Observations of Mars and its satellites by the Mars Imaging Camera (MIC) on Planet-B
We present the specifications of the Mars Imaging Camera (MIC) on the Planet-B spin-stabilized spacecraft, and key scientific objectives of MIC observations. A non-sun-synchronous orbit of Planet-B with a large eccentricity of about 0.87 around Mars provides the opportunities (1) to observe the same...
Gespeichert in:
Veröffentlicht in: | Earth, planets, and space planets, and space, 1998-01, Vol.50 (3), p.183-188 |
---|---|
Hauptverfasser: | , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 188 |
---|---|
container_issue | 3 |
container_start_page | 183 |
container_title | Earth, planets, and space |
container_volume | 50 |
creator | Mukai, Tadashi Akabane, Tokuhide Hashimoto, Tatsuaki Ishimoto, Hiroshi Sasaki, Sho Inada, Ai Toigo, Anthony Nakamura, Masato Abe, Yutaka Kurita, Kei Imamura, Takeshi |
description | We present the specifications of the Mars Imaging Camera (MIC) on the Planet-B spin-stabilized spacecraft, and key scientific objectives of MIC observations. A non-sun-synchronous orbit of Planet-B with a large eccentricity of about 0.87 around Mars provides the opportunities (1) to observe the same region of Mars at various times of day and various solar phase angles with spatial resolution of about 60 m from a distance of 150 km altitude (at periapsis), and (2) to monitor changes of global atmospheric conditions on Mars near an apoapsis of 15 Mars radii. In addition, (3) several encounters of Planet-B with each of the two Martian satellites are scheduled during the mission lifetime of two years from October 1999 to observe their shapes and surface structures with three color filters, centered on 450, 550, and 650 nm. (4) A search for hypothetical dust rings along the orbits of two satellites will be tried from the forward-scattering region of sunlight. |
doi_str_mv | 10.1186/BF03352101 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2928457944</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2928457944</sourcerecordid><originalsourceid>FETCH-LOGICAL-c504t-9ee661d7c6d22a8e1309a821b0d0566920ffcccde55235808afb86045be087b93</originalsourceid><addsrcrecordid>eNpNkEFLAzEUhIMoWKsXf0HAiwqrL8kmTY52sVpoqYd6Xt7uvq1btrs1SYX-eysV9DQD8zEDw9i1gAchrHkcT0ApLQWIEzYQ1kKinRWn__w5uwhhDaAgNWrAlosikP_C2PRd4H3N5-gDx67iTQw8YKS2bSIFXux5_KBjPN3gqulWPMMNeeS382l2x_uOv7XYUUzGl-ysxjbQ1a8O2fvkeZm9JrPFyzR7miWlhjQmjsgYUY1KU0mJloQCh1aKAirQxjgJdV2WZUVaS6UtWKwLayDVBYEdFU4N2c2xd-v7zx2FmK_7ne8Ok7l00qZ65NL0QN0fqdL3IXiq861vNuj3uYD857X87zX1DZ0eXFY</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2928457944</pqid></control><display><type>article</type><title>Observations of Mars and its satellites by the Mars Imaging Camera (MIC) on Planet-B</title><source>Springer Nature OA Free Journals</source><source>J-STAGE (Japan Science & Technology Information Aggregator, Electronic) Freely Available Titles - Japanese</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><source>SpringerLink Journals - AutoHoldings</source><creator>Mukai, Tadashi ; Akabane, Tokuhide ; Hashimoto, Tatsuaki ; Ishimoto, Hiroshi ; Sasaki, Sho ; Inada, Ai ; Toigo, Anthony ; Nakamura, Masato ; Abe, Yutaka ; Kurita, Kei ; Imamura, Takeshi</creator><creatorcontrib>Mukai, Tadashi ; Akabane, Tokuhide ; Hashimoto, Tatsuaki ; Ishimoto, Hiroshi ; Sasaki, Sho ; Inada, Ai ; Toigo, Anthony ; Nakamura, Masato ; Abe, Yutaka ; Kurita, Kei ; Imamura, Takeshi</creatorcontrib><description>We present the specifications of the Mars Imaging Camera (MIC) on the Planet-B spin-stabilized spacecraft, and key scientific objectives of MIC observations. A non-sun-synchronous orbit of Planet-B with a large eccentricity of about 0.87 around Mars provides the opportunities (1) to observe the same region of Mars at various times of day and various solar phase angles with spatial resolution of about 60 m from a distance of 150 km altitude (at periapsis), and (2) to monitor changes of global atmospheric conditions on Mars near an apoapsis of 15 Mars radii. In addition, (3) several encounters of Planet-B with each of the two Martian satellites are scheduled during the mission lifetime of two years from October 1999 to observe their shapes and surface structures with three color filters, centered on 450, 550, and 650 nm. (4) A search for hypothetical dust rings along the orbits of two satellites will be tried from the forward-scattering region of sunlight.