Future of Planetary Atmospheric, Surface, and Interior Science Using Radio and Laser Links
Scientific studies using spacecraft radio links, which are shared with communications and navigation functions, have been carried out on almost every solar system exploration mission in the past five decades. They have led to numerous scientific discoveries as well as technological advances. These r...
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Veröffentlicht in: | Radio science 2019-04, Vol.54 (4), p.365-377 |
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description | Scientific studies using spacecraft radio links, which are shared with communications and navigation functions, have been carried out on almost every solar system exploration mission in the past five decades. They have led to numerous scientific discoveries as well as technological advances. These radio science experiments have investigated the interior structure of every planet in the solar system and several of their satellites, the Moon, and several comets and asteroids and sounded the atmospheres of every planet in the solar system except Mercury, and the atmospheres of Pluto and several large satellites, the Io Plasma Torus, Saturn's and Uranus' rings, and the solar corona. Future experiments at Mercury, the Jovian system, asteroid Psyche, and other targets are currently in various planning and development phases. Over the next 30 years, significant advances in radio and laser link science technologies, including one order of magnitude improvement achievable in range rate and range accuracy and advanced calibration techniques, could enable many additional scientific breakthroughs. Future exploration concepts focus on applications of small spacecraft and entry probes and can include constellations for studies of atmospheric dynamics, interior structures, and surface properties. Selected science‐enabling technologies specific to small spacecraft instrumentation on future missions are under study. Examples include field tests of radio scattering to determine surface properties, constellations for high‐resolution spatial and temporal atmospheric sounding, small science‐quality software‐defined transponders, miniature ultrastable oscillators, and advanced radio‐metric calibrations at the Deep Space Network.
Plain Language Summary
Radio links are used to communicate with spacecraft by sending them commands from ground controllers and receiving back science data. The same links are used to examine important properties of planetary atmospheres, surfaces, and interior structure by carefully studying small changes in the radio signal's frequency and other parameters caused by geophysical phenomena when the spacecraft are close to the planets. Improving the radio system on the spacecraft and ground stations can lead to additional scientific discoveries. There is a trend to use small spacecraft to explore the solar system in future, and research teams are preparing instrumentation systems that are compatible with such possible missions.
Key Points
Spacecraft tele |
doi_str_mv | 10.1029/2018RS006663 |
format | Article |
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Plain Language Summary
Radio links are used to communicate with spacecraft by sending them commands from ground controllers and receiving back science data. The same links are used to examine important properties of planetary atmospheres, surfaces, and interior structure by carefully studying small changes in the radio signal's frequency and other parameters caused by geophysical phenomena when the spacecraft are close to the planets. Improving the radio system on the spacecraft and ground stations can lead to additional scientific discoveries. There is a trend to use small spacecraft to explore the solar system in future, and research teams are preparing instrumentation systems that are compatible with such possible missions.
Key Points
Spacecraft telecommunications links are powerful tools to study planetary atmospheres, interiors, and surfaces as proven over five decades
Instrumentation design and calibration techniques have significantly improved, and concepts are developed for additional breakthroughs
