The Planetary Science Journal (Jan 2024)
Surface Heterogeneity, Physical, and Shape Model of Near-Earth Asteroid (52768) 1998 OR2
- Maxime Devogèle,
- Anna McGilvray,
- Eric MacLennan,
- Courteney Monchinski,
- Sean E. Marshall,
- Dylan Hickson,
- Anne Virkki,
- Jon D. Giorgini,
- Lyu Abe,
- David Augustin,
- Amadeo Aznar-Macías,
- Philippe Baudouin,
- Raoul Behrend,
- Philippe Bendjoya,
- Zouhair Benkhaldoun,
- Josep Bosch,
- Alberto Cellino,
- Joseph Chatelain,
- Marc Deldem,
- Marin Ferrais,
- Rui Goncalves,
- Gerard Houdin,
- Marek Husárik,
- Emmanuel Jehin,
- Teddy Kareta,
- Myung-Jin Kim,
- Javier Licandro,
- Tim Lister,
- Hissa Medeiros,
- Petr Pravec,
- Jean-Pierre Rivet,
- Gerald Rousseau,
- Dong-Goo Roh,
- Brian Skiff,
- Patrick A. Taylor,
- Flaviane Venditti,
- David Vernet,
- Jean-Michel Vienney,
- Hong-Suh Yim,
- Luisa Zambrano-Marin
Affiliations
- Maxime Devogèle
- ORCiD
- Arecibo Observatory, University of Central Florida , HC-3 Box 53995, Arecibo, PR 00612, USA ; [email protected]
- Anna McGilvray
- Arecibo Observatory, University of Central Florida , HC-3 Box 53995, Arecibo, PR 00612, USA ; [email protected]
- Eric MacLennan
- ORCiD
- Department of Physics, University of Helsinki , P.O. Box 64, 00014, Finland
- Courteney Monchinski
- Earth-Life Science Institute (ELSI), Tokyo Institute of Technology , Meguro, Tokyo 152-8550, Japan
- Sean E. Marshall
- ORCiD
- Arecibo Observatory, University of Central Florida , HC-3 Box 53995, Arecibo, PR 00612, USA ; [email protected]
- Dylan Hickson
- ORCiD
- Center for Wave Phenomena , Colorado School of Mines, 1500 Illinois Street, Golden, CO 80401, USA
- Anne Virkki
- ORCiD
- Department of Physics, University of Helsinki , P.O. Box 64, 00014, Finland
- Jon D. Giorgini
- Jet Propulsion Laboratory, California Institute of Technology , Pasadena, CA 91011, USA
- Lyu Abe
- Université Côte d’Azur , CNRS, OCA, LAGRANGE, France
- David Augustin
- Deep Sky Chile , Pichasca, Chile
- Amadeo Aznar-Macías
- ORCiD
- Isaac Aznar Observatory, APT Observatory Group , Alcublas, Valencia, Spain
- Philippe Baudouin
- Société Astronomique du Havre, Saint Martin du Bec , Seine-Maritime, 76615, France
- Raoul Behrend
- Geneva Observatory , CH-1290 Sauverny, Switzerland
- Philippe Bendjoya
- ORCiD
- Université Côte d’Azur , CNRS, OCA, LAGRANGE, France
- Zouhair Benkhaldoun
- ORCiD
- Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, Cadi Ayyad University , Marrakech, Morocco
- Josep Bosch
- S. Maria de Montmagastrell , Tàrrega, Spain
- Alberto Cellino
- ORCiD
- INAF, Osservatorio Astrofisico di Torino , via Osservatorio 20, 10025 Pino Torinese, Italy
- Joseph Chatelain
- ORCiD
- Las Cumbres Observatory (LCO) , 6740 Cortona Drive, Suite 102, Goleta, CA 93117, USA
- Marc Deldem
- Les Barres Observatory , Lamanon, Bouches-du-Rhône, 13113, France
- Marin Ferrais
- ORCiD
- Arecibo Observatory, University of Central Florida , HC-3 Box 53995, Arecibo, PR 00612, USA ; [email protected]
- Rui Goncalves
- Instituto Politecnico de Tomar , Ci2 and UDMF, 2300-313, Tomar, Portugal
- Gerard Houdin
- Deep Sky Chile , Pichasca, Chile
- Marek Husárik
- ORCiD
- Astronomical Institute of the Slovak Academy of Sciences , SK-05960 Tatranská Lomnica, Slovakia
- Emmanuel Jehin
- ORCiD
- Space Sciences, Technologies & Astrophysics Research (STAR) Institute University of Liège Allée du 6 Août 19 , 4000 Liège, Belgium
- Teddy Kareta
- ORCiD
- Lowell Observatory , 1400 W. Mars Hill Rd., Flagstaff, AZ 86001, USA
