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730.5 (dbd:day) |
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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 environments long enough for the emergence of life. ESCAPE is an astrophysics Small Explorer proposed to NASA that employs extreme- and far-ultraviolet spectroscopy (80 – 1650 Å) to characterize the high-energy radiation environment in the habitable zones (HZs) around nearby stars. (en) |
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ESCAPE (en) |
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dbr:Ball_Aerospace |
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dbr:National_Aeronautics_and_Space_Administration |
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dbr:Extreme_Ultraviolet_Explorer |
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wiki-commons:Special:FilePath/ESCAPE_spacecraft_render_2.png?width=300 |
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dbr:Stellar_corona dbr:Circumstellar_habitable_zone dbr:Ultraviolet_astronomy |
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https://escapetelescope.org/ https://lasp.colorado.edu/home/cusp/escape/ https://lasp.colorado.edu/home/cusp/escape/%7C https://www.nasa.gov/press-release/nasa-selects-proposals-to-study-volatile-stars-galaxies-cosmic-collisions%7Ctitle=NASA |
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| dbp:date |
2021-03-25 (xsd:date) |
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Render of ESCAPE spacecraft (en) |
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230 (xsd:integer) |
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File:ESCAPElogo.png (en) |
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ESCAPE mission logo (en) |
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2025 (xsd:integer) |
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dbr:Ball_Aerospace |
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Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (en) |
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ESCAPE (en) |
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dbr:National_Aeronautics_and_Space_Administration |
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dbr:Low_Earth_Orbit |
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256.0 (dbd:watt) |
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dbr:Extreme_Ultraviolet_Explorer |
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dbr:Explorers_program |
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lasp.colorado.edu (en) |
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https://lasp.colorado.edu/home/cusp/escape/%7C |
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Ball Configurable Platform (en) |
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Gregorian telescope, grazing incidence (en) |
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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. (en) |
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Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (en) |
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Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (en) |
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