have split apart, astronomers reported April 2 in a statement.

"Continuing Hubble Space Telescope images of interstellar object 2I/Borisov...show a distinct change in appearance," read the statement, composed by astronomers David Jewitt of UCLA, Max Mutchler of STSCI, Yoonyoung Kim of the Max Planck Institute for Solar System Research, Hal Weaver of John's Hopkin's University's Applied Physics Laboratory and Man-To Hui of the University of Hawaii.

So far, Jewitt tells Popular Mechanics, only a small fragmentmaybe about a tenth of a percent of the total masshas come off of the roughly 1,600-foot-wide body. One of the pieces, according to an Astronomer's Telegram update posted on April 6, has already disappeared.

"Instead, a diffuse, blob-like feature is visible in its place, extending from the remaining component," Qicheng Zhang of Caltech and Quanzhi Ye and Ludmilla Kolokolova of the University of Maryland reported. Ye tells Popular Mechanics that this blob is likely just bits of dust, ice, and rock which have spun off of the comet.

In early March, astronomers recorded several outbursts, where the Comet Borisov shedded a bunch of materiala tell-tale sign that a break-up may be imminent. It takes a while for that heat to permeate through the comet, Jewitt says. Heat from the sun creeps into pockets of ice inside the comet. That ice vaporizes, forming pressure cooker-like conditions, and poof.

These outbursts may have spurred the fast-moving body to shed even more material. They might have another peculiar effect on the comet: they may cause it to speed up. More observations are needed to confirm Jewitt's hypothesis and measure the speed at which its spinning.

NASA, ESA, and D. Jewitt U.C.L.A.

Borisov is just the second interstellar object to slide across our solar system. In 2017, astronomers discovered an elongated interstellar object they called 1I/Oumuamua. While both objects came from distant corners of the universe, 1I/Oumuamua looked and acted more like a lumpy rock. Comet Borisov, however, has all of the typical characteristics of a comet.

"We know it's spent a really long time out there in the interstellar medium at nearly absolute zero temperature," Jewitt says. "So the question is: Have either of those things affected it in some way and made it measurably different from the comets in our solar system?"

Astronomers hope that the splintering comet might spill secrets about its interstellar journey and the solar system from which it came. In October, a pre-print posted to the website ArXiv, reported that traces of water in the comet's tail. Astronomers have also spotted traces of cyanide in the comet's wake. Unfortunately, due to the spread of the novel coronavirus, many Earth-based telescopes that would have otherwise made additional observations about its composition have been shuttered.

So far, it seems to behave in a very similar way to comets that originated much closer to home. "Borisov's behavior is remarkably similar to its solar system siblings," Ye says. "It has a similar composition to solar system comets; we know that solar system comets with similar characteristics are prone to fragment, and Borisov also did."

Fortunately, we've still got a bit of time with Borisov before it disappears from view completely. Ye estimates it will remain visible to ground-based telescopes for another year. Space telescopes like Hubble will likely be able to see the comet for even longer, perhaps a few years, before it slides out of sight.

We've already learned quite a bit about the nature of interstellar comets from 2I/Borisov, but it's taught us something about our own place in the universe, too. "In my opinion, it tells us that our solar system may not be that unique after all," Ye says. "There's something universal across the stars."

Quanzhi Ye (University of Maryland) and Qicheng Zhang (Caltech)/ Ningbo Education Xinjiang Telescope.

Additional observations made by Ye and his colleague Qicheng Zhang of Caltech using the Ningbo Education Xinjiang Telescope, show that Comet C/2019 Y4 (ATLAS) may be breaking up, too.

The comet was discovered on December 28, 2019, by a group of astronomers at Asteroid Terrestrial-impact Last Alert System (ATLAS) in Hawaii. Astronomers had high hopes for Comet C/2019 Y4 (ATLAS), which was expected to become bright enough to be seen with a decent pair of binoculars (or the naked eye, in dark sky areas) this month, but it might meet its demise before that's possible.

These images, taken this weekend "showed an elongated pseudo-nucleus measuring about 3 arcsec in length and aligned with the axis of the tail, a morphology consistent with a sudden decline or cessation of dust production, as would be expected from a major disruption of the nucleus," according to an Astronomer's Telegram update. Trarnslation: Comet C/2019 Y4 (ATLAS) may be headed for Splitsville.

The comet hasn't appeared as bright the past few nights, further suggesting a break-up might be on the horizon. But comets are unpredictable, and that's what makes them worth watching.

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Comets Are Breaking Apart in Our Cosmic Backyard, and Astronomers Are Stoked - Popular Mechanics

South African Radio Astronomy Observatory Mandated To Manage The Production Of Respiratory Ventilators – Space in Africa

South African Department of Trade, Industry and Competition have mandated the South African Radio Astronomy Observatory (SARAO) to manage the national effort required for the local design, development, production and procurement of respiratory ventilators to support the governments response to combat the COVID-19 (coronavirus) pandemic.

SARAO has been mandated to manage the National Ventilator Project based on the experience it gained in the development of complex systems for the MeerKAT radio telescope, a precursor to the worlds largest Square Kilometre Array radio telescope.

With the number of people who have tested positive for COVID-19 steadily increasing in South Africa, the government has called on companies and experts, particularly engineers and scientists, to come with innovative solutions to help combat the pandemic.

As of 03 April 2020, South Africa had 1 505 confirmed cases of COVID-19. The health ministry expects the number to increase exponentially in the next few weeks as more people get tested.

In an effort to meet the anticipated demand for critical medical equipment such as ventilators, the Department of Trade, Industry and Competition is inviting companies and experts to express their interest in the design, development, production and procurement of ventilators in South Africa.

The invitation provides an opportunity for experts and companies to register their interest regarding the goods and services they offer that may be relevant to the National Ventilator Project. Once the specifications are finalised, interested parties will be invited to make a representation of their proposed solutions and the extent to which they would meet the specification.

Interested parties can register here

Experts interested in providing technical support can register here

Submissions have to be in the standard templates, listed below:

New Report: The African space economy is now worth USD 7 billion and is projected to grow at a 7.3% compound annual growth rate to exceed USD 10 billion by 2024. Read the executive summary of the African Space Industry Report - 2019 Edition to learn more about the industry. You can order the report online.

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South African Radio Astronomy Observatory Mandated To Manage The Production Of Respiratory Ventilators - Space in Africa

COVID-19 Forces Earth’s Largest Telescopes to Close. But a Few Isolated Astronomers Are Still Watching Over the Cosmos – Discover Magazine

The alarm sounded at around 3 a.m. on April 3. An electrical malfunction had stalled the behemoth South Pole Telescope as it mapped radiation left over from the Big Bang. Astronomers Allen Foster and Geoffrey Chen crawled out of bed and got dressed to shield themselves from the 70 degree Fahrenheit temperatures outside. They then trekked a few thousand feet across the ice to restart the telescope.

The sun set weeks ago in Antarctica. Daylight wont return for six months. And, yet, life at the bottom of the planet hasnt changed much even as the rest of the world has been turned upside-down. The last flight from the region left on Feb. 15, so theres no need for social distancing. The 42 winterovers still work together. They still eat together. They still share the gym. They even play roller hockey most nights.

And thats why the South Pole Telescope is one of the last large observatories still monitoring the night sky.

Astronomer Allen Foster controls the $20 million South Pole Telescope from inside the comfort of the South Pole Science Station office. (Credit: Jeff Derosa)

An Astronomy magazine tally has found that more than 100 of Earths biggest research telescopes have closed in recent weeks due to the COVID-19 pandemic. What started as a trickle of closures in February and early March has become an almost complete shutdown of observational astronomy. And the closures are unlikely to end soon.

