Surface Heterogeneity, Physical, and Shape Model of Near-Earth Asteroid (52768) 1998 OR2

Author:

Devogèle MaximeORCID,McGilvray Anna,MacLennan EricORCID,Monchinski Courteney,Marshall Sean E.ORCID,Hickson DylanORCID,Virkki AnneORCID,Giorgini Jon D.,Abe Lyu,Augustin David,Aznar-Macías AmadeoORCID,Baudouin Philippe,Behrend Raoul,Bendjoya PhilippeORCID,Benkhaldoun ZouhairORCID,Bosch Josep,Cellino AlbertoORCID,Chatelain JosephORCID,Deldem Marc,Ferrais MarinORCID,Goncalves Rui,Houdin Gerard,Husárik MarekORCID,Jehin EmmanuelORCID,Kareta TeddyORCID,Kim Myung-JinORCID,Licandro JavierORCID,Lister TimORCID,Medeiros Hissa,Pravec PetrORCID,Rivet Jean-PierreORCID,Rousseau Gerald,Roh Dong-GooORCID,Skiff Brian,Taylor Patrick A.ORCID,Venditti FlavianeORCID,Vernet David,Vienney Jean-Michel,Yim Hong-SuhORCID,Zambrano-Marin LuisaORCID

Abstract

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 σ ˆ 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.

Funder

National Aeronautics and Space Administration

Fonds De La Recherche Scientifique - FNRS

Istituto Nazionale di Astrofisica

European Union

Consejería de Educación, Universidades y Sostenibilidad, Gobierno de Canarias

MEC ∣ Agencia Estatal de Investigación

Publisher

American Astronomical Society

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The Unusual Brightness Phase Curve of (65803) Didymos;The Planetary Science Journal;2024-04-01

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3