|
| If this is your first visit, be sure to check out the FAQ by clicking the link above. You may have to register before you can post: click the register link above to proceed. To start viewing messages, select the forum that you want to visit from the selection below. |
|
|||||||
| Register | FAQ | Members List | Calendar | Mark Forums Read |
![]() |
|
|
LinkBack | Thread Tools | Search this Thread | Display Modes |
|
|||
|
I was reading some information about the Sun and I came across something that confused me. (I am only listing the portion I found confusing.) The diagram/explanation of each layer of the sun gave these stats. Radiative, 5,000,000 K; Convection, 5,800 K; Photosphere, 4,400 K - 6,600 K; Chromosphere, 30,000 K.
How does the temperature go from hot to cooler and back to hotter again? Why are the outter temperatures so much hotter than the "middle" regions?
__________________
Calvin: Sometimes when I'm talking, my words can't keep up with my thoughts. I wonder why we think faster than we speak. Hobbes: Probably so we can think twice. ~Calvin & Hobbes~ |
|
||||
|
Quote:
Here is a short answer. This has a little more. It's been a while since I've seen anything new on this phenomenon, but it is quite interesting.
__________________
"A mystic is a person who is puzzled before the obvious but who understands the nonexistent." -- Elbert Hubbard |
|
|||
|
Wait until you try to find the magnetic poles. #-o If you think that one is hard check out the actual rotation.
![]()
__________________
My initials are on the moon, my name is on Mars and Earth is my planet of origin. |
|
||||
|
Quote:
|
![]() |
| Thread Tools | Search this Thread |
| Display Modes | |
|
|