A High-Cadence UV-Optical Telescope Suite On The Lunar South Pole
We propose a suite of telescopes be deployed as part of the Artemis III human-crewed expedition to the lunar south pole, able to collect wide-field simultaneous far-ultraviolet (UV), near-UV, and optical band images with a fast cadence (10 seconds) of a single part of the sky for several hours conti...
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| creator | Fleming, Scott W Barclay, Thomas Bell, Keaton J Bianchi, Luciana Brasseur, C. E Hermes, JJ Loyd, R. O. Parke Million, Chase Osten, Rachel Rest, Armin Ridden-Harper, Ryan Schlieder, Joshua Shkolnik, Evgenya L Szkody, Paula Tucker, Brad E Tucker, Michael A Youngblood, Allison |
| description | We propose a suite of telescopes be deployed as part of the Artemis III
human-crewed expedition to the lunar south pole, able to collect wide-field
simultaneous far-ultraviolet (UV), near-UV, and optical band images with a fast
cadence (10 seconds) of a single part of the sky for several hours
continuously. Wide-field, high-cadence monitoring in the optical regime has
provided new scientific breakthroughs in the fields of exoplanets, stellar
astrophysics, and astronomical transients. Similar observations cannot be made
in the UV from within Earth's atmosphere, but are possible from the Moon's
surface. The proposed observations will enable studies of atmospheric escape
from close-in giant exoplanets, exoplanet magnetospheres, the physics of
stellar flare formation, the impact of stellar flares on exoplanet
habitability, the internal stellar structure of hot, compact stars, and the
early-time evolution of supernovae and novae to better understand their
progenitors and formation mechanisms. |
| doi_str_mv | 10.48550/arxiv.2010.00007 |
| format | Article |
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human-crewed expedition to the lunar south pole, able to collect wide-field
simultaneous far-ultraviolet (UV), near-UV, and optical band images with a fast
cadence (10 seconds) of a single part of the sky for several hours
continuously. Wide-field, high-cadence monitoring in the optical regime has
provided new scientific breakthroughs in the fields of exoplanets, stellar
astrophysics, and astronomical transients. Similar observations cannot be made
in the UV from within Earth's atmosphere, but are possible from the Moon's
surface. The proposed observations will enable studies of atmospheric escape
from close-in giant exoplanets, exoplanet magnetospheres, the physics of
stellar flare formation, the impact of stellar flares on exoplanet
habitability, the internal stellar structure of hot, compact stars, and the
early-time evolution of supernovae and novae to better understand their
progenitors and formation mechanisms.</description><identifier>DOI: 10.48550/arxiv.2010.00007</identifier><language>eng</language><subject>Physics - Earth and Planetary Astrophysics ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2020-09</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2010.00007$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2010.00007$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Fleming, Scott W</creatorcontrib><creatorcontrib>Barclay, Thomas</creatorcontrib><creatorcontrib>Bell, Keaton J</creatorcontrib><creatorcontrib>Bianchi, Luciana</creatorcontrib><creatorcontrib>Brasseur, C. E</creatorcontrib><creatorcontrib>Hermes, JJ</creatorcontrib><creatorcontrib>Loyd, R. O. Parke</creatorcontrib><creatorcontrib>Million, Chase</creatorcontrib><creatorcontrib>Osten, Rachel</creatorcontrib><creatorcontrib>Rest, Armin</creatorcontrib><creatorcontrib>Ridden-Harper, Ryan</creatorcontrib><creatorcontrib>Schlieder, Joshua</creatorcontrib><creatorcontrib>Shkolnik, Evgenya L</creatorcontrib><creatorcontrib>Szkody, Paula</creatorcontrib><creatorcontrib>Tucker, Brad E</creatorcontrib><creatorcontrib>Tucker, Michael A</creatorcontrib><creatorcontrib>Youngblood, Allison</creatorcontrib><title>A High-Cadence UV-Optical Telescope Suite On The Lunar South Pole</title><description>We propose a suite of telescopes be deployed as part of the Artemis III
human-crewed expedition to the lunar south pole, able to collect wide-field
simultaneous far-ultraviolet (UV), near-UV, and optical band images with a fast
cadence (10 seconds) of a single part of the sky for several hours
continuously. Wide-field, high-cadence monitoring in the optical regime has
provided new scientific breakthroughs in the fields of exoplanets, stellar
astrophysics, and astronomical transients. Similar observations cannot be made
in the UV from within Earth's atmosphere, but are possible from the Moon's
surface. The proposed observations will enable studies of atmospheric escape