Observatory directors say they could be offline for three to six months or longer. In many cases, resuming operations will mean inventing new ways of working during a pandemic. And that might not be possible for some instruments that require teams of technicians to maintain and operate. As a result, new astronomical discoveries are expected to come to a crawl.

If everybody in the world stops observing, then we have a gap in our data that you cant recover, says astronomer Steven Janowiecki of the McDonald Observatory in Texas. This will be a period that we in the astronomy community have no data on what happened.

Yet these short-term losses arent astronomers main concern.

Theyre accustomed to losing telescope time to bad weather, and they're just as concerned as everyone else about the risks of coronavirus to their loved ones. So, for now, all that most astronomers can do is sit at home and wait for the storm to clear.

If we have our first bright supernova in hundreds of years, that would be terrible, says astronomer John Mulchaey, director of the Carnegie Observatories. But except for really rare events like that, most of the science will be done next year. The universe is 13.7 billion years old. We can wait a few months.

The prospects get darker when considering the pandemics long-term impacts on astronomy. Experts are already worried that lingering damage to the global economy could derail plans for the next decade of cutting-edge astronomical research.

Yes, there will be a loss of data for six months or so, but the economic impact may be more substantial in the long run, says Tony Beasley, director of the National Radio Astronomy Observatory. Its going to be hard to build new telescopes as millions of people are out of work. I suspect the largest impact will be the financial nuclear winter that were about to live through.

The world's largest optical telescopes, shown here, have shut down in droves in recent weeks (open sites are in green). The Hobby-Eberly Telescope at McDonald Observatory in Texas is the largest optical telescope left observing. Construction has also halted at the Vera C. Rubin Observatory site in Chile. (Credit: Astronomy/Roen Kelly)

Through interviews and email exchanges with dozens of researchers, administrators, press officers and observatory directors, as well as reviewing a private list circulating among scientists, Astronomy magazine has confirmed more than 120 of Earth's largest telescopes are now closed as a result of COVID-19.

Many of the shutdowns happened in late March, as astronomy-rich states like Arizona, Hawaii and California issued stay-at-home orders. Nine of the 10 largest optical telescopes in North America are now closed. In Chile, an epicenter of observing, the government placed the entire country under a strict lockdown, shuttering dozens of telescopes. Spain and Italy, two European nations with rich astronomical communities and a large number of COVID-19 infections closed their observatories weeks ago.

Even many small telescopes have now closed, as all-out shutdowns were ordered on mountaintops ranging from Hawaii's Mauna Kea to the Chilean Atacama to the Spanish Canary Islands. Science historians say nothing like this has happened in the modern era of astronomy. Even during the chaos of World War II, telescopes kept observing.

As wartime fears gripped Americans in the 1940s, German-born astronomer Walter Baade was placed under virtual house arrest. As a result, he famously declared Mount Wilson Observatory in California to be his official residence. With the lights of Los Angeles dimmed to avoid enemy bombs, Baade operated the worlds largest telescope in isolation, making groundbreaking discoveries about the cosmos. Among them, Baades work revealed multiple populations of stars, which led him to realize that the universe was twice as big as previously thought.

In the decades since, astronomers have built ever-larger telescopes to see fainter and farther-off objects. Instruments have become increasingly complex and specialized, often requiring them to be swapped out multiple times in a single night. Enormous telescope mirrors need regular maintenance. All of this means observatory crews sometimes require dozens of people, ranging from engineers and technicians to observers and astronomers. Most researchers also still physically travel to a telescope to observe, taking them to far-flung places. As a result, major observatories can be like small villages, complete with hotel-style accommodations, cooks and medics.

But although observatories might be remote, few can safely operate during a pandemic.

Most of our telescopes still work in classical mode. We do have some remote options, but the large fraction of our astronomers still go to the telescopes, says Mulchaey, who also oversees Las Campanas Observatory in Chile and its Magellan Telescopes. Its not as automated as you might think.

Some of the most complicated scientific instruments on Earth are the gravitational-wave detectors, which pick up almost imperceptible ripples in space-time created when two massive objects merge. In 2015, the first gravitational-wave detection opened up an entirely new way for astronomers to study the universe. And since then, astronomers have confirmed dozens of these events.

The most well-known facilities, the twin Laser Interferometer Gravitational-wave Observatory (LIGO) located in Washington state and Louisiana, both pandemic hot spots closed on March 27. Virgo, their Italian partner observatory, shut down the same day. (Its also located near the epicenter of that countrys COVID-19 pandemic.)

More than 1,200 scientists from 18 countries are involved with LIGO. And no other instruments are sensitive enough to detect gravitational waves from colliding black holes and neutron stars like LIGO and Virgo can. Fortunately, the observatories were already near the end of the third observing run, which was set to end April 30.

You don't know what you missed, says LIGO spokesperson Patrick Brady, an astrophysicist at the University of Wisconsin-Milwaukee. We were detecting a binary black hole collision once a week. So, on average, we missed four. But we don't know how special they would have been.

The gravitational-wave detectors will now undergo upgrades that will take them offline through at least late 2021 or early 2022. But the pandemic has already delayed preliminary testing for their planned fourth run. And it could prevent future work or even disrupt supply chains, Brady says. So, although its still too early to know for sure, astronomy will likely have to wait a couple of years for new gravitational-wave discoveries.

Then there's the Event Horizon Telescope (EHT). Last year, the EHT collaboration released the first-ever image of a black hole. And on April 7, they published another unprecedented image that stares down a black hole's jet in a galaxy located some 5 billion light-years away. But now, EHT has cancelled its entire observing run for the year it can only collect data in March and April due to closures at its partner instruments.

Around the world, only a handful of large optical telescopes remain open.

The Green Bank Observatory, Earths largest steerable radio telescope, is still searching for extraterrestrial intelligence, observing everything from galaxies to gas clouds.

The twin Pan-STARRS telescopes on the summit of Hawaii's Haleakala volcano are still scouting the sky for dangerous incoming asteroids. Both instruments can run without having multiple humans in the same building.

We are an essential service, funded by NASA, to help protect the Earth from (an) asteroid impact, says Ken Chambers, director of the Pan-STARRS Observatories in Hawaii. We will continue that mission as long as we can do so without putting people or equipment at risk.

The 10-meter Hobby-Eberly Telescope at McDonald Observatory in Texas is now operating with just one person in the building. (Credit: Marty Harris/McDonald Observatory)

With observatory domes closed at the world's newest and best telescopes, a smattering of older, less high-tech instruments are now Earth's largest operating observatories.

Sporting a relatively modest 6-meter mirror, the biggest optical telescope still working in the Eastern Hemisphere is Russias 45-year-old Bolshoi Azimuthal Telescope in the Caucasus Mountains, a spokesperson there confirmed.

And, for the foreseeable future, the largest optical telescope on the planet is now the 10-meter Hobby-Eberly Telescope (HET) at McDonald Observatory in rural West Texas. Astronomers managed to keep the nearly-25-year-old telescope open thanks to a special research exemption and drastic changes to their operating procedures.

To reduce exposure, just one observer sits in HET's control room. One person turns things on. And one person swaps instruments multiple times each night, as the telescope switches from observing exoplanets with its Habitable Zone Finder to studying dark energy using its now-poorly-named VIRUS spectrograph. Anyone who doesnt have to be on site now works from home.

