Our new room sucks with motor bikers ripping by at all hours in the night waking us up. We got moved because our old room had bugs in it. This morning when we woke up we requested a move back which will happen at 7 tonight after the bugs are cleared. Again we debated doing our advanced diving course which would certify us for night dives and down to 30m instead of 18m. After a bit of talking Jeff
Ho Chi Mihn City
On November 3rd at 8 a.m. we made our way up the Saigon River to the one and only Ho Chi Minh City. Yep thatrsquos in Vietnam. The whole voyage and the time up until the voyage I was looking forward to Vietnam I thought it was going to be an awesome experience as I didnrsquot really know too much about the place. It wasnrsquot until we left India and began studying Vietnam that I realiz
Boston Science Museum
Today Dean myself and my niece Ashley went to the Boston Science Museum. D and I haven't been there in years. Ashley has never been there until today that is. Anyway I asked Ashley if she wanted to go with me because they are having a Harry Potter exhibit. While Ashley and I were in the exhibit Dean waited for us in the lobby he doesn't care for Harry Potter. It took us about 40 minut
Plan a Runescape Theme Birthday Party to earn runescape gold
Runescape in real life Well the weapons may have to be left in cyberspace but there are many great Runescape online game concepts for a cool party. For a birthday party or another event teenagers will have fun bringing Runescape to life and it will also bring you much runescape gold.Runescape is an online browserbased game played by people all over the world. The game holds the Guinness world
Bahia Ballena
Bahia BallenaFor the folks in Ballena Isle Marina yes there is another Ballena Bay it Is just around Punta Abreojos. The Spanish words abre ojos mean open the eyes and is a reference to the nasty rocks called Roca Ballena just offshore and the dangerous shoals near this point. Again we departed Bahia Asuncion at dawn and found a perfectly flat sea and no wind at all. Motoring again
pre flight test…. again
just a before i go reminder on how to post here... still havent figured out pictures... sorry
Bahia Ballena to Bahia San Juanico
Bahia San Juanicoh2Another dawn start for the anchorage at Bahia San Juanico. It's Christmas day.Here is a photo of echo that shows what it looks like to be out sailing at the break of dawn. Once out of Bahia Ballena the wind picked up and by 0730 it was up to 18 knots with a little bit of sea. By 0830 the wind was over 20 knots and we both reefed down. By 0930 it dropped to 10 knots so w
A ghost of Christmas past
Five years ago I was sitting at work in that quiet week between Christmas and New Year’s Day desperately looking for the 10th planet. I had made a bet five years before that that I would find a new planet by Dec 31, 2004. Time was running out. I was about to lose. I hate losing. So I was searching and researching all of the pictures of the sky I had taken over the past two years hoping that maybe somewhere in those old pictures was something that I had missed. Maybe there was still a planet to be found after all. Maybe I wasn’t going to lose my bet.
Just 3 days after Christmas I came the closest I had ever come. There was something in the old images that had been missed the first time around, and it was bright. I sent email to Chad Trujillo and David Rabinowitz, the two other astronomers I worked with, saying that this new object was so bright that it might well be twice the size of Pluto. Or bigger! Being right after Christmas, we of course called the object Santa.
Santa, which now goes by the official name of Haumea, we now know to be only about ½ the size of Pluto, and we call it – and Pluto – a dwarf planet rather than a planet. But back in those last days of 2004 when the discovery was first made, we had no idea where all of it was heading.
Our understanding of the Kuiper belt has changed dramatically in these past five years. The best example of this change comes, I think, from the discovery of a large Kuiper belt object that was announced just a few days ago. For me it was a particularly surprising discovery. For the first time I was not at the receiving end of a telescope making the discovery, I was at the receiving end of an email asking me about this new object called 2009 YE7.
“Never heard of it,” I thought.
But, by decoding the numbers, I could tell it was something that had just been discovered a few days before. Like anyone else, my first attempt to know more was a quick trip to Google.
Ah ha! A new large Kuiper belt object found from a telescope Chile, by David Rabinowitz! Yes, the same David Rabinowitz from the Haumea discovery. He has moved on to Chile to try to make newer discoveries from there, discoveries in parts of the sky that we didn’t look at back when we were working at Palomar Observatory outside of San Diego.
Based on preliminary information, it looked likely the 9th largest Kuiper belt object ever found. David was clearly on to something good here.
