{"id":192599,"date":"2017-05-11T13:26:02","date_gmt":"2017-05-11T17:26:02","guid":{"rendered":"http:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/9-may-2017-surprise-when-a-brown-dwarf-is-actually-a-planetary-mass-object-news-astronomy-now-online\/"},"modified":"2017-05-11T13:26:02","modified_gmt":"2017-05-11T17:26:02","slug":"9-may-2017-surprise-when-a-brown-dwarf-is-actually-a-planetary-mass-object-news-astronomy-now-online","status":"publish","type":"post","link":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/astronomy\/9-may-2017-surprise-when-a-brown-dwarf-is-actually-a-planetary-mass-object-news-astronomy-now-online\/","title":{"rendered":"[ 9 May 2017 ] Surprise! When a brown dwarf is actually a planetary mass object News &#8211; Astronomy Now Online"},"content":{"rendered":"<p><p>An artists  conception of SIMP J013656.5+093347, or SIMP0136 for short, which  the research team determined is a planetary like member of a  200-million-year-old group of stars called Carina-Near. Credit:  NASA\/JPL, slightly modified by Jonathan Gagn.  <\/p>\n<p>    Sometimes a brown dwarf is actually a planet  or planet-like    anyway. A team led by Carnegies Jonathan Gagn, and including    researchers from the Institute for Research on Exoplanets    (iREx) at Universit de Montral, the American Museum of    Natural History, and University of California San Diego,    discovered that what astronomers had previously thought was one    of the closest brown dwarfs to our own Sun is in fact a    planetary mass object.  <\/p>\n<p>    Their results are published by The Astrophysical Journal    Letters.  <\/p>\n<p>    Smaller than stars, but bigger than giant planets, brown dwarfs    are too small to sustain the hydrogen fusion process that fuels    stars and allows them to remain hot and bright for a long time.    So after formation, brown dwarfs slowly cool down and contract    over time. The contraction usually ends after a few hundred    million years, although the cooling is continuous.  <\/p>\n<p>    This means that the temperatures of brown dwarfs can range    from as hot as stars to as cool as planets, depending on how    old they are, said the AMNHs Jackie Faherty, a co-author on    this discovery.  <\/p>\n<p>    The team determined that a well-studied object known as SIMP    J013656.5+093347, or SIMP0136 for short, is a planetary like    member of a 200-million-year-old group of stars called    Carina-Near.  <\/p>\n<p>    Groups of similarly aged stars moving together through space    are considered prime regions to search for free-floating    planetary like objects, because they provide the only means of    age-dating these cold and isolated worlds. Knowing the age, as    well as the temperature, of a free-floating object like this is    necessary to determine its mass.  <\/p>\n<p>    Gagn and the research team were able to demonstrate that at    about 13 times the mass of Jupiter, SIMP0136 is right at the    boundary that separates brown dwarf-like properties, primarily    the short-lived burning of deuterium in the objects core, from    planet-like properties.  <\/p>\n<p>    Free-floating planetary mass objects are valuable because they    are very similar to gas giant exoplanets that orbit around    stars, like our own solar systems Jupiter or Saturn, but it is    comparatively much easier to study their atmospheres. Observing    the atmospheres of exoplanets found within distant star systems    is challenging, because dim light emitted by those orbiting    exoplanets is overwhelmed by the brightness of their host    stars, which blinds the instruments that astronomers use to    characterize an exoplanets atmospheres.  <\/p>\n<p>    The implication that the well-known SIMP0136 is actually more    planet-like than we previously thought will help us to better    understand the atmospheres of giant planets and how they    evolve, Gagn said.  <\/p>\n<p>    They may be easier to study in great detail, but these    free-floating worlds are still extremely hard to discover    unless scientists spend a lot of time observing them at the    telescope, because they can be located anywhere in the sky and    they are very hard to tell apart from brown dwarfs or very    small stars. For this reason, researchers have confirmed only a    handful of free-floating planetary like objects so far.  <\/p>\n<p>    tienne Artigau, co-author and leader of the original SIMP0136    discovery, added: This newest addition to the very select club    of free-floating planetary like objects is particularly    remarkable, because we had already detected fast-evolving    weather patterns on the surface of SIMP0136, back when we    thought it was a brown dwarf.  <\/p>\n<p>    In a field where analyzing exoplanet atmospheres is of the    utmost interest, having already seen evidence of weather    patterns on an easier-to-observe free-floating object that    exists away from the brightness of its host star is an exciting    realization.  <\/p>\n<p><!-- Auto Generated --><\/p>\n<p>Here is the original post:<\/p>\n<p><a target=\"_blank\" rel=\"nofollow\" href=\"https:\/\/astronomynow.com\/2017\/05\/09\/surprise-when-a-brown-dwarf-is-actually-a-planetary-mass-object\/\" title=\"[ 9 May 2017 ] Surprise! When a brown dwarf is actually a planetary mass object News - Astronomy Now Online\">[ 9 May 2017 ] Surprise! When a brown dwarf is actually a planetary mass object News - Astronomy Now Online<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p> An artists conception of SIMP J013656.5+093347, or SIMP0136 for short, which the research team determined is a planetary like member of a 200-million-year-old group of stars called Carina-Near. Credit: NASA\/JPL, slightly modified by Jonathan Gagn. Sometimes a brown dwarf is actually a planet or planet-like anyway.  <a href=\"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/astronomy\/9-may-2017-surprise-when-a-brown-dwarf-is-actually-a-planetary-mass-object-news-astronomy-now-online\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":6,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[257798],"tags":[],"class_list":["post-192599","post","type-post","status-publish","format-standard","hentry","category-astronomy"],"_links":{"self":[{"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/posts\/192599"}],"collection":[{"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/users\/6"}],"replies":[{"embeddable":true,"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/comments?post=192599"}],"version-history":[{"count":0,"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/posts\/192599\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/media?parent=192599"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/categories?post=192599"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.euvolution.com\/prometheism-transhumanism-posthumanism\/wp-json\/wp\/v2\/tags?post=192599"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}