We don't have the world's best observatory site. Were not on Mauna Kea or anything as spectacular, says Janowiecki, the HETs science operations manager. We don't have any of the expensive adaptive optics. We dont even have a 2-axis telescope. That was [intended as] a massive cost savings.

But, he added, In this one rare instance, its a strength.

The supervising astronomer of HET now manages Earths current largest telescope from a few old computer monitors he found in storage and set up on a foldout card table in his West Texas guest bedroom.

Like the Hobby-Eberly Telescope, the handful of remaining observatories run on skeleton crews or are entirely robotic. And all of the telescope managers interviewed for this story emphasized that even if theyre open now, they wont be able to perform repairs if something breaks, making it unclear how long they could continue operating in the current environment.

The 48-inch Zwicky Transient Facility telescope at Palomar Observatory in Southern California. (Credit: Palomar/Caltech)

The Zwicky Transient Facility (ZTF) is a medium-sized, robotic telescope at Palomar Observatory in Southern California that's still producing nightly maps of the northern sky. And, thanks to automation, it remains open.

The so-called discovery engine searches for new supernovas and other momentary events thanks to computers back at Caltech that compare each new map with the old ones. When the software finds something, it triggers an automatic alert to telescopes around the world. Last week, it sent out notifications on multiple potentially new supernovas.

Similarly, the telescopes that make up the Catalina Sky Survey, based at Arizonas Mount Lemmon, are still searching the heavens for asteroids. In just the past week, they found more than 50 near-Earth asteroids none of them dangerous.

Another small group of robotic telescopes, the international Las Cumbres Observatory network, has likewise managed to stay open, albeit with fewer sites than before. In recent weeks, their telescopes have followed up on unexpected astronomical events ranging from asteroids to supernovas.

"We are fortunate to still be keeping an eye on potential new discoveries," says Las Cumbres Observatory director Lisa Storrie-Lombardi.

But, overall, there are just fewer telescopes available to catch and confirm new objects that appear in our night sky, which means fewer discoveries will be made.

Chambers, the Pan-STARRS telescope director, says his team has been forced to do their own follow-ups as they find new asteroids and supernovas. This will mean we make fewer discoveries, and that we will miss some objects that we would have found in normal times, he says.

NASA's DART spacecraft is scheduled to launch in 2021 on a mission to visit the binary asteroid Didymos. Astronomers need additional observations to help plot the course. (Credit: NASA/JHUAPL)

Astronomer Cristina Thomas of Northern Arizona University studies asteroids. She was the last observer to use the 4.3-meter Lowell Discovery Telescope before it closed March 31 under Arizonas stay-at-home order.

Thomas warns that, in the short term, graduate students could bear the brunt of the lost science. Veteran astronomers typically have a backlog of data just waiting for them to analyze. But Ph.D. students are often starved for data they need to collect in order to graduate on time.

It's stressing them out in a way that it doesn't for me. Were used to building in a night or so for clouds, Thomas says. If this goes on for months, this could put [graduate students] pretty far behind.

One of Thomas' students was set to have observations collected for their dissertation by SOFIA, NASAs airborne observatory. But the flying telescope is currently grounded in California, leaving it unclear when the student will be able to complete their research. And even when astronomy picks back up, everyone will be reapplying for telescope time at once.

But the damage isn't only limited to graduate students. An extended period of observatory downtime could also have an impact on Thomas' own research. Later this year, shes scheduled to observe Didymos, a binary asteroid that NASA plans to visit in 2021. Those observations are supposed to help chart the course of the mission.

The big question for us is: When are we going to be able to observe again? Thomas says. If its a few months, well be able to get back to normal. If it ends up being much longer, were going to start missing major opportunities.

The Keck Observatory telescopes in Hawaii use high-tech adaptive optics equipment that changes their mirrors' shape 1,000 times per second to counter the twinkling caused by Earth's atmosphere. Keck instruments also need to be chilled below freezing to reduce noise. If the warm up, cooling them down can take days or weeks. (Credit: W. M. Keck Observatory/Andrew Richard Hara)

The same qualities that brought observational astronomy to a standstill in the era of social distancing will also make it tough to turn the telescopes back on until the pandemic has completely passed. So, even after the stay-at-home orders lift, some observatories may not find it safe to resume regular operations. They'll have to find new ways to work as a team in tight spaces.

We are just starting to think about these problems now ourselves, says Caltech Optical Observatories deputy director Andy Boden, who also helps allocate observing time on the Keck Observatory telescopes in Hawaii. There are aspects of telescope operations that really do put people in shared spaces, and thats going to be a difficult problem to deal with as we come out of our current orders.

Astronomers say theyre confident they can find solutions. But it will take time. Tony Beasley, the NRAO director, says his team is already working around a long list of what theyre now calling VSDs, or violation of social distancing problems. Their workarounds are typically finding ways to have one person do something that an entire team used to do.

Beasley's research center operates the Green Bank Telescope in West Virginia, as well as the Very Large Array in New Mexico and the global Very Long Baseline Array all of which are still observing, thanks to remote operations and a reimagined workflow.

Although the new workflow is not as efficient as it was in the past, so far there haven't been any problems that couldn't be solved. However, Beasley says some work eventually may require the use of personal protective equipment for people who must work in the same room. And he says they cant ethically use such gear while hospitals are in short supply.

But Beasley and others think interesting and valuable lessons could still come out of the catastrophe.

There's always been kind of a sense that you had to be in the building, and you've got to stare the other people down in the meeting, he says. In the space of a month, I think everyone is surprised at how effective they can be remotely. As we get better at this over the next six months or something, I think there will be parts where we won't go back to some of the work processes from before.

Despite best efforts and optimistic outlooks, some things will remain outside astronomers' control.

Right now, researchers are completing the 2020 Astronomy and Astrophysics Decadal Survey, a kind of scientific census. The guiding document sets priorities and recommends where money should be spent over the next 10 years. NASA and Congress take its recommendations to heart when deciding which projects get funded. Until recent weeks, the economy had been strong and astronomers had hoped for a decade of new robotic explorers, larger telescopes, and getting serious about defending Earth from asteroids.

Engineers prep NASA's Mars InSight lander for launch to the Red Planet. It is currently stationed on Mars investigating the planet's deep interior. (Credit: NASA)

Many of NASAs most important activities from Mars exploration to studying extrasolar planets to understanding the cosmos are centuries-long projects, the modern version of the construction of the great medieval cathedrals, Princeton University astrophysicist David Spergel told the website SpaceNews.com last year as the process got underway. The decadal surveys provide blueprints for constructing these cathedrals, and NASA science has thrived by being guided by these plans.

However, many experts are predicting the COVID-19 pandemic will send the U.S. into a recession; some economists say job losses could rival those seen during the Great Depression.

If that happens, policymakers could cut the funding needed to construct these cathedrals of modern science even after a crisis has us calling on scientists to save society.

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COVID-19 Forces Earth's Largest Telescopes to Close. But a Few Isolated Astronomers Are Still Watching Over the Cosmos - Discover Magazine

Supermoon and a meteor shower: 2 astronomical events in April to watch from your backyard – LancasterOnline

With the recent pandemic, stay-at-home orders and business closures, remember one thing: the sky will always be there.

There are two big astronomical events happening in April. Permitting that the weather is clear and that light pollution is low, hopeful viewers should see the cosmos in action this month.

April 8 is when the moon will be at its fullest. This year's April full moon, also known as the full pink moon, will also be a supermoon.

Supermoons happen when the moon is at its closest point to the Earth in its orbit, known as its perigee.

