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Earth-Based Visible and Near-IR Imaging of Mercury
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2007 (English)In: Space Science Reviews, ISSN 0038-6308, E-ISSN 1572-9672, Vol. 132, no 2-4, 351-397 p.Article in journal (Refereed) Published
Abstract [en]

New planned orbiter missions to Mercury have prompted renewed efforts to investigate the surface of Mercury via ground-based remote sensing. While the highest resolution instrumentation optical telescopes (e.g., HST) cannot be used at angular distances close to the Sun, advanced ground-based astronomical techniques and modern analytical and software can be used to obtain the resolved images of the poorly known or unknown part of Mercury. Our observations of the planet presented here were carried out in many observatories at morning and evening elongation of the planet. Stacking the acquired images of the hemisphere of Mercury, which was not observed by the Mariner 10 mission (1974–1975), is presented. Huge features found there change radically the existing hypothesis that the “continental” character of a surface may be attributed to the whole planet. We present the observational method, the data analysis approach, the resulting images and obtained properties of the Mercury’s surface.

Place, publisher, year, edition, pages
2007. Vol. 132, no 2-4, 351-397 p.
Keyword [en]
Solar system, Unknown side of Mercury, Ground based observation, Resolved images, Regolith physical properties
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:uu:diva-24838DOI: 10.1007/s11214-007-9290-3ISI: 000251996200008OAI: oai:DiVA.org:uu-24838DiVA: diva2:52612
Available from: 2008-01-25 Created: 2008-01-25 Last updated: 2017-12-07Bibliographically approved

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Publisher's full texthttp://adsabs.harvard.edu/abs/2007SSRv..132..351K

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Warell, Johan

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