Photometric and spectroscopic investigation of 2867 Steins, target of the Rosetta mission. Ground-based results prior to the Rosetta fly-by

Keywords

Asteroid, Photometry (optics), Absolute magnitude, Physics, Astrophysics

References

• Asteroid 2867 Steins III. Spitzer Space Telescope observations, size determination, and thermal propertiesP. L. Lamy, L. Jordá, S. Fornasier — 2008
• Opposition polarimetry and photometry of S- and E-type asteroidsI. N. Belskaya, V. G. Shevchenko, N. N. Kiselev — 2003
• The surface composition of Jupiter Trojans: Visible and near-infrared survey of dynamical families ☆E. Dotto, S. Fornasier, M. A. Barucci — 2006
• Searching for water ice on 47171 1999 TC36, 1998 SG35, and 2000 QC243: ESO large program on TNOs and centaursE. Dotto — 2003
• Opposition Effect of AsteroidsI. N. Belskaya — 2000
• Asteroid target selection for the new Rosetta mission baseline: 21 Lutetia and 2867 SteinsMaria Antonella Barucci, M. Fulchignoni, S. Fornasier — 2005
• Determination of the light curve of the Rosetta target asteroid (2867) Steins by the OSIRIS cameras onboard RosettaM. Küppers, S. Mottola, S. C. Lowry — 2006
• Photometric observations of Rosetta target asteroid 2867 SteinsP. R. Weissman, S. C. Lowry, Young‐Jun Choi — 2007
• UBVRI Photometric Standard Stars in the Magnitude Range 11A. U. Landolt — 1992
• Asteroids 2867 Steins and 21 Lutetia: surface composition from far infrared observations with the Spitzer space telescopeM. A. Barucci, S. Fornasier, E. Dotto — 2008
• First albedo determination of 2867 Steins, target of the Rosetta missionS. Fornasier, I. N. Belskaya, M. Fulchignoni — 2006
• Are the E-type asteroids (2867) Steins, a target of the Rosetta mission, and NEA (3103) Eger remnants of an old asteroid family?S. Fornasier, F. Marzari, E. Dotto — 2007
• Phase relations of high albedo asteroids: The unusual opposition brightening of 44 Nysa and 64 Angelina☆A.W. Harris — 1989
• Photoelectric observations of asteroids 3, 24, 60, 261, and 863Alan W. Harris, James W. Young, E. Bowell — 1989
• Visible and near infrared spectroscopic investigation of E-type asteroids, including 2867 Steins, a target of the Rosetta missionS. Fornasier, A. Migliorini, E. Dotto — 2008
• Asteroid 2867 Steins - II. Multi-telescope visible observations, shape reconstruction, and rotational stateP. L. Lamy, M. Kaasalainen, S. C. Lowry — 2008
• Asteroid 2867 Steins. I. Photometric properties from OSIRIS/Rosetta and ground-based visible observationsL. Jordá, P. Lamy, G. Faury — 2008

Cited by

• The light curve of asteroid 21 Lutetia measured by VIRTIS-M during the Rosetta fly-byF. Tosi, A. Coradini, F. Capaccioni — 2010
• The far-ultraviolet albedo of Šteins measured with Rosetta-ALICEMichael F. A’Hearn, Lori M. Feaga, Jean‐Loup Bertaux — 2010
• Sample Return Missions from Minor Bodies: Achievements, Future Plan and Observational SupportJ. R. Brucato, A. Rotundi, E. Mazzotta Epifani — 2009
• Evidence for surface variegation in Rosetta OSIRIS images of asteroid 2867 ŠteinsStefan Schröder, H. U. Keller, P. J. Gutiérrez — 2010
• Search for Steins' surface inhomogeneities from OSIRIS Rosetta imagesC. Leyrat, S. Fornasier, A. Barucci — 2010
• Thermal properties of the asteroid (2867) Steins as observed by VIRTIS/RosettaC. Leyrat, A. Coradini, S. Érard — 2011
• Asteroid observations at low phase angles. IV: Average parameters for the new H, G1, G2 magnitude systemV. G. Shevchenko, I. N. Belskaya, K. Muinonen — 2016
• Disk-resolved photometry of Vesta and Lutetia and comparison with other asteroidsA. Longobardo, E. Palomba, M. Ciarniello — 2016
• Inhomogeneities on the surface of 21 Lutetia, the asteroid target of the Rosetta mission. Ground-basD. Perna, E. Dotto, M. Lazzarin — 2010
• History and Implications of Asteroid ExplorationSijia WEI, Yuyang HE, Tianyu LIU — 2024
• Laboratory reflectance spectra of enstatite and oldhamite mixtures for comparison with Earth-based reflectance spectra of asteroid 2867 Šteins and MercuryKathrin Markus, G. Arnold, L. V. Moroz — 2024
• 2.14 – Asteroids2014

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