It's sciencey!
Oct. 16th, 2006 07:54 pm![[personal profile]](https://www.dreamwidth.org/img/silk/identity/user.png)
1. Backlit Saturn.
2. Ununoctium, the noble gas after radon.
3. This Wikipedia featured picture showing Lorentz transformations in action is really clever.
2. Ununoctium, the noble gas after radon.
3. This Wikipedia featured picture showing Lorentz transformations in action is really clever.
no subject
Date: 2006-10-16 11:59 pm (UTC)no subject
Date: 2006-10-17 01:30 am (UTC)no subject
Date: 2006-10-17 01:37 am (UTC)no subject
Date: 2006-10-17 01:43 am (UTC)no subject
Date: 2006-10-17 01:45 am (UTC)no subject
Date: 2006-10-17 03:29 am (UTC)I'm not sure I understand
Date: 2006-10-17 05:27 am (UTC)Re: I'm not sure I understand
Date: 2006-10-17 11:50 am (UTC)The sun is directly behind the planet. Everything we're seeing is forward-scattered light. We can't see through the planet but we can see through the rings in some places. The viewpoint is above the rings, and the part of the rings right in front of the planet is further darkened by Saturn's shadow on the rings, which is why there's such a pronounced boundary at the limb of Saturn.
Re: I'm not sure I understand
Date: 2006-10-17 11:52 am (UTC)but look at the discontinuities
Date: 2006-10-17 01:36 pm (UTC)EXCEPT! now I see that all the lines in the middle of the rings DO line up. The outer edge just seems to fade into oblivion in the more diffuse light. But I'm still baffled by what I thought was an image of the inner edge, the uppermost section of the bright band across the middle of the planet.
Re: but look at the discontinuities
Date: 2006-10-17 06:40 pm (UTC)I think that's a combination of the rings, and the ring-light illuminating the surface of the planet itself. The relatively sharp dark line across the equator is there because the rings block most of the light reflected off them when seen edge on, so the clouds along the equator get less ring-light.