In total, four supermoons will be visible in 2020. Two have already happened: one each in February and March.

After April's supermoon, there will be one more in May, known as the full flower supermoon.

From April 22 to 23, the Lyrids meteor shower will be visible.

It's one of the smaller visible meteor showers, producing around 20 or so visible meteors an hour at its peak.

Meteors are best viewed when the skies are especially dark, so watching from a location with little light pollution will be key to watching the showers later this month.

The Lyrids are the precursor to the more lively Eta Aquarids meteor shower, which will happen from May 6 to 7.

Viewers can expect to see 60 or more visible meteors an hour at its peak.

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Supermoon and a meteor shower: 2 astronomical events in April to watch from your backyard - LancasterOnline

Photos: Venus and the Pleiades prepare to meet | Astronomy Essentials – EarthSky

Submit your photo to EarthSky Community Photos here

Dont miss Venus and the Pleiades! Their conjunction was April 3

Stefano De Rosa? in Turin, Italy captured Venus and the Pleiades on April 2, 2020.

Clouded out? Gianluca Masi at the Virtual Telescope Project is also gearing up to present the Venus-Pleiades conjunction to you online. He wrote to EarthSky this weekend:

In the coming week week, the sky will offer us something unique, coming back every 8 years only: a stunning conjunction, involving planet Venus, the brightest object up there these evenings and the wonderful Pleiades, a spectacular star cluster, one of the best gems of the deep sky. To bring some joy from this cosmic show to people worldwide, often quarantined to limit the dissemination of COVID-19, the Virtual Telescope will share this celestial treasure with everyone, offering a live view covering the climax of this cosmic hug between Venus and the Pleiades.

Click into the Virtual Telescopes site to learn more.

Larry Ilardo caught the Pleiades and Venus from Buffalo, New York, on April 1.

View larger at EarthSky Community Photos. | Pradnya Gharpure caught Venus and the Pleiades on April 1 from Nagpur, India, and wrote: Dazzling Venus and the pretty cluster Pleiades make a beautiful sight this evening as they draw closer!!

View larger at EarthSky Community Photos. | Kevin Saragozza captured this striking view of Venus and the Pleiades from Siracusa Plemmeiro on April 1. He wrote: I positioned myself outside in my garden, not having the possibility to catch the alignment together with interesting terrestrial elements because of the COVID-19 quarantine, I preferred a view only from the sky, the Pleiades and Venus aligned in a vertical position.

View larger at EarthSky Community Photos. | Radu Anghel captured many Pleiades stars and a brilliant Venus in this photo from April 1 taken in Bacau, Romania. Radu wrote: Venus and the Pleiades cluster. Two more days before the 8 years meeting. From isolation, but with a great western view.

Piotr Wieczorek shared this beautiful view of the Pleiades and Venus that he took on March 31. Thank you, Piotr!

View at EarthSky Community Photos. | Marek Nikodem caught these stargazers near Szubin, Poland, looking at the moon, Venus and the Pleiades on March 28, 2020. Thank you, Marek.

The moon, Venus and the Pleiades March 28, 2020 via Fred Espenak.

View at EarthSky Community Photos. | Dennis Schoenfelder saw this glorious view of Venus, the moon, and the Pleiades from his front door in Alamosa, Colorado, on March 28. Thank you, Dennis!

Astronomer Alessandro Marchini director of the Astronomical Observatory at the University of Siena in Italy wrote on March 28, 2020: Stargazing from my backyard this evening, with the wonderful triangle with the crescent moon, Venus and the Pleiades (1.3 light-second, 5.5 light-minutes, 445 light-years away each from Earth). Photographed with my Canon Camera and a 100 mm lens on a tripod. Thank you, Alessandro! Venus is the bright object next to the moon. The Pleiades is the tiny, dipper-shaped star cluster at the top of the photo.

View at EarthSky Community Photos. | Stephen Thurston captured this view of the moon, Venus and the Pleiades on March 27. He wrote: Moon and Venus setting over Lake Champlain from Ferrisburgh, VT.

Tom Wildoner of the Dark Side Observatory wrote: I was lucky on the evening on March 27, 2020, to capture this nice view of the planet Venus approaching the Pleiades star cluster in the constellation Taurus. Think this is close? Wait until the evening on April 3rd, the planet Venus will be inside this cluster! Thank you, Tom!

Bottom line: This week, Venus the brightest planet and dazzling evening star in the west after sunset now will pass the beautiful Pleiades star cluster, also known as the Seven Sisters. Were already getting photos submit yours here. Look west after sunset!

Continued here:

Photos: Venus and the Pleiades prepare to meet | Astronomy Essentials - EarthSky

The Thirty Meter Telescope: How a volcano in Hawaii became a battleground for astronomy – Space.com

MAUNAKEA, Hawaii The sun pointed to a little before noon when a chorus of conch shells and bamboo flutes trumpeted into the sharp mountainside breezes. The noise marked the start of a religious ceremony and a demonstration against construction of a massive telescope on what some consider sacred land. The participants saluted east, toward the distant ocean; then south, toward the volcanic shell of a past eruption; then west; then north, toward the summit where a dozen telescopes loomed far out of sight.

Many of the people taking part in that ceremony, halfway up the mountain of Maunakea at the heart of Hawaii's Big Island, were native Hawaiians who call themselves kia'i (pronounced kee AH ee), or protectors. By that, they mean protectors of the mountain itself, from the construction of the Thirty Meter Telescope (TMT) at its summit, where the facility would join venerable observatories like the twin Keck domes and NASA's Infrared Telescope Facility.

I visited the kia'i encampment on the last day of 2019 and the 172nd day of the continuing vigil against construction. Nearby was an octagonal road sign edited to read "Kia'i STOP TMT." Less than two weeks before, with the mountain's harsh winter looming, law enforcement had left the spot. The retreat marked an acknowledgement of a stalemate that began nearly a decade ago and stretches from the ocean to the stars, but is expected to shift once again as spring returns.

(Outside events have already prompted a shift in the situation. In response to the spread of the novel coronavirus that is causing the serious respiratory disease COVID-19, the kia'i have asked visitors to stay away from their previously welcoming encampment, according to a statement released on March 14.)

For the kia'i, the 160-foot-tall TMT (49 meters) would be one telescope too many at a site they see as stolen, sacred, delicate and consistently mismanaged. "It's too big, too massive, and it's in the wrong place," E. Kalani Flores, a professor of Hawaiian studies at Hawaii Community College and one of the lead plaintiffs in court cases surrounding the construction of the Thirty Meter Telescope, told Space.com. "There's a certain tipping point and the TMT would exceed that tipping point."

That's why a subset of native Hawaiians have said no to TMT, in words and actions, for years. Some are calling the current situation an existential crisis for astronomy and for Hawaii. It's certainly a crisis of communication for astronomers who support the project. And while some of the tension reflects Hawaii's history of colonization and oppression, some of the main sticking points display remarkable irony given the telescope's priorities.

Related: Controversy over giant telescope roils astronomy conference in HawaiiMore: Thirty Meter Telescope: Hawaii's giant space eye in pictures

The saga of the TMT began in 2003, when a nonprofit partnership formed between two universities in California and counterparts in Japan, China, India and Canada. Now called TMT International Observatory, the group set out to design a telescope with such a massive observing mirror that it would change science forever. Its findings could tackle some of astronomy's signature existential questions, Gordon Squires, TMT's vice president for external relations and an astronomer by profession, told Space.com: Are we alone? How did the universe wake up? What is dark matter?