from close-in giant exoplanets, exoplanet magnetospheres, the physics of
stellar flare formation, the impact of stellar flares on exoplanet
habitability, the internal stellar structure of hot, compact stars, and the
early-time evolution of supernovae and novae to better understand their
progenitors and formation mechanisms.</description><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotz8FOhDAUBdBuXJgZP8CV_YGOLbS81yUh6piQYDLolrxCGZogEAaM_r3jOHdzk7u4yWHsXsmdRmPkI83f4WsXyfMgz4FblqZ8H46dyKjxQ-35-4copiXU1PPS9_5Uj5PnhzUsnhcDLzvP83WgmR_Gden429j7LbtpqT_5u2tvWPn8VGZ7kRcvr1maC0oAhDaJw7ZpDBI2DjSQjq1ykbUIspaUYCyNQgu2lagtOlSQGCWtisDEDuINe_i_vRiqaQ6fNP9Uf5bqYol_Abp2QHA</recordid><startdate>20200930</startdate><enddate>20200930</enddate><creator>Fleming, Scott W</creator><creator>Barclay, Thomas</creator><creator>Bell, Keaton J</creator><creator>Bianchi, Luciana</creator><creator>Brasseur, C. E</creator><creator>Hermes, JJ</creator><creator>Loyd, R. O. Parke</creator><creator>Million, Chase</creator><creator>Osten, Rachel</creator><creator>Rest, Armin</creator><creator>Ridden-Harper, Ryan</creator><creator>Schlieder, Joshua</creator><creator>Shkolnik, Evgenya L</creator><creator>Szkody, Paula</creator><creator>Tucker, Brad E</creator><creator>Tucker, Michael A</creator><creator>Youngblood, Allison</creator><scope>GOX</scope></search><sort><creationdate>20200930</creationdate><title>A High-Cadence UV-Optical Telescope Suite On The Lunar South Pole</title><author>Fleming, Scott W ; Barclay, Thomas ; Bell, Keaton J ; Bianchi, Luciana ; Brasseur, C. E ; Hermes, JJ ; Loyd, R. O. Parke ; Million, Chase ; Osten, Rachel ; Rest, Armin ; Ridden-Harper, Ryan ; Schlieder, Joshua ; Shkolnik, Evgenya L ; Szkody, Paula ; Tucker, Brad E ; Tucker, Michael A ; Youngblood, Allison</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a677-456b8fdd58a8db747a4391b299870c0a6830518979f08498b8176510912753b73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Fleming, Scott W</creatorcontrib><creatorcontrib>Barclay, Thomas</creatorcontrib><creatorcontrib>Bell, Keaton J</creatorcontrib><creatorcontrib>Bianchi, Luciana</creatorcontrib><creatorcontrib>Brasseur, C. E</creatorcontrib><creatorcontrib>Hermes, JJ</creatorcontrib><creatorcontrib>Loyd, R. O. Parke</creatorcontrib><creatorcontrib>Million, Chase</creatorcontrib><creatorcontrib>Osten, Rachel</creatorcontrib><creatorcontrib>Rest, Armin</creatorcontrib><creatorcontrib>Ridden-Harper, Ryan</creatorcontrib><creatorcontrib>Schlieder, Joshua</creatorcontrib><creatorcontrib>Shkolnik, Evgenya L</creatorcontrib><creatorcontrib>Szkody, Paula</creatorcontrib><creatorcontrib>Tucker, Brad E</creatorcontrib><creatorcontrib>Tucker, Michael A</creatorcontrib><creatorcontrib>Youngblood, Allison</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Fleming, Scott W</au><au>Barclay, Thomas</au><au>Bell, Keaton J</au><au>Bianchi, Luciana</au><au>Brasseur, C. E</au><au>Hermes, JJ</au><au>Loyd, R. O. Parke</au><au>Million, Chase</au><au>Osten, Rachel</au><au>Rest, Armin</au><au>Ridden-Harper, Ryan</au><au>Schlieder, Joshua</au><au>Shkolnik, Evgenya L</au><au>Szkody, Paula</au><au>Tucker, Brad E</au><au>Tucker, Michael A</au><au>Youngblood, Allison</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A High-Cadence UV-Optical Telescope Suite On The Lunar South Pole</atitle><date>2020-09-30</date><risdate>2020</risdate><abstract>We propose a suite of telescopes be deployed as part of the Artemis III
human-crewed expedition to the lunar south pole, able to collect wide-field
simultaneous far-ultraviolet (UV), near-UV, and optical band images with a fast
cadence (10 seconds) of a single part of the sky for several hours
continuously. Wide-field, high-cadence monitoring in the optical regime has
provided new scientific breakthroughs in the fields of exoplanets, stellar
astrophysics, and astronomical transients. Similar observations cannot be made
in the UV from within Earth's atmosphere, but are possible from the Moon's
surface. The proposed observations will enable studies of atmospheric escape
from close-in giant exoplanets, exoplanet magnetospheres, the physics of
stellar flare formation, the impact of stellar flares on exoplanet
habitability, the internal stellar structure of hot, compact stars, and the
early-time evolution of supernovae and novae to better understand their
progenitors and formation mechanisms.</abstract><doi>10.48550/arxiv.2010.00007</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - Earth and Planetary Astrophysics Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
| title | A High-Cadence UV-Optical Telescope Suite On The Lunar South Pole |
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