I didn’t have time to delve into any more details because all of this had occurred as I was sitting in a movie theater waiting for the start of The Princess and the Frog with Lilah. She loved the part before the movie started because she could watch the on-screen ads. I checked my email and found out that there was a large Kuiper belt object that someone else had discovered. Then the movie started. I was itching to get more information about 2009 YE7, but I allowed my mind to drift down the bayou instead.
After the movie, though, my mind set to work on the implications of this new discovery. Based on its brightness it might well be a perfect size to test one of my new theories about medium-sized Kuiper belt objects. I feel like I now understand the largest objects, and I fear that I will never understand the smallest objects, but the middle ones are within grasp, if we can just find a few more to test some pet theories about them. For 2009 YE7 to be a good candidate for my theory we need to know if it has a moon, what color it is, and what materials are on its surface. Then we’ll see. I started thinking about where 2009 YE7 is in the sky, what telescopes I could use to point at it, how to time the observations.
Even as I was thinking these thoughts, my mind was drifting back to the discovery of Haumea exactly five years earlier. Back then, on the day of the discovery, we knew absolutely nothing. I had no good ideas about what Haumea would be like; I had no theories I was testing, no hypothesis to work out, no predictions to boldly claim. We were simply in the very early stages of exploration to see what was there. The exploration was going well! Soon after the discovery of Haumea, we tripled the jackpot by first discovering Eris – the one we now know to be larger than Pluto – just two weeks later, and then Makemake – the one we now know to be just a bit smaller than Pluto – a few months later. I felt the universe was exploding with new bright Kuiper belt objects and possibilities were endless. We didn’t know anything about what these objects were, how big they were, what they were made of, or what had happened to them. In April 2005 I still believed it possible that they were all 3 larger than Pluto and that they would eventually be called the 10th, 11th, and 12th planets.
In the five years since, we’ve learned a tremendous amount. We determined their sizes and gave up on any of the things in the Kuiper belt being planets (I lost my bet, too). We found Haumea’s two moons; we found that it had a surface that looks like an almost perfect glaze of ice; we found that it was white, again like ice, we found it elongated and spinning end over end every 4 hours, and we found a cloud of other smaller objects on similar orbits. We found that Makemake is covered in thick layers of frozen methane, that Eris is bigger and heavier than Pluto, and, most importantly, that things were beginning to make sense. We had moved from exploration to explanation. Haumea’s strange properties – and that cloud of objects in similar orbits – were all a consequence of a giant impact 4 billion years ago or so. Eris and Makemake were large enough that they should have methane on them.
With our new found knowledge even things that had been discovered earlier were finally being put in context. Quaoar is a weird combination of Haumea and Makemake. Orcus is what Makemake would look like if it were just a little smaller. Varuna is, well, Varuna is still confusing.
Mostly, though, now instead of each object being an individually mystery to be solved, each new object is a piece of a puzzle where many of the pieces have already been put into place. With only a little information, we can guess where the piece likely goes.
Which brings me back to 2009 YE7. Five years ago, its discovery would have been a thorough mystery to solve. But when I first heard of it two days ago, it was, instead, potentially the exact area of the puzzle I had been looking to fill in. I thought it was going to be that perfect medium-sized Kuiper belt object to try out my theories. I just needed some telescopes, some computers, and some time, and everything would fall into place. I thought it would be a fun month or two to try to collect and analyze the data quickly.
I was wrong. It took me about 2 minutes to figure out almost everything that there is to know about this object and its violent history.
When I finally got home and got a chance to look a little more closely (and “a little more closely” here doesn’t mean much; as of today still nothing is known about the object except for its position for about the past two weeks), I realized two things that told the whole story. First, 2009 is YE7 bright. In absolute terms, it is the 9th brightest object, which is what led to the reasonable assumption that it is likely the 9th largest object (by absolute brightness here, I mean the brightness things would have if they were all the same distance away; some objects are bright just by virtue of being close). Second, the orbit of 2009 YE7 is tilted relative to the planets by 29 degrees. Following the position of an object for only 2 weeks doesn’t give you a precise measurement of much about its orbit, but that tilt is one thing that is solidly known even with this limited data. An angle of 29 degrees is an unusually high angle. Not too many objects are tilted by that much. But one that is is Haumea. Ah! Haumea! Haumea with its family of shards all going around the sun on orbits just like it. Tilted by 29 degrees.