Squires said he believes that the process of answering those questions, and the answers themselves, could change humanity forever; that's why he became an astronomer in the first place. "If the world saw the universe the way I do, or the way we do, the world would be a fundamentally different place," he said. "I still believe that."

In 2009, the TMT set its sights on the summit of Maunakea; since then, it has worked to negotiate access and construction with the state, which owns the land, and the University of Hawaii, which manages the astronomy precinct.

It has not gone smoothly.

Flores and other native Hawaiians have filed multiple court cases over the permits required for construction. When the TMT tried to break ground in 2014, the kia'i interrupted the ceremony. Tensions came to a head in July 2019, when the TMT announced it was ready to try building again and the kia'i mobilized, blocking construction trucks from the road that climbs to the summit. They settled in with tents and Porta-Potties, a kitchen and a makeshift university offering lessons in native history and culture.

(By then, the TMT had spent $500 million in 2014 dollars worldwide on the project; current estimates suggest it will total about $2.4 billion in today's dollars, although that number will change based on where and when construction finally begins, a TMT representative said.)

Related: The biggest telescopes on Earth

Each morning, the kia'i greet the sun; three times a day, they conduct a ceremony called the 'aha, or the protocol, a series of chants and dances representing their beliefs about the mountain and lasting an hour or longer. It's that protocol the kia'i began by greeting the cardinal directions, barefoot and clad in street clothes. Early in the ceremony, they called on their ancestors. "Grant us insight, grant us power," one chant reads in a translation posted to the kia'i's website.

For centuries, kia'i told me, those ancestors have come to the mountain and, more frequently, worshipped it from afar. The tenuous atmosphere at the summit, 13,000 feet (4,000 meters) above sea level, leaves little oxygen to feed a human brain. For native Hawaiians, that shortage is a sign that the summit is the realm of deities and that humans should visit only for specific purposes.

That's why Noelani Goodyear-Kaopua, a native Hawaiian and a political scientist at the University of Hawaii at Manoa, has only ever been to the summit once, 10 years ago. Ever since, she has remembered what breathing the thin atmosphere felt like, she told Space.com. "The line between living and dead, or here and the next realm or the realm of the ancestors or however you want to think about that, was much more porous because you are so much out of the realm of where humans are normally supposed to be."

But devotion at a distance has complicated matters for the Hawaiians who wish to see the mountain protected: Because a key piece of their religious practice lies in leaving the summit alone, they've struggled to convince authorities that the land is important to them or that they should have a say in what happens to it.

That said, the kia'i can point to a ring of hundreds of shrines about 1,000 feet below the summit, which they say mark the edge of the most sacred zone. These shrines are nothing dramatic, Flores said: standing stones a foot or two tall, reaching the height of a kneecap, some toppled by time. But TMT construction would run right through that ring, he said, and that shouldn't be acceptable.

(Squires contends that TMT selected its location in consultation with native Hawaiians to avoid areas of concern. "It's on a site that has no historically significant or cultural practice areas on it," he said, citing the nearest cultural site as being a mile away.)

Related: World's largest reflecting telescopes explained (infographic)

In a controversy that is often framed as a conflict between science and religion, despite native Hawaiians pointing to their long history of studying the stars, the shrines point to the first key irony underlying the TMT controversy. Many of the standing stones mark points on the horizon where particularly meaningful stars rose, set or reached their zenith, according to Flores.

"There's hundreds of shrines around, and some of these shrines are interconnected together and then they build a star grid," Flores said. "What you see in the heavens is what you see on Earth."

Hawaii's rich tradition of skywatching is hardly the extent of Maunakea's sacredness, however. Down the slope, as the noontime ceremony continues, the kia'i sing of the creation of what they call Mauna a Wakea, from the union of Wakea the Skyfather and Papa the Earthmother. Native Hawaiians tie their own origin story to that of the mountain.

"We have always revered Maunakea as our sacred mauna," Noe Noe Wong-Wilson, a leader of the kia'i, told Space.com. "In fact, it is part of our cosmology, the very beginning of Earth from which man descends, so for us it's a very spiritual matter."

That's the second irony of the controversy surrounding the TMT, which is tailored to elucidate astronomy's own vision of cosmology.

"Astronomers oftentimes think that an interest in the universe and our origins in the universe is what unites all cultures," Sara Kahanamoku, a native Hawaiian and a doctoral student in marine ecology at the University of California, Berkeley, told Space.com. "But [they] maybe don't realize that some cultures don't necessarily need to explore the universe to know where we come from."

Kahanamoku is the lead author of one of a collection of native-led white papers exploring the ways astronomy in Hawaii affects non-astronomers. The group submitted the papers as public comments to the government's decadal survey of astrophysics, which sets scientific priorities for the field. She and her co-authors offer a collection of recommendations for dealing with situations like the TMT, including establishing a system paralleling the institutional review boards that oversee research done on humans.

"We really believe that good science also means that you also need to be good to the people that you're working among," Kahanamoku said.

Related: Hawaii night sky revealed in stunning new video

Of course, some Hawaiian residents and native Hawaiians alike support the TMT, seeing the telescopes atop Maunakea as modern successors to the islanders' pre-contact expertise at navigating by the stars, as a vital segment of the local economy, and as a pathway to educational and employment opportunities for their children.

(A TMT representative said that it's too early to estimate how much would be spent in Hawaii if the project goes through, but that once the facility is observing, the organization expects to spend about $50 million each year on operations and employ 140 people.)

Tyler Trent, a doctoral student in astronomy at the University of Arizona, is one of those native Hawaiians, although he said he wrestled with the decision. "Whether I'm for it or against it, if that gets built, people are going to be hurt by it," he told Space.com.

Trent concluded that TMT and its counterparts deserve a place on the sacred summit. "I don't see them as like another shopping center or another hotel," he said. "These are special things that are illuminating secrets of the universe." He worries that continuing opposition to the TMT is painting his culture as backward and anti-science, despite the loud objections of kia'i that they are no such thing, and he's disappointed that some astronomers unaffiliated with the project have started speaking out against construction on Maunakea.

"Maybe astronomers taking too neutral of a stance or even supporting the kia'i because that's what they believe being respectful to native Hawaiian culture is I'm starting to think that maybe that's not the right way to go about it," he said. "I think at the end of the day, it's people from the outside picking which native Hawaiian culture they want to support or they want to agree with. I think that if outsiders want to pick one, I truly think that they should support the side that is trying to integrate the two, that is trying to build bridges between the two."

Trent added that he thought he would feel the same way if the site were on his own island, Oahu, which holds Honolulu. But it can't be. For scientists hoping to build the TMT, the summit of Maunakea is simply the best possible site. They want a Northern Hemisphere location to better facilitate partnerships with telescopes in the south, including the equally massive Giant Magellan Telescope already under construction in Chile.

Then, it's a matter of atmospheres. It's here that Maunakea really shines, although you wouldn't know that halfway to the summit, where the kia'i camp amid gusts of wind and transitory bursts of showers and sun.

It's a different story at the summit itself, which picky astronomers consider among the best places on Earth for ground-based astronomy. That's in part because of, ironically, one of the same reasons native Hawaiians consider the peak sacred: the barely-there oxygen. Like so many telescopes around the world, TMT has gravitated to a mountaintop site that would carry its optical equipment through some of the lower layers of Earth's atmosphere, which can blur telescope images.

Even the summit's view, however, leaves astronomers dissatisfied. That's why TMT would be armed with an adaptive optics system, which measures and automatically subtracts blurriness caused by the atmosphere. TMT's version would be equipped with lasers that create artificial stars for the system to judge, which lets astronomers observe fainter objects.

