Impressive results released today show just how much we're learning about the 'hot Jupiters' that comprise about a quarter of known exoplanets. The first concern HD 149026b, a distant world which the infrared Spitzer instrument has shown to be the hottest planet ever studied. It's somewhat smaller than Saturn but more massive, and is thought to contain more heavy elements than could be found in our entire Solar System outside the Sun itself, with a core as much as 90 times the mass of the Earth. And the odd thing about HD 149026b is that for it to reach the measured temperature -- a smoking 3,700 degrees Fahrenheit, or 2,300 degrees Kelvin -- it would have to be absorbing just about all the starlight reaching it. The upshot is a planet whose surface is blacker than charcoal, re-radiating incoming energy in the infrared. What a view for the nearby traveler: "The high heat would make the planet glow slightly, so it would look like an ember in space, absorbing all incoming light but...
Twilight of a Supernova
The thought that Eta Carinae, a star at least 100 times more massive than the Sun, is a ticking time bomb seems to infuse much of the coverage about the huge supernova recently observed by the Chandra X-ray Observatory. And you can see why. Big explosions are marketable, which is why it sometimes seems that one way to categorize many of today's movies is by how many cars were blown up during the making of them. When you're talking about something a hundred times larger than the typical supernova, you're going to get attention. What if a star 100 times the size of the Sun -- or larger -- goes off in our neighborhood? Adding to the comparison is the fact that the supernova, known as SN 2006gy, seems to have expelled a large amount of material before the catastrophe. Eta Carina also shows signs of expelling mass, and it's 7500 light years away, vs. the 240 million light years of SN 2006gy. Close enough to cause us problems? I don't know the answer, but it does seem clear that one result...
A New Vision for Space
History teaches that when big operations falter, small upstarts often rise to the challenge. In the case of NASA, the process may already be at work, and the upstarts are emerging: SpaceX, Blue Origin, Virgin Galactic. Out in the wilds of Las Cruces, New Mexico is building a spaceport. In fact, says Russell Saunders, Jr., the time has come to consider contingency plans. 'Saunders' is a pseudonym for a space scientist who works for a major aerospace organization. His essay appeared this afternoon on the NASA Watch site. Saunders believes NASA is fixated on an iconography that's half a century old, referring back to the spectacular space series that ran in Collier's magazine in the early 1950's. These were glorous, von Braunian visions of enormous rockets and flotillas of spacecraft pushing outward to Mars, but they're an uncomfortable fit with today's realities. Here's what Saunders is talking about: Imagine what the artists and pioneers behind the Colliers vision might have done with...
NIAC’s Contributions and the Future
The news that NASA intends to close its Institute for Advanced Concepts has many in the space community concerned, and Centauri Dreams' comment on the matter was but one of many to fill the Net when the news broke in March. Now, however, there appears to be at least an attempt to keep the Institute alive. People who have had some connection with NIAC are being asked to step in with demonstrated benefits from its activities. That news comes via this post on the Space Elevator Blog, as passed along by Joseph Mahaney. I've just confirmed it with sources inside NIAC. Here are the areas for which contributions are solicited: Subsequent investment by NASA, other government agencies, or the private sector. Intellectual contributions that have resulted in an agency putting resources into its own studies of a concept. For example, prompted by the success of a Phase I or Phase II concept, an agency convenes panels to study the work or otherwise funds studies of its own. Unexpected spin-off...
On Wally Schirra
I wish I had something profound to say about Wally Schirra. But when I think about him, what I get instead are moments. Great moments. I remember watching Schirra's Atlas booster muscling Sigma 7 downrange that day in 1962. A space-struck kid, I thought the astronaut was as cool and unflappable as any man who would ever ride a rocket. His sense of humor was irrepressible, especially in the context of hazardous early space missions. Thus the 'Jingle Bells' moment on the harmonica, and his sighting of the 'UFO' -- Santa Claus and his reindeer. "We have an object, looks like a satellite going from north to south, probably in polar orbit... I see a command module and eight smaller modules in front. The pilot of the command module is wearing a red suit..." Tom Stafford was in on that gag on Gemini 6 (he would later go on to command Apollo 10). I was in college when Apollo 7 flew and recall the squabbles with controllers on the ground. To be fair, Schirra had a cold, a famous one that he...
