Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution
id:
extreme-ultraviolet-stellar-characterization-for-atmospheric-physics-and-evolution-263-1074951
title:
Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution
text:
The Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (ESCAPE) mission aims to find environments beyond Earth's solar system that might host planets with thick atmospheres to support life. The long-term stability of exoplanetary atmospheres depends critically on the extreme-ultraviolet (EUV) flux from the host star. The EUV flux likely drives the demographics of the short-period planet population as well the ability for rocky planets to maintain habitable environ
brand slug:
wiki
category slug:
encyclopedia
description:
original url:
https://en.wikipedia.org/wiki/Extreme-ultraviolet_Stellar_Characterization_for_Atmospheric_Physics_and_Evolution
date created:
date modified:
2023-08-13T07:39:19Z
main entity:
{"identifier":"Q106311249","url":"https://www.wikidata.org/entity/Q106311249"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/c/c9/ESCAPE_spacecraft_render_2.png","width":1920,"height":1080}
fields total:
13
integrity:
14