But such technology doesn't negate astronomers' desire to remain perched at high elevations, TMT project scientist Christophe Dumas told Space.com. For a project as ambitious as TMT, he said, siting is crucial to an instrument's output, despite opposition. The TMT has its eye on a site in the Canary Islands as a back-up location, which would slightly reduce the project's price tag, a representative said. But that site is still a clear second choice for astronomers and would require some adjustments to the facility, he said.

For the kia'i, their opposition is not just about Maunakea, it's about the way astronomy and science in general operates, particularly given that mountaintops are nearly always sacred to someone. One leader of the kia'i emphasized that the solution was not merely for the TMT to move, as some astronomers have begun to call for, but to find a location where people truly welcome it.

That could require a new way of approaching such projects, several native Hawaiians said. In particular, scientists looking to start a new project would be wise to incorporate local communities in discussions long before any opposition begins long before it's even a project, in fact.

'Imiloa Astronomy Center, which operates under the aegis of the University of Hawaii at Hilo and seeks to tell all the various stories of Maunakea, is working to foster these conversations at Maunakea and elsewhere. Such dialogues should begin earlier and without such tense motivation, Ka'iu Kimura, a native Hawaiian and 'Imiloa's director, told Space.com. "Not because there's conflict, but because it's just the right thing to do," she said.

The astronomy precinct at Maunakea and the TMT specifically are far, far past that point. Construction on the first modern telescope at the site began in 1964, and over the intervening decades, plenty of hard feelings have built up.

TMT isn't the first Maunakea project to meet opposition, but supporters and kia'i alike told me that things seem to be different this time. "I think a lot of people are saying, we have stood by long enough," Goodyear-Kaopua said. "The narrative that's been put forward is, well, why can't Hawaiians just share? We have been sharing for a long time, not always at our consent." She wants to see more native Hawaiians involved in making decisions about the summit.

One of the most significant decisions about the summit was made in the fall of 2018, when a state Supreme Court ruling allowed the project to continue. Four justices agreed with the state land management board's argument that astronomy had already changed the summit so much that one more observatory couldn't really make a difference. One dissented, arguing that this so-called degradation principle set a dangerous precedent.

For the kia'i, who see the mountain as a relative as much as a resource, "one more can't hurt" is not an acceptable philosophy. Many of the native Hawaiians I spoke with pointed to the degradation principle to voice their concerns about how decisions are made not just at Maunakea, but around the world. Some referenced climate change, others focused on land use, but many expressed concern about how humans have exploited and continue to exploit the planet.

Related: European scientists are taking a mock moon mission in Hawaii right now

Toward the end of the protocol, the ceremony leader explained that the next dance was a new addition to the daily ceremony. It traced water on its journey throughout the island and the water cycle, they said: from ocean to clouds to rain to waterfalls to ponds to rivers to cultivated fields to estuaries to ocean, with plenty of stops in between.

It's that same connected water that the kia'i mentioned again and again in their concerns about the TMT. It's another irony in the controversy: Among other discoveries, the TMT could help astronomers identify planets with water in their atmospheres, a first step toward finding a habitable world. But the kia'i already know of one very habitable planet with that precious liquid in its atmosphere, and they consider it their responsibility to protect that water and the mountain that anchors it to the Big Island.

(It was while watching this dance that I was struck by how closely the protocol seemed to parallel the kia'i concerns about the telescope; I've structured this story to follow the protocol as a mark of gratitude for the ceremony leader's work to make that connection.)

"Water is a sacred thing for all of humanity," Kealoha Pisciotta, a native Hawaiian who was a technician at two telescopes on Maunakea before deciding she couldn't condone the way the observatories treat the summit, told Space.com. "We use it ceremonially as well; the snow, ice and water from Maunakea is collected for ceremony."

One of Pisciotta's concerns about astronomy at Maunakea has been the observatories' treatment of the water. She said that during her time working on the summit, she saw spills of hazardous substances from bug spray to mercury, and that she has seen evidence of only one existing observatory addressing those issues.

It's one of the most common concerns I heard about TMT as well, that it could contaminate water across the island. The TMT's response is that those concerns are completely unfounded. There's no evidence the observatory could affect the water, the TMT says; the nearest wells are about 12 miles away; the observatory won't rely on mercury, the worst of the chemicals used to clean telescope mirrors; the facility has a system to transport wastewater from science operations and human staff support alike off the mountain.

But still, the kia'i say, they worry about the water. The summit is a particularly sensitive place in the eyes of native Hawaiians because it's where water first touches land. "It's in its purest form, unaltered by humans, unaltered by any other aspects," Flores said of the rain, snow and fog at the summit, which makes interfering with it particularly dire. "You disrupt, disturb, desecrate the water in its highest forms, and [the elders] tell us the water is the basic form of life for all of us on this planet."

And while the kia'i agree that the hydrology models of Hawaii to date show that TMT shouldn't contaminate anything, that isn't a satisfactory response for them. "I think regardless of that, because the models are not clear, there's still a possibility that there could be infiltration because it's very complex," Rosie Alegado, a native Hawaiian and an oceanographer at University of Hawaii at Manoa, told Space.com. "The models that we have are definitely incomplete."

For Stephanie Malin, an environmental sociologist at Colorado State University, that situation is not surprising. Development projects typically rely on technocratic assessment of potential risks, she said, while indigenous groups tend to exercise a precautionary principle that delays development until there is certainty that there are no risks which isn't always possible.

"I don't necessarily think that the two groups are talking the same language, even," Malin told Space.com.

Related: How space exploration can teach us to preserve all life on Earth

Near the end of the noontime ceremony, the gathered kia'i completed a series of dances open to all, regardless of their knowledge of hula. The only requirement, the ceremony leader explained, was that participants dance with the intention of stopping TMT from being constructed on Maunakea. And so the kia'i hold space at the mountain and dance three times a day, to protect the mountain that tells them their place in the universe. Later, they progressed toward the summit, taking one step at a time, dodging the tents around the dance space.

It's not clear what the TMT's steps forward might be. If the TMT decides the Maunakea site is no longer worth the pain, as the kia'i hope, they will take their plans to the Canary Islands. It's unclear how much longer they are willing to wait to begin construction which is scheduled to last 10 years in earnest.

A sharper deadline is also looming over Maunakea: the master lease agreement between the state and the University of Hawaii, which governs every observatory's sublease, will expire in 2033. What negotiations might look like is still unclear, but chances are they won't resemble the process that led to the original agreement decades ago. The master lease worries all the observatories on the summit, but particularly TMT, which dreads reaching first light just in time for site access to fall apart entirely.

Even the most strident opponents of TMT aren't calling for all the telescopes to be removed. They do, however, want the observatories to be better neighbors, more responsive to local concerns and more respectful of the land from which they study the stars.

No one thinks that will be straightforward. For the astronomers affiliated with the TMT project, the conversations of the past decade have already challenged their perceptions of their own values. "We never thought we were the bad people, and some people think authentically that we are," Squires said.

The kia'i I spoke with never phrased their feelings quite like that. Many insisted they aren't trying to stop science: Instead, they're trying to improve it.

"Science that doesn't empower humanity for a better Earth is maybe not the science we need to be doing," Pisciotta, the former telescope technician who once dreamed of studying cosmology and who described her family as traditional star people, said. That's perhaps especially true of astronomy, she added, since astronomers cannot escape the way distance acts as a time machine across the universe.

