About: Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution

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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.

Attributes	Values
rdf:type	Thing schema:Event dul:Event societal event wikidata:Q1656682 wikidata:Q2133344 event space mission
rdfs:label	Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (en)
rdfs:comment	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)
foaf:name	Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (en)
foaf:homepage	https://escapetelescope.org/ https://lasp.colorado.edu/home/cusp/escape/
name	Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (en)
foaf:depiction
dcterms:subject	Astronomical surveys Satellites orbiting Earth Explorers Program Proposed spacecraft
Wikipage page ID	67130324 (xsd:integer)
Wikipage revision ID	1033942802 (xsd:integer)
Link from a Wikipage to another Wikipage	Pennsylvania State University University of California Berkeley University of Colorado Boulder Stellar classification Low Earth Orbit NASA Coronal mass ejection Laboratory for Atmospheric and Space Physics Smithsonian Astrophysical Observatory Stellar corona Kevin France Microchannel plate detector Exoplanet atmosphere Extreme Ultraviolet Explorer Solar flare Astronomical surveys Satellites orbiting Earth James Webb Space Telescope Explorers Program Proposed spacecraft Large Ultraviolet Optical Infrared Surveyor Marshall Space Flight Center Circumstellar habitable zone Gregorian telescope Explorers program National Aeronautics and Space Administration Mikulski Archive for Space Telescopes Solar energetic particles Extreme ultraviolet Ultraviolet astronomy LASP Ball Aerospace
Link from a Wikipage to an external page	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
sameAs	Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution
telescope type	Gregorian telescope, grazing incidence (en)
telescope wavelength	80 (xsd:integer) 1280 (xsd:integer)
dbp:wikiPageUsesTemplate	dbt:Space_observatories dbt:Cite_web dbt:Convert dbt:Infobox_spaceflight dbt:More_citations_needed dbt:Portal_bar dbt:Reflist dbt:Use_American_English dbt:Use_dmy_dates dbt:Dual dbt:Explorer_program dbt:Future_spaceflights
thumbnail	wiki-commons:Special:FilePath/ESCAPE_spacecraft_render_2.png?width=300
sourcepath	https://lasp.colorado.edu/home/cusp/escape/%7C
date	2021-03-25 (xsd:date)
image caption	Render of ESCAPE spacecraft (en)
image size	230 (xsd:integer)
insignia	File:ESCAPElogo.png (en)
insignia size	230 (xsd:integer)
launch date	2025 (xsd:integer)
manufacturer	Ball Aerospace
mission duration	6.31152E7 (second)
mission type	Stellar corona Circumstellar habitable zone Ultraviolet astronomy
names list	ESCAPE (en)
operator	National Aeronautics and Space Administration
orbit reference	Low Earth Orbit
power	256.0 (watt)
previous mission	Extreme Ultraviolet Explorer
programme	Explorers program
source	lasp.colorado.edu (en)
spacecraft bus	Ball Configurable Platform (en)
website	https://escapetelescope.org/
has abstract	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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