</description><identifier>ISSN: 1880-5981</identifier><identifier>EISSN: 1880-5981</identifier><identifier>DOI: 10.1186/BF03352101</identifier><language>eng</language><publisher>Heidelberg: Springer Nature B.V</publisher><subject>Cameras ; Mars ; Mars satellites ; Planetary orbits ; Planets ; Satellite imagery ; Satellite observation ; Satellites ; Spacecraft ; Spatial resolution ; Sun-synchronous orbits ; Sunlight</subject><ispartof>Earth, planets, and space, 1998-01, Vol.50 (3), p.183-188</ispartof><rights>The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1998.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c504t-9ee661d7c6d22a8e1309a821b0d0566920ffcccde55235808afb86045be087b93</citedby><cites>FETCH-LOGICAL-c504t-9ee661d7c6d22a8e1309a821b0d0566920ffcccde55235808afb86045be087b93</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Mukai, Tadashi</creatorcontrib><creatorcontrib>Akabane, Tokuhide</creatorcontrib><creatorcontrib>Hashimoto, Tatsuaki</creatorcontrib><creatorcontrib>Ishimoto, Hiroshi</creatorcontrib><creatorcontrib>Sasaki, Sho</creatorcontrib><creatorcontrib>Inada, Ai</creatorcontrib><creatorcontrib>Toigo, Anthony</creatorcontrib><creatorcontrib>Nakamura, Masato</creatorcontrib><creatorcontrib>Abe, Yutaka</creatorcontrib><creatorcontrib>Kurita, Kei</creatorcontrib><creatorcontrib>Imamura, Takeshi</creatorcontrib><title>Observations of Mars and its satellites by the Mars Imaging Camera (MIC) on Planet-B</title><title>Earth, planets, and space</title><description>We present the specifications of the Mars Imaging Camera (MIC) on the Planet-B spin-stabilized spacecraft, and key scientific objectives of MIC observations. A non-sun-synchronous orbit of Planet-B with a large eccentricity of about 0.87 around Mars provides the opportunities (1) to observe the same region of Mars at various times of day and various solar phase angles with spatial resolution of about 60 m from a distance of 150 km altitude (at periapsis), and (2) to monitor changes of global atmospheric conditions on Mars near an apoapsis of 15 Mars radii. In addition, (3) several encounters of Planet-B with each of the two Martian satellites are scheduled during the mission lifetime of two years from October 1999 to observe their shapes and surface structures with three color filters, centered on 450, 550, and 650 nm. (4) A search for hypothetical dust rings along the orbits of two satellites will be tried from the forward-scattering region of sunlight.</description><subject>Cameras</subject><subject>Mars</subject><subject>Mars satellites</subject><subject>Planetary orbits</subject><subject>Planets</subject><subject>Satellite imagery</subject><subject>Satellite observation</subject><subject>Satellites</subject><subject>Spacecraft</subject><subject>Spatial resolution</subject><subject>Sun-synchronous orbits</subject><subject>Sunlight</subject><issn>1880-5981</issn><issn>1880-5981</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1998</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNpNkEFLAzEUhIMoWKsXf0HAiwqrL8kmTY52sVpoqYd6Xt7uvq1btrs1SYX-eysV9DQD8zEDw9i1gAchrHkcT0ApLQWIEzYQ1kKinRWn__w5uwhhDaAgNWrAlosikP_C2PRd4H3N5-gDx67iTQw8YKS2bSIFXux5_KBjPN3gqulWPMMNeeS382l2x_uOv7XYUUzGl-ysxjbQ1a8O2fvkeZm9JrPFyzR7miWlhjQmjsgYUY1KU0mJloQCh1aKAirQxjgJdV2WZUVaS6UtWKwLayDVBYEdFU4N2c2xd-v7zx2FmK_7ne8Ok7l00qZ65NL0QN0fqdL3IXiq861vNuj3uYD857X87zX1DZ0eXFY</recordid><startdate>19980101</startdate><enddate>19980101</enddate><creator>Mukai, Tadashi</creator><creator>Akabane, Tokuhide</creator><creator>Hashimoto, Tatsuaki</creator><creator>Ishimoto, Hiroshi</creator><creator>Sasaki, Sho</creator><creator>Inada, Ai</creator><creator>Toigo, Anthony</creator><creator>Nakamura, Masato</creator><creator>Abe, Yutaka</creator><creator>Kurita, Kei</creator><creator>Imamura, Takeshi</creator><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PCBAR</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope></search><sort><creationdate>19980101</creationdate><title>Observations of Mars and its satellites by the Mars Imaging Camera (MIC) on Planet-B</title><author>Mukai, Tadashi ; Akabane, Tokuhide ; Hashimoto, Tatsuaki ; Ishimoto, Hiroshi ; Sasaki, Sho ; Inada, Ai ; Toigo, Anthony ; Nakamura, Masato ; Abe, Yutaka ; Kurita, Kei ; Imamura, Takeshi</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c504t-9ee661d7c6d22a8e1309a821b0d0566920ffcccde55235808afb86045be087b93</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1998</creationdate><topic>Cameras</topic><topic>Mars</topic><topic>Mars satellites</topic><topic>Planetary orbits</topic><topic>Planets</topic><topic>Satellite imagery</topic><topic>Satellite observation</topic><topic>Satellites</topic><topic>Spacecraft</topic><topic>Spatial resolution</topic><topic>Sun-synchronous orbits</topic><topic>Sunlight</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Mukai, Tadashi</creatorcontrib><creatorcontrib>Akabane, Tokuhide</creatorcontrib><creatorcontrib>Hashimoto, Tatsuaki</creatorcontrib><creatorcontrib>Ishimoto, Hiroshi</creatorcontrib><creatorcontrib>Sasaki, Sho</creatorcontrib><creatorcontrib>Inada, Ai</creatorcontrib><creatorcontrib>Toigo, Anthony</creatorcontrib><creatorcontrib>Nakamura, Masato</creatorcontrib><creatorcontrib>Abe, Yutaka</creatorcontrib><creatorcontrib>Kurita, Kei</creatorcontrib><creatorcontrib>Imamura, Takeshi</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><jtitle>Earth, planets, and space</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Mukai, Tadashi</au><au>Akabane, Tokuhide</au><au>Hashimoto, Tatsuaki</au><au>Ishimoto, Hiroshi</au><au>Sasaki, Sho</au><au>Inada, Ai</au><au>Toigo, Anthony</au><au>Nakamura, Masato</au><au>Abe, Yutaka</au><au>Kurita, Kei</au><au>Imamura, Takeshi</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Observations of Mars and its satellites by the Mars Imaging Camera (MIC) on Planet-B</atitle><jtitle>Earth, planets, and space</jtitle><date>1998-01-01</date><risdate>1998</risdate><volume>50</volume><issue>3</issue><spage>183</spage><epage>188</epage><pages>183-188</pages><issn>1880-5981</issn><eissn>1880-5981</eissn><abstract>We present the specifications of the Mars Imaging Camera (MIC) on the Planet-B spin-stabilized spacecraft, and key scientific objectives of MIC observations. A non-sun-synchronous orbit of Planet-B with a large eccentricity of about 0.87 around Mars provides the opportunities (1) to observe the same region of Mars at various times of day and various solar phase angles with spatial resolution of about 60 m from a distance of 150 km altitude (at periapsis), and (2) to monitor changes of global atmospheric conditions on Mars near an apoapsis of 15 Mars radii. In addition, (3) several encounters of Planet-B with each of the two Martian satellites are scheduled during the mission lifetime of two years from October 1999 to observe their shapes and surface structures with three color filters, centered on 450, 550, and 650 nm. (4) A search for hypothetical dust rings along the orbits of two satellites will be tried from the forward-scattering region of sunlight.</abstract><cop>Heidelberg</cop><pub>Springer Nature B.V</pub><doi>10.1186/BF03352101</doi><tpages>6</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1880-5981 |
ispartof | Earth, planets, and space, 1998-01, Vol.50 (3), p.183-188 |
issn | 1880-5981 1880-5981 |
language | eng |
recordid | cdi_proquest_journals_2928457944 |
source | Springer Nature OA Free Journals; J-STAGE (Japan Science & Technology Information Aggregator, Electronic) Freely Available Titles - Japanese; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection; SpringerLink Journals - AutoHoldings |
subjects | Cameras Mars Mars satellites Planetary orbits Planets Satellite imagery Satellite observation Satellites Spacecraft Spatial resolution Sun-synchronous orbits Sunlight |
title | Observations of Mars and its satellites by the Mars Imaging Camera (MIC) on Planet-B |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-08T00%3A28%3A02IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Observations%20of%20Mars%20and%20its%20satellites%20by%20the%20Mars%20Imaging%20Camera%20(MIC)%20on%20Planet-B&rft.jtitle=Earth,%20planets,%20and%20space&rft.au=Mukai,%20Tadashi&rft.date=1998-01-01&rft.volume=50&rft.issue=3&rft.spage=183&rft.epage=188&rft.pages=183-188&rft.issn=1880-5981&rft.eissn=1880-5981&rft_id=info:doi/10.1186/BF03352101&rft_dat=%3Cproquest_cross%3E2928457944%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2928457944&rft_id=info:pmid/&rfr_iscdi=true |