"Everything in astronomy is looking back in time," she said. "It has to find its modern relevancy. Yes, it's noble, but we can make it more noble together, though."

Email Meghan Bartels at mbartels@space.com or follow her @meghanbartels. Follow us on Twitter @Spacedotcom and on Facebook.

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The Sky This Week from March 20 to 27 – Astronomy Magazine

Friday, March 20Its officially spring in the Northern Hemisphere. To celebrate, Mars and Jupiter meet up in the morning sky in the first of two planetary conjunctions this month. Look for the glittering stars of Sagittarius the Archer in the southeast in the two hours or so before sunrise. There, magnitude 0.9 Mars is a mere 0.7 south of magnitude 2.1 Jupiter.

About 7 east of Jupiter, magnitude 0.7 Saturn waits its turn for a close-up with the Red Planet. Mars will soon tango with the ringed world, coming closest on March 31.

Saturday, March 21Today is the perfect day to seek out our solar systems speediest planet. The Moon passes 4 south of Mercury at 2 P.M. EDT, but youll want to catch the pair in the morning before sunrise. At that time, the two will stand 5 apart, with Mercury glowing at magnitude 0.2 in the east-southeast 30 minutes before the Sun crosses the horizon.

Saturday is also Galactic Tick Day. The holiday is celebrated every 633.7 days (1.7361 years) to mark one galactic tick, which represents 1/100 of an arcseconds worth of the orbit our Sun and solar system make around the Milky Way. (It takes 225 million years to complete a full orbit.) You can learn more about the origins of this quirky and humbling holiday on the Galactic Tick Day homepage.

In honor of our journey through the galaxy, step outside from a dark site to see if you can spot the Milky Way running overhead. The plane of our galaxy runs through Cygnus the Swan, setting in the northwest as the sky grows darker after sunset. In the east, Orion the Hunter rises with the Milky Way at his right shoulder, which is marked by the bright red star Betelgeuse.

Sunday, March 22The fast-fading Moon is just 3 percent lit and rises shortly before the Sun, making tonight an excellent night to search out some of the skys fainter objects. Consider trying for M81 and M82, also known as Bodes Galaxy and the Cigar Galaxy, respectively. Both in the constellation of Ursa Major, these two galaxies appear only 37' apart on the sky and are easy to catch in the same field of view through binoculars or a telescope at low magnification. M81 has an active supermassive black hole in its center, while M82 is undergoing a massive burst of star formation hence its classification as a starburst galaxy. Astronomers believe this flurry of activity was actually caused by gravitational interactions with M81. Through a scope, M82 appears long and thin like a cigar while M81 has a rounder shape.

Monday, March 23Mercury reaches greatest western elongation (28) at 10 P.M. EDT, several hours before it rises ahead of the Sun. At sunrise, the tiny magnitude 0.3 planet is 10 above the horizon in the east-southeast, and its 7"-wide disk is just over half lit.

Today also marks the 180th anniversary of the first photograph ever taken of the Full Moon. John Draper captured the daguerreotype on this date from his observatory in New York after several previous attempts.

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Slooh will livestream astronomy lesson for K-12 students during coronavirus outbreak – Space.com

Slooh astronomers will livestream a free astronomy lesson for K-12 students who are homebound during the coronavirus pandemic.

On Thursday (March 19), Slooh will livestream a free, 1-hour astronomy lesson and live telescope views from around the world. The webcast, which is geared toward K-12 students, will begin at 4:30 p.m. EDT (2030 GMT). You can watch it live on Slooh's YouTube channel, or stream it here on Space.com, courtesy of Slooh.

"Slooh is committed to bringing out the very best in students and all people," Russell Glenn, director of education for Slooh, said in an emailed statement. "We believe that space education is crucial in understanding and gaining perspective on the world around us."

Related: Free space projects for kids (and adults) stuck at home during the coronavirus outbreak

During the webcast, Glenn and Slooh astronomer Paul Cox will walk viewers through one of Slooh's starter quests, called Cosmic Explorer, which introduces students to the Slooh interface and offers a basic lesson on the sun, moon, galaxies, and the birth and death of stars. This livestream will also provide views of objects that are visible in the night sky.

"We want to help people to share in the wonder of space together as a community so that we can recognize our shared humanity," Glenn said. "We will be bringing as much content as possible during this challenging time. We see this great challenge as a great opportunity for students to own their learning and get excited about space."

The webcast will also provide views of space from Slooh's 10 online telescopes, including those situated at the Institute of Astrophysics of the Canary Islands, which makes daytime astronomy possible for students in the United States, Slooh officials said in a statement.

In addition to this free astronomy lesson, Slooh offers several paid membership options for students, teachers and parents to learn about space while they are homebound. Slooh community members can control Slooh's telescopes online, schedule missions, and select and work on different educational activities, called quests.

"When their mission is active, they can be observing and capturing images in real time," Glenn said in the email to Space.com. "Additionally, students can observe other missions planned by other members of the Slooh community and capture images of the objects that they are viewing."

Slooh also offers astronomy clubs for educators to engage students and citizens from home and explore space together via a network of online telescopes. This includes remote learning activities and support from Slooh's astronomy educators.

Follow Samantha Mathewson @Sam_Ashley13. Follow us on Twitter @Spacedotcom and on Facebook.

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Astronomers have found the edge of the Milky Way at last – Science News

Our galaxy is a whole lot bigger than it looks. New work finds that the Milky Way stretches nearly 2 million light-years across, more than 15 times wider than its luminous spiral disk. The number could lead to a better estimate of how massive the galaxy is and how many other galaxies orbit it.

Astronomers have long known that the brightest part of the Milky Way, the pancake-shaped disk of stars that houses the sun, is some 120,000 light-years across (SN: 8/1/19). Beyond this stellar disk is a disk of gas. A vast halo of dark matter, presumably full of invisible particles, engulfs both disks and stretches far beyond them (SN: 10/25/16). But because the dark halo emits no light, its diameter is hard to measure.

Now, Alis Deason, an astrophysicist at Durham University in England, and her colleagues have used nearby galaxies to locate the Milky Ways edge. The precise diameter is 1.9 million light-years, give or take 0.4 million light-years, the team reports February 21 in a paper posted at arXiv.org.

To put that size into perspective, imagine a map in which the distance between the sun and the Earth is just one inch. If the Milky Ways heart were at the center of the Earth, the galaxys edge would be four times farther away than the moon actually is.

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To find the Milky Ways edge, Deasons team conducted computer simulations of how giant galaxies like the Milky Way form. In particular, the scientists sought cases where two giant galaxies arose side by side, like the Milky Way and Andromeda, our nearest giant neighbor, because each galaxys gravity tugs on the other (SN: 5/12/15). The simulations showed that just beyond the edge of a giant galaxys dark halo, the velocities of small nearby galaxies drop sharply (SN: 3/11/15).

Using existing telescope observations, Deason and her colleagues found a similar plunge in the speeds of small galaxies near the Milky Way. This occurred at a distance of about 950,000 light-years from the Milky Ways center, marking the galaxys edge, the scientists say. The edge is 35 times farther from the galactic center than the sun is.

Although dark matter makes up most of the Milky Ways mass, the simulations reveal that stars should also exist at these far-out distances. Both have a well-defined edge, Deason says. The edge of the stars is very sharp, almost like the stars just stop at a particular radius.

In the future, astronomers can refine the location of the Milky Ways edge by discovering additional small galaxies nearby. Astronomers could also search for individual stars out at the boundary, says Mike Boylan-Kolchin, an astrophysicist at the University of Texas at Austin who was not involved with the study. The farthest such stars will be very dim, but future observations should be able to find them.