2009 YE7, the brightest object discovered in the Kuiper belt in almost 5 years, is almost certainly one of the large shards (perhaps even the largest) blasted off of the surface of Haumea 4 billion years ago. 2009 YE7 and the other shards have been circling the sun on their own ever since. It is bright not because it is particularly large, but because all of the fragments of Haumea have extremely bright, reflective, icy surfaces which make them stand out against the more common darker Kuiper belt objects. 2009 YE7 is not the 9th largest Kuiper belt object; it is probably about 440 km in diameter and so in the top 50.
I will admit that I miss the old Kuiper belt. I miss the mystery and wonder of exploration of unknown territories. There will be nothing like it in solar system studies for a long time to come, I suspect. Perhaps ever. And yet, as much as exploration is thrilling and exhilarating, there is something deeply satisfying about learning about a new bright Kuiper belt object while sitting in a movie with your daughter and understanding most of its 4.5 billion year history soon after getting home. We’ve learned so much. We’ve come so far.
….
A technical aside on 2009 YE7. The tilt of the orbit alone does not prove it to be a Haumea fragment, particularly since the other parameters of the orbit are still poorly known. Above, when I say it is “almost certainly” a fragment, the assessment is a judgment based on experience, rather than a scientific fact. But I’m pretty confident, sufficiently confident that I’d be willing to bet (I need to win back some of my loss from that old 2005 bet, right?). The real confirmation, though, would come from an infrared spectrum that shows evidence of deep water ice absorption features, but that requires a pretty big telescope. Almost as good, though, would be optical colors showing it to be white (solar-colored, really) like all of the other Haumea fragments. Measuring these colors is actually quite easy; all you need is a ~1 meter telescope and ~1 night of observing. Any two photometric bands would be good. I would probably just try V and R. Then measure a solar colored standard star and compare. They will be the same, I predict. Go do it! Tell me the answer! It’s fun to make predictions, and even more fun for them to come true.
…….
I don’t actually think the exploration is finished yet. The southern skies are still largely terra incognito for the Kuiper belt. David Rabinowitz has clearly just started the journey; others are scanning out there, too. Much of what they find may indeed fit into the frame of the puzzle that we already know, but I still hope some day to open up some email and read about some new discovery and sit stunned realizing that someone just found something that I didn’t expect at all.
Book Excerpt: Who Ordered This Truckload of Dung?
On allowing ourselves to see our mistakes as unique features of ourselves.
We’re the Government — and You’re Not
Peek-a-moon | Bad Astronomy
I don’t have a whole lot to add to this amazing shot from Cassini of Saturn’s moon Rhea reappearing from behind the giant moon Titan:
[Click to entitanate.]
Except: coooool. Titan is over three times the size of Rhea, and Rhea was more than twice as far from Cassini when this was taken, making Rhea look even smaller in comparison. Also, check out how the high-altitude haze in Titan’s atmosphere isn’t the same height all the way around the moon. Near the top you can see they poof up higher. If you look closely, can you see the Enterprise?
Code Protecting 80 Percent of Cellphone Convos Finally Cracked | 80beats
Are your phone conversations about to become less secure? A German encryption expert says he’s cracked the two-decade-old algorithm that protects most of the world’s cellphones: GSM (Global System for Mobile communication).
Karsten Nohl says his intentions were noble; he wanted to show the world that though GSM protects 80 percent of the cellphones in the world, it’s far from invincible. “This shows that existing G.S.M. security is inadequate,” Mr. Nohl, 28, told about 600 people attending the Chaos Communication Congress, a four-day conference of computer hackers that runs through Wednesday in Berlin. “We are trying to push operators to adopt better security measures for mobile phone calls” [The New York Times].
Nohl and a team of others had been working independently since August to hack the code. Developed in 1988, the system prevents the interception of calls by forcing phones and base stations to change frequencies constantly [The Guardian]. Nohl and the others generated countless random code combinations until they’d completed an encryption code book. As an analogy, think of encryption like a jigsaw puzzle where you have to find one specific puzzle piece. If the puzzle only has 25 pieces, it won’t take you too long to accomplish. That is like a weak encryption algorithm. However, if the puzzle has 10,000 pieces it will take significantly longer [PC World].
