Initial refinement of minor planet orbits for pointing and observation with the Hubble Space Telescope
Refinements of the orbital elements for 24 minor planets that will be observed with the Fine Guidance Sensors (FGSs) on the Hubble Space Telescope (HST) are presented. The accuracy of these orbits is discussed in the context of the ephemeris requirements for target acquisition with the FGSs. Compari...
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Veröffentlicht in: | The Astronomical journal 1991-08, Vol.102 (2), p.816-822 |
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creator | Whipple, Arthur L. Hemenway, Paul D. Ingram, Doug |
description | Refinements of the orbital elements for 24 minor planets that will be observed with the Fine Guidance Sensors (FGSs) on the Hubble Space Telescope (HST) are presented. The accuracy of these orbits is discussed in the context of the ephemeris requirements for target acquisition with the FGSs. Comparisons with standard catalog orbits are made to evaluate the suitability of the use of the catalog orbits for HST pointing. It is found that the orbits published in the most recent Minor Planet Circulars are capable of positional predictions that are accurate at the 1-arcsec level. However, there are still many orbits that have not been revised in the last 10 yr and these should not be used for critical pointing ephemerides. In many cases, the orbital elements will have to be refined using recent ground-based observations before a minor planet can be reliably observed by HST. |
doi_str_mv | 10.1086/115913 |
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The accuracy of these orbits is discussed in the context of the ephemeris requirements for target acquisition with the FGSs. Comparisons with standard catalog orbits are made to evaluate the suitability of the use of the catalog orbits for HST pointing. It is found that the orbits published in the most recent Minor Planet Circulars are capable of positional predictions that are accurate at the 1-arcsec level. However, there are still many orbits that have not been revised in the last 10 yr and these should not be used for critical pointing ephemerides. In many cases, the orbital elements will have to be refined using recent ground-based observations before a minor planet can be reliably observed by HST.</description><identifier>ISSN: 0004-6256</identifier><identifier>EISSN: 1538-3881</identifier><identifier>DOI: 10.1086/115913</identifier><identifier>CODEN: ANJOAA</identifier><language>eng</language><publisher>Legacy CDMS: University of Chicago Press</publisher><subject>Asteroids (minor planets) ; Astronomy ; Earth, ocean, space ; Exact sciences and technology ; Planets, their satellites and rings. 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The accuracy of these orbits is discussed in the context of the ephemeris requirements for target acquisition with the FGSs. Comparisons with standard catalog orbits are made to evaluate the suitability of the use of the catalog orbits for HST pointing. It is found that the orbits published in the most recent Minor Planet Circulars are capable of positional predictions that are accurate at the 1-arcsec level. However, there are still many orbits that have not been revised in the last 10 yr and these should not be used for critical pointing ephemerides. In many cases, the orbital elements will have to be refined using recent ground-based observations before a minor planet can be reliably observed by HST.</description><subject>Asteroids (minor planets)</subject><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Planets, their satellites and rings. 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Asteroids</topic><topic>Solar system</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Whipple, Arthur L.</creatorcontrib><creatorcontrib>Hemenway, Paul D.</creatorcontrib><creatorcontrib>Ingram, Doug</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>The Astronomical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Whipple, Arthur L.</au><au>Hemenway, Paul D.</au><au>Ingram, Doug</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Initial refinement of minor planet orbits for pointing and observation with the Hubble Space Telescope</atitle><jtitle>The Astronomical journal</jtitle><date>1991-08-01</date><risdate>1991</risdate><volume>102</volume><issue>2</issue><spage>816</spage><epage>822</epage><pages>816-822</pages><issn>0004-6256</issn><eissn>1538-3881</eissn><coden>ANJOAA</coden><abstract>Refinements of the orbital elements for 24 minor planets that will be observed with the Fine Guidance Sensors (FGSs) on the Hubble Space Telescope (HST) are presented. The accuracy of these orbits is discussed in the context of the ephemeris requirements for target acquisition with the FGSs. Comparisons with standard catalog orbits are made to evaluate the suitability of the use of the catalog orbits for HST pointing. It is found that the orbits published in the most recent Minor Planet Circulars are capable of positional predictions that are accurate at the 1-arcsec level. However, there are still many orbits that have not been revised in the last 10 yr and these should not be used for critical pointing ephemerides. In many cases, the orbital elements will have to be refined using recent ground-based observations before a minor planet can be reliably observed by HST.</abstract><cop>Legacy CDMS</cop><pub>University of Chicago Press</pub><doi>10.1086/115913</doi><tpages>7</tpages></addata></record> |
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subjects | Asteroids (minor planets) Astronomy Earth, ocean, space Exact sciences and technology Planets, their satellites and rings. Asteroids Solar system |
title | Initial refinement of minor planet orbits for pointing and observation with the Hubble Space Telescope |
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