COROT’s First Exoplanet
The early news from COROT couldn't be more encouraging. Just sixty days into its science mission, the spacecraft has found its first transiting exoplanet and has returned information about the interior of a star. The latter findings point to COROT's role in asteroseismology, the study of stellar interiors through analysis of the star's light curves. What has mission scientists smiling is that in both cases, the instruments they're watching show signs of working even better than planned. True, the data carrying these results are still noisy and in need of plenty of analysis, but COROT project scientist Malcolm Fridlund sounds quite an optimistic note: "The data we are presenting today is still raw but exceptional. It shows that the on-board systems are working better than expected in some cases - up to ten times the expectation before launch. This will have an enormous impact on the results of the mission." One would think so. It raises the stakes for COROT from detecting...
HAT-P-2b: ‘A Really Weird Planet’
Last night I was thinking that the day would come when all the planets we've been discovering have proper names instead of stark designations in catalogs. Then I realized that this is unlikely. As the rate of planetary discoveries accelerates through space-borne missions and ever more precise detection methods here on Earth, it may be that we'll keep generating new finds faster than the naming process can catch up with them. So I guess we should get used to designations like Gliese 581 c. Of course, a planet can have multiple designations, depending on how it's catalogued or found. The recently announced gas giant HAT-P-2b (a very strange place indeed) is called this not for its place in a catalog but its discovery method, the HAT network of automated telescopes. HAT stands for Hungarian-made Automated Telescope, but the project is headquartered at the Harvard-Smithsonian Center for Astrophysics (CfA) and works with instruments in Arizona, Hawaii and in this case, Israel. Its focus:...
Calculating How Stars Age
We need to know more about how stars age. Ponder this: Centauri A and B are perhaps 2.5 billion years older than our Sun. If we're interested in the development of intelligent life, older is clearly better -- who knows what Earth might develop in the next two billion years? But are there planets around either of the primary Centauri stars? And if there are, how have their planetary systems changed over the course of those milennia? Addendum: See the comments below -- my figure of 2.5 billion years older than the Sun is in the middle of more extreme age estimates in both directions, and even these are questioned by the work we discuss in the following paragraphs. One way to study these things is by looking at how stars rotate. A recently announced method called gyrochronology works with the premise that a star's age is tightly bound up with both its rotation and its color. Syndey Barnes, who developed the technique at Lowell Observatory, explains it this way: "If you know the...
Death of an Astrophysicist
Bohdan Paczynski, the Princeton astrophysicist who died April 19, was a major contributor to the exoplanet hunt, fine-tuning the techniques used in gravitational microlensing. Coming to Princeton in 1982 after twenty years at Warsaw's Copernicus Astronomical Center, Paczynski understood early on that the bending of light by foreground objects, predicted by Einstein, could be applied to surveying stars in our own galaxy. A star passing directly in front of another can focus the light from the background star, producing a natural lens that allows investigation of objects otherwise impossible to observe. The consortium of scientists that Paczynski led would go on to found the Optical Gravitational Lensing Experiment (OGLE), now active at Chile's Las Campanas Observatory. Says Michael Strauss, a professor of astrophysical sciences and a colleague of Paczynski's: "The next thing Bohdan realized was that when you observe lensing that often, you can do other clever things, such as use it to...
‘Asia Emerging’: The Director’s Cut
Having had time to decompress from their exhausting Asian trip, Gregory and Elisabeth Benford have revised and enlarged the account of their travels that Centauri Dreams published in late March. The text contains numerous additional insights, but what makes this revision truly stand out from the original post are the photographs, fully seven times the number first published, each illustrating a unique facet of their journey. I've inserted the new Asia Emerging in the archives. Don't miss its unforgettable images and insights into a part of the world that will have much to say about our future on this planet. I told Gregory that my favorite photograph is the one of him at the Raffles Hotel in Singapore, Singapore Sling in hand. Shades of Somerset Maugham...
Philosophia Naturalis #9 Online
Philosophia Naturalis #9 has just become available, with numerous links to stories on the Gliese 581 c discovery and intriguing looks at everything from quantum mechanics to gamma ray bursts. Nobody can keep up with all the weblogs out there, which is why a blog 'carnival' like this one is must reading to see how the latest findings play among scientists and laymen alike (this is where I discovered Clifford's Johnson's Asymptotia, itself a sufficient reason to keep reading in hopes of future finds). Hosted this month by Science and Reason, the carnival moves from site to site with each new edition, none of which are to be missed.