Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Exosphere
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
===Upper boundary=== [[File:IBEX ENA Feature FInal Fig3.jpg|thumb|Earth's exosphere, [[energetic neutral atoms]] (ENA) and [[magnetosphere]].]] In principle, the exosphere covers distances where particles are still [[Gravity|gravitationally]] bound to [[Earth]], i.e. particles still have ballistic orbits that will take them back towards Earth. The upper boundary of the exosphere can be defined as the distance at which the influence of solar [[radiation pressure]] on atomic [[hydrogen]] exceeds that of Earth's gravitational pull. This happens at half the distance to the Moon or somewhere in the neighborhood of {{convert|200,000|km}}. The exosphere, observable from space as the [[geocorona]], is seen to extend to at least {{convert|100,000|km}} from Earth's surface.<ref>{{cite web| url=https://scied.ucar.edu/learning-zone/atmosphere/exosphere#:~:text=Since%20the%20exosphere%20gradually%20fades,about%20halfway%20to%20the%20Moon.|title=The Exosphere|website=University Corporation for Atmospheric Research|access-date=October 5, 2022}}</ref>
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)