by iamlucky13 » Mon Oct 16, 2006 6:08 pm
Presumably, the mass that is "boiling away" is doing so because it is gaining kinetic energy from the star's radiation. The KE of the remaining mass should be unaffected...I would think. Also, I think the discussion of gas boiling away is not due to observations, but due to computer modelling of these hot Jupiter systems, but it seems like a very reasonable result.
Astro_uk, you raise an interesting point about friction. I believe gas giants are not expected to be able to form this close to star. Instead, they form at greater distances and migrate inward. I don't remember the proposed mechanism, but I think it was either friction in the still-condensing accretion disk.
Presumably, the mass that is "boiling away" is doing so because it is gaining kinetic energy from the star's radiation. The KE of the remaining mass should be unaffected...I would think. Also, I think the discussion of gas boiling away is not due to observations, but due to computer modelling of these hot Jupiter systems, but it seems like a very reasonable result.
Astro_uk, you raise an interesting point about friction. I believe gas giants are not expected to be able to form this close to star. Instead, they form at greater distances and migrate inward. I don't remember the proposed mechanism, but I think it was either friction in the still-condensing accretion disk.