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| 題名: | Spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko from the OSIRIS instrument onboard the ROSETTA spacecraft |
| 作者: | 葉永烜;Fornasier, S.;Hasselmann, P. H.;Barucci, M. A.;Feller, C.;Besse, S.;Leyrat, C.;Lara, L.;Gutierrez, P. J.;Oklay, N.;Tubiana, C.;Scholten, F.;Sierks, H.;Barbieri, C.;Lamy, P. L.;Rodrigo, R.;Koschny, D.;Rickman, H.;Keller, H. U.;Agarwal, J.;A’Hearn, M. F.;Bertaux, J.-L.;Bertini, I.;Cremonese, G.;Da Deppo, V.;Davidsson, B.;Debei, S.;De Cecco, M.;Fulle, M.;Groussin, O.;Güttler, C.;Hviid, S. F.;Ip, W.;Jorda, L.;Knollenberg, J.;Kovacs, G.;Kramm, R.;Kührt, E.;Küppers, M.;La Forgia, F.;Lazzarin, M.;Lopez Moreno, J. J.;Marzari, F.;Matz, K.-D.;Michalik, H.;Moreno, F.;Mottola, S.;Naletto, G.;Pajola, M.;Pommerol, A.;Preusker, F.;Shi, X.;Snodgrass, C.;Thomas, N.;Vincent, J.-B. |
| 貢獻者: | 理學院天文研究所 |
| 關鍵詞: | Astrophysics;Cameras;Comet nuclei;Comets;comets: individual: 67P/Churyumov-Gerasimenko;Earth and Planetary Astrophysics;Illumination;methods: data analysis;Photometry;Radiance;Rosetta mission;Sciences of the Universe;Surges;techniques: photometric |
| 日期: | 2015-11-01 |
| 上傳時間: | 2026-04-21 14:42:53 (UTC+8) |
| 出版者: | EDP Sciences |
| 摘要: | 摘要： Context. The Rosetta mission of the European Space Agency has been orbiting the comet 67P/Churyumov-Gerasimenko (67P) since August 2014 and is now in its escort phase. A large complement of scientific experiments designed to complete the most detailed study of a comet ever attempted are onboard Rosetta. Aims. We present results for the photometric and spectrophotometric properties of the nucleus of 67P derived from the OSIRIS imaging system, which consists of a Wide Angle Camera (WAC) and a Narrow Angle Camera (NAC). The observations presented here were performed during July and the beginning of August 2014, during the approach phase, when OSIRIS was mapping the surface of the comet with several filters at different phase angles (1.3°–54°). The resolution reached up to 2.1 m/px. Methods. The OSIRIS images were processed with the OSIRIS standard pipeline, then converted into I/F radiance factors and corrected for the illumination conditions at each pixel using the Lommel-Seeliger disk law. Color cubes of the surface were produced by stacking registered and illumination-corrected images. Furthermore, photometric analysis was performed both on disk-averaged photometry in several filters and on disk-resolved images acquired with the NAC orange filter, centered at 649 nm, using Hapke modeling. Results. The disk-averaged phase function of the nucleus of 67P shows a strong opposition surge with a G parameter value of −0.13 ± 0.01 in the HG system formalism and an absolute magnitude Hv(1,1,0) = 15.74 ± 0.02 mag. The integrated spectrophotometry in 20 filters covering the 250−1000 nm wavelength range shows a red spectral behavior, without clear absorption bands except for a potential absorption centered at ~290 nm that is possibly due to SO2 ice. The nucleus shows strong phase reddening, with disk-averaged spectral slopes increasing from 11%/(100 nm) to 16%/(100 nm) in the 1.3°−54° phase angle range. The geometric albedo of the comet is 6.5 ± 0.2% at 649 nm, with local variations of up to ~16% in the Hapi region. From the disk-resolved images we computed the spectral slope together with local spectrophotometry and identified three distinct groups of regions (blue, moderately red, and red). The Hapi region is the brightest, the bluest in term of spectral slope, and the most active surface on the comet. Local spectrophotometry shows an enhancement of the flux in the 700−750 nm that is associated with coma emissions.
出版者： EDP Sciences
出版日期： 2015-11-01
出處： Astronomy & Astrophysics, 2015-11, Vol.583, p.A30-
資源來源： EDP Sciences
版權： licence_http://creativecommons.org/publicdomain/zero
識別號： ISSN: 0004-6361
識別號： ISSN: 1432-0746
識別號： EISSN: 1432-0746
識別號： DOI: 10.1051/0004-6361/201525901 |
| 顯示於類別: | [天文研究所] 期刊論文
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