The measurement should also help astronomers tease out other galactic properties. For instance, the larger the Milky Way, the more massive it is and the more galaxies there should be revolving around it, says Rosemary Wyse, an astronomer at Johns Hopkins University who was not part of the new work. So far, there are about 60 known Milky Way satellites, but astronomers suspect that many more await discovery.

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Astronomers test string theory using NASA’s Chandra X-ray space telescope – Space.com

Astronomers have probed the Perseus galaxy cluster in search of an (so far) undetected particle that would help to support string theory.

String theory is the idea that all known forces, particles and interactions can be connected through a single framework to understand the physical universe. A team of astronomers using NASA's Chandra X-ray Observatory studied galaxy clusters the largest structures in the universe held together by gravity for signs of an ultra-low-mass particle called an axion, which many models of string theory predict should exist.

"While it may sound like a long shot to look for tiny particles like axions in gigantic structures like galaxy clusters, they are actually great places to look," David Marsh, co-author of the study from Stockholm University in Sweden, said in a statement from the Chandra X-ray Observatory.

Related: 7 surprising things about the universe

Axion particles are believed to have incredibly low masses, potentially ranging from a millionth of the mass of an electron down to zero mass. The team also looked for signs of "axion-like particles," which are a broader class of ultra-low-mass particles with similar properties to axions, according to the statement.

Additionally, these ultra-low-mass particles may sometimes convert into photons the particles that make up light when they pass through magnetic fields. In turn, photons may also convert into axions under certain conditions. Both scenarios depend on the mass of the particles and how easily they can make the conversion, also known as convertibility, according to the statement.

As part of this new study, astronomers using the Chandra space telescope studied the spectrum of X-ray emissions produced by material falling towards the supermassive black hole at the center of the Perseus galaxy cluster.

"Galaxy clusters contain magnetic fields over giant distances, and they also often contain bright X-ray sources," Marsh said in the statement. "Together these properties enhance the chances that conversion of axion-like particles would be detectable."

However, the team did not detect any distortions in the X-ray emissions that would indicate axion-like particles were present, according to the statement.

"Our research doesn't rule out the existence of these particles, but it definitely doesn't help their case," Helen Russell, co-author of the study from the University of Nottingham in the UK, said in the statement. "These constraints dig into the range of properties suggested by string theory, and may help string theorists weed their theories."

One possible explanation for these recent observations is that the particles have either a lower or higher convertibility than the Chandra space telescope is able to detect, the researchers said.

"Until recently I had no idea just how much X-ray astronomers bring to the table when it comes to string theory, but we could play a major role," Christopher Reynolds, lead author of the study from the University of Cambridge in the United Kingdom, said in the statement. "If these particles are eventually detected it would change physics forever."

Their findings were published Feb. 10 in The Astrophysical Journal.

Follow Samantha Mathewson @Sam_Ashley13. Follow us on Twitter @Spacedotcom and on Facebook.

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We All Live In A Croissant-Shaped Giant Bubble, Say Astronomers – Forbes

Is this what the heliosphere looks like? New research suggests so. The size and shape of the ... [+] magnetic "force field" that protects our solar system from deadly cosmic rays has long been debated by astrophysicists.

Physicistshave revealed a refined new model of the heliospherethe vast region around the Sun extending more than twice as far as Plutothat depicts it as a crescent-shaped magnetic force-field resembling a freshly baked croissant.

Its the region of space that the Sun commands; its sphere of influence. Its the extent of the solar windcharged particles spewed-out by the Sunthat extends far past the orbits of the planets, creating a bubble around the Sun that accompanies it in its journey through interstellar space. At the edges of the heliosphere is where the solar wind meets the interstellar wind. It casts a magnetic force field around all the planets, deflecting charged particles that would otherwise get into the solar system ... and destroy DNA.

Thats controversial. Until recently, the consensus was that the shape of the heliosphere is comet-like. Its long been thought that the heliosphere stretches behind the solar system, creating a comet-like shapewith a round nose on one side and a long tail extending in the opposite direction. However, its also been described as a beachball-shape. However, according to Merav Opher, professor of astronomy and researcher at Boston UniversitysCenter for Space Physics, and her coauthor James Drake of the University of Maryland, the helio-sphere should really now be called the helio-crescent.

This graphic shows the position of NASA's Voyager 1 and Voyager 2 probes, outside of the ... [+] heliosphere, a protective bubble created by the Sun that extends well past the orbit of Pluto.

Opher and Drakes original paper in 2015 used data from NASAs Voyager 1 spacecraft, which crossed the boundary from heliosphere to interstellar space in May 2012. They identified two giant jets of material shooting backwards over the north and south poles of the Sun that curve around in two relatively short tails toward the back; a heliosphere that looks a lot more like a crescent moon than a comet.

A new simulation of the heliosphere the magnetic bubble surrounding the sun shows it to have two ... [+] relatively short jets streaming away from the nose.

Opher and Drakes research was controversial. It was very contentious, she says. I was getting bashed at every conference! But I stuck to my guns. However, in 2017 another model was proposed by scientists working on NASAs Cassini mission at Saturn. It stated that the heliosphere is much more compact and rounded than previously thoughtsomething like a beach ball.

Many other stars show tails that trail behind them like a comets tail, supporting the idea that our ... [+] solar system has one too. However, new evidence from NASAs Cassini, Voyager and Interstellar Boundary Explorer missions suggest that the trailing end of our solar system may not be stretched out in a long tail. From top left and going counter clockwise, the stars shown are LLOrionis, BZ Cam and Mira.

Its Opher and Drakes refined theory, with colleagues Avi Loeb of Harvard University and Gabor Toth of the University of Michiganoutlined in a new paper published in Nature Astronomythat two jets extend downstream from the nose rather than a single fade-away tail. Their new 3D model of the heliospheredeveloped on NASAs Pleiades supercomputer and supported by NASA and by the Breakthrough Prize Foundationreconciles their croissant model with the beach ball model. It does so by distinguishing between the solar wind and incoming neutral particles that drift into the solar system; the latter get much hotter so have an outsized influence on the shape of the heliosphere. However, there is still uncertainty; it depends on exactly how you define the edge of the heliosphere.

This artists impression shows the view from the surface of one of the planets in the TRAPPIST-1 ... [+] system.

The solar wind and the heliosphere could be key ingredients in the recipe for life in the Milky Way and beyond. "If we want to understand our environment we'd better understand all the way through this heliosphere," says Loeb, Opher's collaborator. Researchers studying exoplanets are keen to compare the Suns heliosphere with those around other stars. Theres also the DNA-shredding interstellar particles, which actually could have helped drive the genetic mutations that led to life like us, says Loeb. "At the right amount, they introduce changes, mutations that allow an organism to evolve and become more complex," he says. "There is always a delicate balance when dealing with life as we know it. Too much of a good thing is a bad thing," says Loeb.

Starting in the early 2030s, the Interstellar Probe would exit the solar system.

We need to explore the sea of space between our Sun and other potentially habitable systems. For now, all we have are the fading 40 year old science instruments on Voyager 1 and Voyager 2. Cue plans for the Interstellar Probe, a spacecraft that could launch in the 2030s and go farther and faster than any spacecraft before it to help us understand our home in the galaxy. It would start exploring the edge of the heliosphere 10 or 15 years after that. With the Interstellar Probe we hope to solve at least some of the innumerous mysteries that Voyagers started uncovering, says Opher.

Wishing you clear skies and wide eyes.

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