- Myung-Jin Kim
- ORCiD
- Korea Astronomy and Space Science Institute , 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea
- Javier Licandro
- ORCiD
- Departamento de Astrofísica, Universidad de La Laguna , 38205 La Laguna, Tenerife, Spain
- Tim Lister
- ORCiD
- Las Cumbres Observatory (LCO) , 6740 Cortona Drive, Suite 102, Goleta, CA 93117, USA
- Hissa Medeiros
- Departamento de Astrofísica, Universidad de La Laguna , 38205 La Laguna, Tenerife, Spain; Instituto de Astrofísica de Canarias (IAC) , C/Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain
- Petr Pravec
- ORCiD
- Astronomical Institute of the Czech Academy of Sciences , Czech Republic
- Jean-Pierre Rivet
- ORCiD
- Université Côte d’Azur , CNRS, OCA, LAGRANGE, France
- Gerald Rousseau
- Observatoire le Chillou , La Roche Clermault, Indre-et-Loire, 37500, France
- Dong-Goo Roh
- ORCiD
- Korea Astronomy and Space Science Institute , 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea
- Brian Skiff
- Lowell Observatory , 1400 W. Mars Hill Rd., Flagstaff, AZ 86001, USA
- Patrick A. Taylor
- ORCiD
- National Radio Astronomy Observatory , Green Bank Observatory, 1180 Boxwood Estate Rd., Charlottesville, VA 22903, USA
- Flaviane Venditti
- ORCiD
- Arecibo Observatory, University of Central Florida , HC-3 Box 53995, Arecibo, PR 00612, USA ; [email protected]
- David Vernet
- Université Côte d’Azur , CNRS, OCA, GALILEE, France
- Jean-Michel Vienney
- Roncevaux Observatory , Buthiers, Seine et Marne, 77760, France
- Hong-Suh Yim
- ORCiD
- Korea Astronomy and Space Science Institute , 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea
- Luisa Zambrano-Marin
- ORCiD
- Arecibo Observatory, University of Central Florida , HC-3 Box 53995, Arecibo, PR 00612, USA ; [email protected]
- DOI
- https://doi.org/10.3847/PSJ/ad1f70
- Journal volume & issue
-
Vol. 5,
no. 2
p. 44
Abstract
On 2020 April 29, the near-Earth object (52768) 1998 OR2 experienced a close approach to Earth at a distance of 16.4 lunar distances (LD). 1998 OR2 is a potentially hazardous asteroid of absolute magnitude H = 16.04 that can currently come as close to Earth as 3.4 LD. We report here observations of this object in polarimetry, photometry, and radar. Our observations show that the physical characteristics of 1998 OR2 are similar to those of both M- and S-type asteroids. Arecibo’s radar observations provide a high radar albedo of ${\hat{\sigma }}_{\mathrm{OC}}\,=$ 0.29 ± 0.08, suggesting that metals are present in 1998 OR2 near-surface. We find a circular polarization ratio of μ _c = 0.291 ± 0.012, and the delay-Doppler images show that the surface of 1998 OR2 is a top-shape asteroid with large-scale structures such as large craters and concavities. The polarimetric observations display a consistent variation of the polarimetric response as a function of the rotational phase, suggesting that the surface of 1998 OR2 is heterogeneous. Color observations suggest an X-complex taxonomy in the Bus–DeMeo classification. Combining optical polarization, radar, and two epochs from the NEOWISE satellite observations, we derived an equivalent diameter of D = 1.80 ± 0.1 km and a visual albedo p _v = 0.21 ± 0.02. Photometric and radar data provide a sidereal rotation period of P = 4.10872 ± 0.00001 hr, a pole orientation of (332.°3 ± 5°, 20.°7 ± 5°), and a shape model with dimensions of $({2.08}_{-0.10}^{+0.10},{1.93}_{-0.10}^{+0.10},{1.60}_{-0.05}^{+0.05})$ km.
Keywords