Component-resolved near-infrared spectra of the (22) Kalliope system
We observed (22) Kalliope and its companion Linus with the integral-field spectrograph OSIRIS, which is coupled to the adaptive optics system at the W.M. Keck 2 telescope on March 25, 2008. We present, for the first time, component-resolved spectra acquired simultaneously in each of the Zbb (1–1.18...
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| Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 2009-12, Vol.204 (2), p.574-579 |
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| container_title | Icarus (New York, N.Y. 1962) |
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| creator | Laver, Conor de Pater, Imke Marchis, Franck Ádámkovics, Máté Wong, Michael H. |
| description | We observed (22) Kalliope and its companion Linus with the integral-field spectrograph OSIRIS, which is coupled to the adaptive optics system at the W.M. Keck 2 telescope on March 25, 2008. We present, for the first time, component-resolved spectra acquired simultaneously in each of the Zbb (1–1.18
μm), Jbb (1.18–1.42
μm), Hbb (1.47–1.80
μm), and Kbb (1.97–2.38
μm) bands. The spectra of the two bodies are remarkably similar and imply that both bodies were formed at the same time from the same material; such as via incomplete re-accretion after a major impact on the precursor body. |
| doi_str_mv | 10.1016/j.icarus.2009.07.002 |
| format | Article |
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μm), Jbb (1.18–1.42
μm), Hbb (1.47–1.80
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μm), Jbb (1.18–1.42
μm), Hbb (1.47–1.80
μm), and Kbb (1.97–2.38
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μm), Jbb (1.18–1.42
μm), Hbb (1.47–1.80
μm), and Kbb (1.97–2.38
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| subjects | Asteroids Infrared observations |
| title | Component-resolved near-infrared spectra of the (22) Kalliope system |
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