Despite the fact that it took 21 years before someone figured out their jigsaw puzzle, GSM’s creators at the GSM Association aren’t pleased. “We consider this research, which appears to be motivated in part by commercial considerations, to be a long way from being a practical attack on GSM,” said Claire Cranton, a spokeswoman. “To do this while supposedly being concerned about privacy is beyond me” [The Guardian].
While Nohl claims his works was academic and GSM spokespeople say it’s not a threat, not everyone is convinced it’s so harmless. Law enforcement officials and well-financed cyber criminals have been able to crack GSM encryption for sometime, but the investment was so high that it didn’t pose much of a threat. This new method lowers the price of entry to the point that it is more of an issue, but still not a high risk [PC World].
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Image: flickr / Ed Yourdon
Specially Modified Music Can Rewire Brain & Alleviate Tinnitus | 80beats
Tinnitus, the perceived ringing and buzzing in one’s ears, may not be fully understood, but what is known is that it can severely disrupt a person’s life. Treatment for the condition has been unreliable, but now scientists are reporting a new way to turn down the ringing by turning up music, according to a new study.
Scientists altered participants’ favourite music to remove notes which matched the frequency of the ringing in their ears. After a year of listening to the modified music, individuals reported a drop in the loudness of their tinnitus [BBC News]. Participants who listened to music in which notes of a different frequency were removed reported no such improvement. The treatment could be a cheap way to help the three percent of the population that suffers from tinnitus, say the researchers, who published their findings in the Proceedings of the National Academy of Sciences.
The idea is to remove the spectrum of noise linked to tinnitus from the music a person listens to so that the area of the brain associated with that frequency will not be as active. The researchers propose that the therapy might work by re-wiring parts of the auditory cortex that have become over-active to instead tune into surrounding—but different—tones. Another possibility is that with deprivation, these specially tuned auditory neurons would undergo “long-term depression,” causing them to become less active overall [Scientific American]. How ironic that one of the causes of ringing ears may also be the solution.
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Image: flickr / Neil T
Free Tropical Vacation! (If You Try an Experimental Diarrhea Drug) | Discoblog
It’s about that time of year when people return home from spending holidays with the family, only to realize they need a vacation to recover from their vacation. Well, if you’re a resident of the U.K. or Germany who’s in good health, between 18 and 64 years old, and can keep a diary for two and a half weeks, your vacation to Mexico or Guatemala could be gratis. Oh, and one more thing: You have to be a guinea pig for a potential diarrhea drug.
A U.S. vaccine manufacturer called Intercell calls it the “Trek Study.” The company says it needs 1,800 volunteers between now and May to visit these locales, where sun-seeking tourists often get diarrhea. But fear not, travelers: A smaller study Intercell did on Americans showed a 75 percent reduction in diarrhea incidence, so perhaps fewer of you will spend your Caribbean holiday in excruciating, gut-wrenching pain than you normally would.
From BBC News:
Intercell’s clinical director, Nigel Thomas, told the UK’s Independent newspaper: “We are looking for people who have already planned to go to Mexico or Guatemala and think this would add another interesting aspect.
“It is almost like going on a package holiday. They will be met by a concierge who will take them to their hotel and arrange for them to give their first blood sample within 48 hours.”
Fake leprosy, it seems, isn’t the only way to snag a medical vacation in the tropics.
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DISCOVER: Megadeath in Mexico
Image: flickr / lightmatter
Halfway to Pluto! | Bad Astronomy
Today, December 29, 2009, the New Horizons Pluto probe crosses an arbitrary but psychologically important line: it is now closer to Pluto than it is to Earth.
If there were people on board the small interplanetary probe, no doubt they’d be popping champagne. I’m sure that back on Earth, the team behind NH are pretty happy. This probe has a checkered history, having been planned, canceled, re-planned, delayed, on and on. It’s amazing it got to launch at all. But on January 19, 2006 the small, half-ton probe was sent on its way, and on July 14, 2015 it’ll sail past Pluto and its collection of moons, snapping pictures and taking data.
Today marks the official halfway point, where New Horizons has half its path already behind it. Here’s a plot of its distance to Earth (in blue) and Pluto (red) care of the New Horizons site:
Distance in the graph is measured in Astronomical Units (a yardstick used by astronomers for convenience; it’s the distance of the Earth to the Sun, about 150 million km (93 million miles)). The distance to Earth is wiggly because the Earth goes around the Sun as New Horizons moves out, and the distance to Pluto decreases steadily as the spacecraft catches up on its journey. Where the two lines cross is where the distances are equal, and that’s now, today!
