Discussion about this post

User's avatar
beingreleased's avatar

The first extrasolar planets that were found were called Hot Jupiters. They were basically Jupiter-sized planets very close to the stars - their orbits were only a few days. They are thought to have formed farther out from the star and then moved inwards. When a star is young, it has a gas disk - interactions between the disk and the planet cause the planet to spiral inwards (it's kind of like a frictional interaction). The disk doesn't go all the way to the star, just close, so the planet doesn't get eaten up by the star. When the star gets older, the disk goes away.

Most of the first planets found were like this because they were the easiest to find: massive, short period planets were favored by the detection techniques. Since then we've discovered thousands of planets and solar systems similar to ours are much more common.

As far as the atmospheres part, atmospheres are complicated. It kind of makes sense that our atmosphere is like it is, but I wouldn't say it has to be like that.

Just a side note: the first extrasolar planet was discovered in 1995 - not that long ago. The field has progressed incredibly in that time. The Kepler mission, which sadly is likely to end any day now (out of fuel), found thousands of planets and TESS, which just launched, will find lots more.

Expand full comment
193 more comments...

No posts