There is a trend to miniaturize spacecraft and components and fly them in groups, sometimes in formation flying</description><identifier>ISSN: 0048-6604</identifier><identifier>EISSN: 1944-799X</identifier><identifier>DOI: 10.1029/2018RS006663</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Asteroid missions ; Asteroids ; Atmosphere ; Atmospheric sounding ; Calibration ; Comets ; CubeSats ; Deep space ; Doppler tracking ; Dynamic structural analysis ; Exploration ; Field tests ; Geophysics ; Ground stations ; Instrumentation ; Instruments ; Links ; Mercury ; Navigation ; occultations ; Oscillators ; Planetary atmospheres ; Pluto (dwarf planet) ; Properties (attributes) ; radio metrics ; Radio scattering ; radio science ; Radio signals ; Satellites ; Saturn ; Saturn atmosphere ; Science ; Solar corona ; Solar system ; Space exploration ; Space missions ; Spacecraft ; Surface properties ; telecommunications links ; Transponders ; Uranus</subject><ispartof>Radio science, 2019-04, Vol.54 (4), p.365-377</ispartof><rights>2019. American Geophysical Union. All Rights Reserved.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c3440-22990e73f076d55db46d10c2d2d5a94b709942585a2d47bfb6f65350514445373</citedby><cites>FETCH-LOGICAL-c3440-22990e73f076d55db46d10c2d2d5a94b709942585a2d47bfb6f65350514445373</cites><orcidid>0000-0002-3950-894X ; 0000-0002-9912-645X ; 0000-0003-2391-8490</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2018RS006663$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2018RS006663$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>315,782,786,1419,1435,11523,27933,27934,45583,45584,46418,46477,46842,46901</link.rule.ids></links><search><creatorcontrib>Asmar, Sami. W.</creatorcontrib><creatorcontrib>Lazio, Joseph</creatorcontrib><creatorcontrib>Atkinson, David H.</creatorcontrib><creatorcontrib>Bell, David J.</creatorcontrib><creatorcontrib>Border, James S.</creatorcontrib><creatorcontrib>Grudinin, Ivan S.</creatorcontrib><creatorcontrib>Mannucci, Anthony J.</creatorcontrib><creatorcontrib>Paik, Meegyeong</creatorcontrib><creatorcontrib>Preston, Robert A.</creatorcontrib><title>Future of Planetary Atmospheric, Surface, and Interior Science Using Radio and Laser Links</title><title>Radio science</title><description>Scientific studies using spacecraft radio links, which are shared with communications and navigation functions, have been carried out on almost every solar system exploration mission in the past five decades. They have led to numerous scientific discoveries as well as technological advances. These radio science experiments have investigated the interior structure of every planet in the solar system and several of their satellites, the Moon, and several comets and asteroids and sounded the atmospheres of every planet in the solar system except Mercury, and the atmospheres of Pluto and several large satellites, the Io Plasma Torus, Saturn's and Uranus' rings, and the solar corona. Future experiments at Mercury, the Jovian system, asteroid Psyche, and other targets are currently in various planning and development phases. Over the next 30 years, significant advances in radio and laser link science technologies, including one order of magnitude improvement achievable in range rate and range accuracy and advanced calibration techniques, could enable many additional scientific breakthroughs. Future exploration concepts focus on applications of small spacecraft and entry probes and can include constellations for studies of atmospheric dynamics, interior structures, and surface properties. Selected science‐enabling technologies specific to small spacecraft instrumentation on future missions are under study. Examples include field tests of radio scattering to determine surface properties, constellations for high‐resolution spatial and temporal atmospheric sounding, small science‐quality software‐defined transponders, miniature ultrastable oscillators, and advanced radio‐metric calibrations at the Deep Space Network.
Plain Language Summary
Radio links are used to communicate with spacecraft by sending them commands from ground controllers and receiving back science data. The same links are used to examine important properties of planetary atmospheres, surfaces, and interior structure by carefully studying small changes in the radio signal's frequency and other parameters caused by geophysical phenomena when the spacecraft are close to the planets. Improving the radio system on the spacecraft and ground stations can lead to additional scientific discoveries. There is a trend to use small spacecraft to explore the solar system in future, and research teams are preparing instrumentation systems that are compatible with such possible missions.