You may be wondering about the timing: New Horizons is halfway in distance to Pluto, but the mission timeline halfway point isn’t until October 16, 2010 (if I’ve done the math correctly). The probe was launched at high speed, slowed down due to the Earth’s and Sun’s gravity, picked up a kick from Jupiter in early 2007, and has been slowing ever since. Since it was moving faster before, it reached the distance halfway point before the schedule halfway point.
New Horizons is now 16.37 AU – 2.449 billion km, or 1.522 billion miles — from home. But maybe now, home is no longer Earth. Once it crossed that line today, home became deep space. Even Pluto and its moons Charon, Nix, and Hydra are only milestones for it. It won’t be stopping when it gets there; New Horizons will sail on by, continuing into deep space. It’ll become one of several other spacecraft we’ve sent out of the solar system itself, set to wander interstellar space forever.
That is, unless one day we catch up to them ourselves. I imagine in a few hundred years they’d make fine museum pieces. Or maybe, if poetry still exists in humans all those far-flung centuries from now, we’ll let those probes continue on. I rather like that idea better.
You can follow the New Horizons probe on Twitter, which is how I found out about this milestone today.
Art credit: ESO/L. Calçada
Fermi smooths out space | Bad Astronomy
This news came out a little while ago but I didn’t cover it at the time, and it’s cool enough that it deserves to be covered. I got it from my friends with NASA’s Fermi satellite outreach group. I used to work on Fermi outreach before the satellite launched and was still called GLAST (Gamma-ray Large Area Space Telescope), and it was fun trying to come up with lesson plans and educational efforts based on gamma rays (the Hulk came up a lot).
Anyway, one thing Fermi can do is measure the exact time when high-energy gamma rays hit its detectors. Not too long ago, photons from a distant explosion slammed into Fermi, and it found that all these photons arrived essentially simultaneously from the event, irrespective of their energies.
So what? So, Einstein was right. Check it out for yourself:
Basically, the idea is that some quantum mechanics theories propose that space is irregular, foamy, and bumpy on incredibly small scales, and this means the speed at which photons travel may change very slightly if they are more or less energetic. The difference is so small that it takes very long trips to detect it — imagine two cars traveling at 50 versus 50.5 kph: after a few seconds you’ll hardly see any difference, but over an hour they’re separated by half a kilometer. So the longer the trip, the easier it is to measure.
After 7 billion years, if those specific QM theories are right, two photons should arrive at very different times, but Fermi found that the high energy gamma rays hit Fermi less than a second after the low energy ones. This means that space really is smooth, or at smooth at scales smaller than predicted by those quantum theories. QM is still a solid model for the Universe — after all, solar panels, computers, and nuclear bombs do work — but this means that we need to rethink certain aspects of them.
I love hearing stuff like this. We have lots of ideas on how the Universe works, but we need observations of the Universe to know if we’re traveling down the correct path or not. Fermi has shown us that some of these paths lead to dead ends, and we need to look elsewhere for our journey to continue. And I will guarantee that not only will that journey go on, but we’ll find ever-more roads to investigate as we travel.
Good Things In Small Packages
CU Students to Build Tiny Spacecraft to Observe 'Space Weather' Environment
"The University of Colorado at Boulder has been awarded $840,000 from the National Science Foundation for students to build a tiny spacecraft to observe energetic particles in space that should give scientists a better understanding of solar flares and their interaction with Earth's atmosphere. Known as the Colorado Student Space Weather Experiment, or CSSWE, the instruments package is expected to weigh less than 5 pounds."
Scott Brown for US Senate – Massachusetts: New TV Ad
Special Election - Ted Kennedy seat
It's being hailed as perhaps the most brillant political TV ad ever. But is it enough to propel Republican Brown to the US Senate from deeply Democrat Massachusetts?
