The microscope for Beagle 2
The microscope for the Beagle 2 lander, which was launched as part of the European Space Agency's Mars Express mission on 2 June 2003, will provide images of the Martian surface at around 6 μm resolution. It will provide optical images of the surface of Mars at a resolution 5 times higher than...
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| Veröffentlicht in: | Planetary and space science 2004-08, Vol.52 (9), p.853-866 |
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| container_title | Planetary and space science |
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| creator | Thomas, N. Lüthi, B.S. Hviid, S.F. Keller, H.U. Markiewicz, W.J. Blümchen, T. Basilevsky, A.T. Smith, P.H. Tanner, R. Oquest, C. Reynolds, R. Josset, J.-L. Beauvivre, S. Hofmann, B. Rüffer, P. Pillinger, C.T. |
| description | The microscope for the Beagle 2 lander, which was launched as part of the European Space Agency's Mars Express mission on 2 June 2003, will provide images of the Martian surface at around
6
μm
resolution. It will provide optical images of the surface of Mars at a resolution 5 times higher than any other experiment currently planned. The device has a working distance of
12
mm
and uses a set of 12 light-emitting diodes which surround the aperture to illuminate the sample in four colours. The target is brought into focus using a stepper motor. This article describes the scientific objectives and the design of the microscope. It also discusses initial results from ground calibration exercises which were designed to validate the system and describes aspects of its operation. |
| doi_str_mv | 10.1016/j.pss.2004.02.008 |
| format | Article |
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6
μm
resolution. It will provide optical images of the surface of Mars at a resolution 5 times higher than any other experiment currently planned. The device has a working distance of
12
mm
and uses a set of 12 light-emitting diodes which surround the aperture to illuminate the sample in four colours. The target is brought into focus using a stepper motor. This article describes the scientific objectives and the design of the microscope. It also discusses initial results from ground calibration exercises which were designed to validate the system and describes aspects of its operation.</description><identifier>ISSN: 0032-0633</identifier><identifier>EISSN: 1873-5088</identifier><identifier>DOI: 10.1016/j.pss.2004.02.008</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><subject>Beagle 2 ; Instrument ; Lander ; Mars ; Microscope</subject><ispartof>Planetary and space science, 2004-08, Vol.52 (9), p.853-866</ispartof><rights>2004 Elsevier Ltd</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c357t-6047aef7565798786e1e3dfc809117f27221fc209bf3995eb8276e15c312eca63</citedby><cites>FETCH-LOGICAL-c357t-6047aef7565798786e1e3dfc809117f27221fc209bf3995eb8276e15c312eca63</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/j.pss.2004.02.008$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,780,784,3550,27924,27925,45995</link.rule.ids></links><search><creatorcontrib>Thomas, N.</creatorcontrib><creatorcontrib>Lüthi, B.S.</creatorcontrib><creatorcontrib>Hviid, S.F.</creatorcontrib><creatorcontrib>Keller, H.U.</creatorcontrib><creatorcontrib>Markiewicz, W.J.</creatorcontrib><creatorcontrib>Blümchen, T.</creatorcontrib><creatorcontrib>Basilevsky, A.T.</creatorcontrib><creatorcontrib>Smith, P.H.</creatorcontrib><creatorcontrib>Tanner, R.</creatorcontrib><creatorcontrib>Oquest, C.</creatorcontrib><creatorcontrib>Reynolds, R.</creatorcontrib><creatorcontrib>Josset, J.-L.</creatorcontrib><creatorcontrib>Beauvivre, S.</creatorcontrib><creatorcontrib>Hofmann, B.</creatorcontrib><creatorcontrib>Rüffer, P.</creatorcontrib><creatorcontrib>Pillinger, C.T.</creatorcontrib><title>The microscope for Beagle 2</title><title>Planetary and space science</title><description>The microscope for the Beagle 2 lander, which was launched as part of the European Space Agency's Mars Express mission on 2 June 2003, will provide images of the Martian surface at around
6
μm
resolution. It will provide optical images of the surface of Mars at a resolution 5 times higher than any other experiment currently planned. The device has a working distance of
12
mm
and uses a set of 12 light-emitting diodes which surround the aperture to illuminate the sample in four colours. The target is brought into focus using a stepper motor. This article describes the scientific objectives and the design of the microscope. 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6
μm
resolution. It will provide optical images of the surface of Mars at a resolution 5 times higher than any other experiment currently planned. The device has a working distance of
12
mm
and uses a set of 12 light-emitting diodes which surround the aperture to illuminate the sample in four colours. The target is brought into focus using a stepper motor. This article describes the scientific objectives and the design of the microscope. It also discusses initial results from ground calibration exercises which were designed to validate the system and describes aspects of its operation.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/j.pss.2004.02.008</doi><tpages>14</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0032-0633 |
| ispartof | Planetary and space science, 2004-08, Vol.52 (9), p.853-866 |
| issn | 0032-0633 1873-5088 |
| language | eng |
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| source | ScienceDirect Freedom Collection (Elsevier) |
| subjects | Beagle 2 Instrument Lander Mars Microscope |
| title | The microscope for Beagle 2 |
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