It seems that astrometry has finally succeeded at detecting a planet. A star and its planets perform a complex dance as they move through space. In astrometry planet hunting one looks for a planet by looking for the "wobble" of a star as it moves across the sky. This is contrast with the two other methods used to detect planets around stars, which use radial velocity or transits to detect the planets. Now it seems that a team from JPL has used a series of measurements over 12 years to detect a Jupiter sized planet tugging on its star, VB 10. The wobble in this case is a movement of about one sixth of an arcsecond per year. Very cool.
The Quantum Pontiff
Theoretical Musings
Search

Profile
Dave Bacon is a theoretical ski bum who is also a pseudo professor. His research is on quantum computing, his scientific passions extend to everything in physics, mathematics, computer science and beyond, and his personal pleasures include making wine, playing poker, skiing, camping, and daydreaming (although not all of those at the same time.)
Nothing he says on this blog should be construed as having anything to do with his employer or his dog.
Recent Comments
- Neil B on So Long and Thanks For All the Fish!
- Si-Hui Tan on Ecto and LaTeXiT
- evden eve nakliyat on Google Hella Cool
- Peter Lund on Google Hella Cool
- wolfgang on So Long and Thanks For All the Fish!
- Rod on So Long and Thanks For All the Fish!
- Art on So Long and Thanks For All the Fish!
- John Sidles on Dead Spins And The Dirty Ground
- Jonathan Vos Post on Dead Spins And The Dirty Ground
- John Sidles on Dead Spins And The Dirty Ground
Recent Posts
- So Long and Thanks For All the Fish!
- Dead Spins And The Dirty Ground
- Bacon Camp
- Best Paper at STOC
- Pr(Future Dave Bacons|Library Cuts) is Small
- De Took Er DataBs Jrbs!
- Google Hella Cool
- Portrait of a Reviewer as a Young Man
- Theory Matters Vision Nuggets
- What To Do With Scirate?
Other Information
Cows are well approximated by a sphere.

« Online Weekly Colloquia? | Main | When Tomorrow Was Yesterday »
Astrometry Finds Planet
Category: Astronomy
Posted on: May 28, 2009 3:02 PM, by Dave Bacon
TrackBacks
TrackBack URL for this entry: http://scienceblogs.com/mt/pings/111074
Click here to search for this post on the new blog.


Comments
http://www.sciencedaily.com/releases/2009/05/090528141509.htm
... The newfound exoplanet, called VB 10b, is about 20 light-years away in the constellation Aquila. It is a gas giant, with a mass six times that of Jupiter's, and an orbit far enough away from its star to be labeled a "cold Jupiter" similar to our own. In reality, the planet's own internal heat would give it an Earth-like temperature.
The planet's star, called VB 10, is tiny. It is what's known as an M-dwarf and is only one-twelfth the mass of our sun, just barely big enough to fuse atoms at its core and shine with starlight. For years, VB 10 was the smallest star known -- now it has a new title: the smallest star known to host a planet. In fact, though the star is more massive than the newfound planet, the two bodies would have a similar girth....
Because the star is so small, its planetary system would be a miniature, scaled-down version of our own. For example, VB 10b, though considered a cold Jupiter, is located about as far from its star as Mercury is from the sun. Any rocky Earth-size planets that might happen to be in the neighborhood would lie even closer in.
Posted by: Jonathan Vos Post | May 29, 2009 2:26 PM
thanks it it the topic
Posted by: zayıflama | May 29, 2009 2:44 PM