New Moon Marvels
The Cassini orbiter has been working overtime during the holidays to deliver a cartload of gifts from Saturn and its moons. Highlights include fresh views of frost-spewing Enceladus and yam-shaped Prometheus, plus a "Nutcracker"-style ballet of Saturnian satellites. The excitement began last week with the animated images of moonsimage advisory, the folks who process Cassini's pictures compared the interplay to the dance of the Sugar Plum Fairy from Tchaikovsky's "Nutcracker" ballet. passing back and forth with the giant planet and its rings as a backdrop. In an
My favorite movie is "Moon Jumble," which has Rhea in the starring role, joined by its siblings Janus, Mimas and Pandora. (That's the real Pandora, not the fictional "Avatar" moon). Make sure you stretch your browser window wide enough to take in the whole picture.
"As yet another year in Saturn orbit draws to a close, these wondrous movies of an alien place clear across the solar system remind us how fortunate we are to be engaged in this magnificent exploratory expedition," imaging team leader Carolyn Porco said. "So, from all of us on the Cassini Imaging Team to all of you, Happy Holidays!"
That might fool you into thinking the Cassini team was taking the holidays off. There's no way that was going to happen. On Christmas and the day after, the orbiter snapped pictures as it flew past Enceladus and Prometheus. Over the weekend, Cassini zoomed within 600 miles (960 kilometers) of Titan's north pole.
A sampling of the raw imagery released on Sunday includes a striking full-disk view of Enceladus and its geysers of water ice, spewing out from southern fissures that have been nicknamed "tiger stripes." Such geysers hint at the existence of a subsurface ocean beneath Enceladus' icy surface - an ocean that just might harbor alien life.
The latest picture was taken from a distance of 383,000 miles (617,000 kilometers), and it might make you wonder why those geysers hadn't been spotted decades ago when the Voyager spacecraft flew past. In a posting to the imaging team's Web site, Porco says it wouldn't have been that easy for Voyager to spot the frosty spray.
"We never got a good look at the southern hemisphere with Voyager; we even missed the tiger stripes back then," she wrote. Porco also said "some of the jets - and maybe all of them - are 'intermittent' in the sense that we expect they could turn on and off on a daily timescale (where 'daily' here means 1.3 Earth days)."
Another raw image provides the best view yet of Prometheus, a "shepherding" moon that along with Pandora helps keep Saturn's F ring in line. This view was captured from a distance of 36,000 miles (59,000 kilometers). A farther-out image from Cassini, released five years ago, shows Prometheus at work.
The Planetary Society's Emily Lakdawalla put together the raw imagery to produce a natural-color composite photo of the moon, which measures 74 miles long and as little as 38 miles wide (119 by 87 by 61 kilometers).
"This is one of the more elongated moons to be seen in the solar system, almost exactly twice as long as it is wide," Lakdawalla observes. "The word 'potato' is commonly used to describe the shape of small bodies in the solar system, but I think that Prometheus, with its pointy ends, looks more like a related vegetable, a yam."
The fact that candied yams are a traditional holiday dish makes Prometheus even more palatable as a year-end picture - and whets the appetite for more from Cassini in the year to come.
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North Carolina Democrat Senate leader, resigns over Shooting incident and alleged Sex scandal
From Cliff Thies:
After a grand jury indictment for shooting a 22-year old man, North Carolina state Sen. R.C. Soles, a Democrat, said he will not seek re-election next year. A criminal attorney, Soles apparently maintained close relations with his former clients. He says this was to ease them back to a law-abiding life and denies it was because he was having sexual relations with them. Soles is the latest in a string of senior Democrats in the state legislature that are stepping down.
Soles, from Tabor City, is the State's longest serving legislator.
From the Raleigh News & Observer, Dec. 30:
Soles long was at the center of grumbling in his hometown of Tabor City about young men who were former legal clients and hung around his home or law office.
In the August incident, Soles shot 22-year-old Thomas Kyle Blackburn, who was allegedly trying to kick in Soles' front door.
Soles' lawyer, Joseph Cheshire of Raleigh, has said the shooting was self-defense. Cheshire and Soles repeatedly have said that Soles has been generous to former clients in hoping to ease them back to a law-abiding life. Soles has denied having sexual relations with any of the young men.
An NC political blog out of Wilmington - Clean it up Dammit - which regularly covers corrupt politics in the region has more details:
The boy, a 16 year old kid with some troubles that the good senator helped to deal with, told the senator that he would go to the news with stories that would ruin the senator's career. The Senator had the kid, Allen Strickland, arrested and the kid said, "see you in prison"
(Photo of the 16 year old accuser at the Clean it up blog.)