Key Points
Spacecraft telecommunications links are powerful tools to study planetary atmospheres, interiors, and surfaces as proven over five decades
Instrumentation design and calibration techniques have significantly improved, and concepts are developed for additional breakthroughs
There is a trend to miniaturize spacecraft and components and fly them in groups, sometimes in formation flying</description><subject>Asteroid missions</subject><subject>Asteroids</subject><subject>Atmosphere</subject><subject>Atmospheric sounding</subject><subject>Calibration</subject><subject>Comets</subject><subject>CubeSats</subject><subject>Deep space</subject><subject>Doppler tracking</subject><subject>Dynamic structural analysis</subject><subject>Exploration</subject><subject>Field tests</subject><subject>Geophysics</subject><subject>Ground stations</subject><subject>Instrumentation</subject><subject>Instruments</subject><subject>Links</subject><subject>Mercury</subject><subject>Navigation</subject><subject>occultations</subject><subject>Oscillators</subject><subject>Planetary atmospheres</subject><subject>Pluto (dwarf planet)</subject><subject>Properties (attributes)</subject><subject>radio metrics</subject><subject>Radio scattering</subject><subject>radio science</subject><subject>Radio signals</subject><subject>Satellites</subject><subject>Saturn</subject><subject>Saturn atmosphere</subject><subject>Science</subject><subject>Solar corona</subject><subject>Solar system</subject><subject>Space exploration</subject><subject>Space missions</subject><subject>Spacecraft</subject><subject>Surface properties</subject><subject>telecommunications links</subject><subject>Transponders</subject><subject>Uranus</subject><issn>0048-6604</issn><issn>1944-799X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp90FFLwzAQB_AgCs7pmx8g4Ouql_SSNo9jOh0UlNaB-FLSJtXOrZ1Ji-zb2zkffPJeDo4fd9yfkEsG1wy4uuHA4jQDkFKGR2TEFGIQKfVyTEYAGAdSAp6SM-9XAAyFxBF5nfdd7yxtK_q01o3ttNvRabdp_fbdurqc0Kx3lS7thOrG0EXTDdPW0aysbVNauvR180ZTber2ByTaW0eTuvnw5-Sk0mtvL377mCznd8-zhyB5vF_MpklQhogQcK4U2CisIJJGCFOgNAxKbrgRWmERgVLIRSw0NxgVVSErKUIBgiGiCKNwTK4Oe7eu_eyt7_JV27tmOJnzoRRXUu3V5KBK13rvbJVvXb0Zvs0Z5Pv08r_pDZwf-Fe9trt_bZ7eZhyiGMJvVVBuKA</recordid><startdate>201904</startdate><enddate>201904</enddate><creator>Asmar, Sami. W.</creator><creator>Lazio, Joseph</creator><creator>Atkinson, David H.</creator><creator>Bell, David J.</creator><creator>Border, James S.</creator><creator>Grudinin, Ivan S.</creator><creator>Mannucci, Anthony J.</creator><creator>Paik, Meegyeong</creator><creator>Preston, Robert A.</creator><general>Blackwell Publishing Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7SP</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-3950-894X</orcidid><orcidid>https://orcid.org/0000-0002-9912-645X</orcidid><orcidid>https://orcid.org/0000-0003-2391-8490</orcidid></search><sort><creationdate>201904</creationdate><title>Future of Planetary Atmospheric, Surface, and Interior Science Using Radio and Laser Links</title><author>Asmar, Sami. W. ; Lazio, Joseph ; Atkinson, David H. ; Bell, David J. ; Border, James S. ; Grudinin, Ivan S. ; Mannucci, Anthony J. ; Paik, Meegyeong ; Preston, Robert A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c3440-22990e73f076d55db46d10c2d2d5a94b709942585a2d47bfb6f65350514445373</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Asteroid missions</topic><topic>Asteroids</topic><topic>Atmosphere</topic><topic>Atmospheric sounding</topic><topic>Calibration</topic><topic>Comets</topic><topic>CubeSats</topic><topic>Deep space</topic><topic>Doppler tracking</topic><topic>Dynamic structural analysis</topic><topic>Exploration</topic><topic>Field tests</topic><topic>Geophysics</topic><topic>Ground stations</topic><topic>Instrumentation</topic><topic>Instruments</topic><topic>Links</topic><topic>Mercury</topic><topic>Navigation</topic><topic>occultations</topic><topic>Oscillators</topic><topic>Planetary atmospheres</topic><topic>Pluto (dwarf planet)</topic><topic>Properties (attributes)</topic><topic>radio metrics</topic><topic>Radio scattering</topic><topic>radio science</topic><topic>Radio signals</topic><topic>Satellites</topic><topic>Saturn</topic><topic>Saturn atmosphere</topic><topic>Science</topic><topic>Solar corona</topic><topic>Solar system</topic><topic>Space exploration</topic><topic>Space missions</topic><topic>Spacecraft</topic><topic>Surface properties</topic><topic>telecommunications links</topic><topic>Transponders</topic><topic>Uranus</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Asmar, Sami. W.</creatorcontrib><creatorcontrib>Lazio, Joseph</creatorcontrib><creatorcontrib>Atkinson, David H.</creatorcontrib><creatorcontrib>Bell, David J.</creatorcontrib><creatorcontrib>Border, James S.</creatorcontrib><creatorcontrib>Grudinin, Ivan S.</creatorcontrib><creatorcontrib>Mannucci, Anthony J.</creatorcontrib><creatorcontrib>Paik, Meegyeong</creatorcontrib><creatorcontrib>Preston, Robert A.</creatorcontrib><collection>CrossRef</collection><collection>Electronics & Communications Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Radio science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Asmar, Sami. W.</au><au>Lazio, Joseph</au><au>Atkinson, David H.</au><au>Bell, David J.</au><au>Border, James S.</au><au>Grudinin, Ivan S.</au><au>Mannucci, Anthony J.</au><au>Paik, Meegyeong</au><au>Preston, Robert A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Future of Planetary Atmospheric, Surface, and Interior Science Using Radio and Laser Links</atitle><jtitle>Radio science</jtitle><date>2019-04</date><risdate>2019</risdate><volume>54</volume><issue>4</issue><spage>365</spage><epage>377</epage><pages>365-377</pages><issn>0048-6604</issn><eissn>1944-799X</eissn><abstract>Scientific studies using spacecraft radio links, which are shared with communications and navigation functions, have been carried out on almost every solar system exploration mission in the past five decades. They have led to numerous scientific discoveries as well as technological advances. These radio science experiments have investigated the interior structure of every planet in the solar system and several of their satellites, the Moon, and several comets and asteroids and sounded the atmospheres of every planet in the solar system except Mercury, and the atmospheres of Pluto and several large satellites, the Io Plasma Torus, Saturn's and Uranus' rings, and the solar corona. Future experiments at Mercury, the Jovian system, asteroid Psyche, and other targets are currently in various planning and development phases. Over the next 30 years, significant advances in radio and laser link science technologies, including one order of magnitude improvement achievable in range rate and range accuracy and advanced calibration techniques, could enable many additional scientific breakthroughs. Future exploration concepts focus on applications of small spacecraft and entry probes and can include constellations for studies of atmospheric dynamics, interior structures, and surface properties. Selected science‐enabling technologies specific to small spacecraft instrumentation on future missions are under study. Examples include field tests of radio scattering to determine surface properties, constellations for high‐resolution spatial and temporal atmospheric sounding, small science‐quality software‐defined transponders, miniature ultrastable oscillators, and advanced radio‐metric calibrations at the Deep Space Network.
Plain Language Summary
Radio links are used to communicate with spacecraft by sending them commands from ground controllers and receiving back science data. The same links are used to examine important properties of planetary atmospheres, surfaces, and interior structure by carefully studying small changes in the radio signal's frequency and other parameters caused by geophysical phenomena when the spacecraft are close to the planets. Improving the radio system on the spacecraft and ground stations can lead to additional scientific discoveries. There is a trend to use small spacecraft to explore the solar system in future, and research teams are preparing instrumentation systems that are compatible with such possible missions.
Key Points
Spacecraft telecommunications links are powerful tools to study planetary atmospheres, interiors, and surfaces as proven over five decades
Instrumentation design and calibration techniques have significantly improved, and concepts are developed for additional breakthroughs
There is a trend to miniaturize spacecraft and components and fly them in groups, sometimes in formation flying</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2018RS006663</doi><tpages>13</tpages><orcidid>https://orcid.org/0000-0002-3950-894X</orcidid><orcidid>https://orcid.org/0000-0002-9912-645X</orcidid><orcidid>https://orcid.org/0000-0003-2391-8490</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Asteroid missions Asteroids Atmosphere Atmospheric sounding Calibration Comets CubeSats Deep space Doppler tracking Dynamic structural analysis Exploration Field tests Geophysics Ground stations Instrumentation Instruments Links Mercury Navigation occultations Oscillators Planetary atmospheres Pluto (dwarf planet) Properties (attributes) radio metrics Radio scattering radio science Radio signals Satellites Saturn Saturn atmosphere Science Solar corona Solar system Space exploration Space missions Spacecraft Surface properties telecommunications links Transponders Uranus |
title | Future of Planetary Atmospheric, Surface, and Interior Science Using Radio and Laser Links |
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