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Characterisation of 2020 CD3, Earth's Second Minimoon

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Characterisation of 2020 CD3, Earth's Second Minimoon EPSC Abstracts Vol. 14, EPSC2020-658, 2020 https://doi.org/10.5194/epsc2020-658 Europlanet Science Congress 2020 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Characterisation of 2020 CD3, Earth’s second minimoon Grigori Fedorets1, Marco Micheli2,3, Robert Jedicke4, Shantanu P. Naidu5, Davide Farnocchia5, Mikael Granvik6,7, Nicholas Moskovitz8, Megan E. Schwamb1, Robert Weryk4, Kacper Wierzchos9, Eric Christensen9, Theodore Pruyne9, William F. Bottke10, Quanzhi Ye11, Richard Wainscoat4, Maxime Devogele8, Laura E. Buchanan1, and the et al.* 1Queen's University Belfast, School of Maths and Physics, Astrophysics Research Centre, Belfast, co. Antrim, United Kingdom of Great Britain and Northern Ireland ([email protected]) 2ESA NEO Coordination Centre, Frascati, Italy 3INAF - Osservatorio Astronomico di Roma, Italy 4University of Hawaii, Institute for Astronomy, Honolulu, Hawaii, USA 5Jet Propulsion Laboratory, California University of technology, Pasadena, California, USA 6Department of Physics, University of Helsinki, Finland 7Division of Space Technology, Lulea University of Technology, Kiruna, Sweden 8Lowell Observatory, Flagstaff, Arizona, USA 9University of Arizona, Lunar and Planetary Laboratory, Tucson, Arizona, USA 10Department of Space Studies, Southwest Research Institute, Boulder, Colorado, USA 11Department of Astronomy, University of Maryland, College Park, Maryland, USA *A full list of authors appears at the end of the abstract Introduction Small solar system objects may occasionally become captured temporarily by planets. Theoretical models (Granvik et al. 2012, Fedorets et al. 2017) predict the existence of a steady-state population of these objects, also known as minimoons, also in the Earth-Moon system. Only one minimoon, 2006 RH120 has been discovered until recently (Kwiatkowski et al. 2009). Since minimoons spend a significant amount of time in Earth’s vicinity, they have been identified as outstanding targets for in situ exploration, or test cases for initial steps of asteroid resource utilisation (Granvik et al. 2013, Chyba et al. 2014, Brelsford et al. 2016, Jedicke et al. 2018). Moreover, not only are minimoons outstanding targets to constrain the size-frequency distribution of metre-sized asteroids (Harris & D’Abramo 2015, Granvik et al. 2016, Tricarico 2017, Brown et al. 2002), but also for studying the structure of the smallest asteroids. However, until now, the observational evidence of the minimoon population has been lacking. Observations The object 2020 CD3 was discovered on February 15th 2020 at the Mt. Lemmon station of the Catalina Sky Survey, and was noticed to be on a geocentric orbit the following night. We report the results of the astrometric and photometric observational campaign to characterise 2020 CD3 performed by Gemini North, LDT, NOT, CFHT, CSS, and other telescopes during spring 2020. By investigating the solar radiation pressure signature on the astrometry of 2020 CD3, and broad-band photometry, we present evidence that 2020 CD3 is indeed the second temporary natural satellite in the Earth-Moon system. We describe its discovery circumstances, physical characterisation, rotational period and orbital evolution. Discussion Using 2020 CD3 as an example case, we discuss the challenges of discovering minimoons with contemporary surveys. For the first time, we are able to compare the observational evidence of minimoons with the theoretical models. We also assess the capture duration and rotation period of 2020 CD3 in context of simulation and similar objects. Finally, we compare the origin of minimoons as captured objects from the NEO population against their origin as lunar ejecta, and show why the first mechanism is dominant. Prospects The discovery of 2020 CD3, and the comparison to discovery predictions with other surveys (Bolin et al. 2014), assures that the expectation of discovery of tens of minimoons with LSST is realistic (Fedorets et al. 2020). With the anticipated growth of the population of minimoons, the path for further exploration of minimoons is foreseen. References Bolin et al. (2014), Icarus 241, 280 Brelsford et al. (2016), PSS, 123, 4. Brown et al. (2002), Nature, 420, 294. Chyba et al. (2014) JIMO, 10(2), 477. Fedorets et al. (2017) Icarus, 285, 83. Fedorets et al. (2020), Icarus, 338, 113517. Granvik et al. (2012), Icarus, 218, 262. Granvik et al. (2013) in V. Badescu ed. Asteroids: Prospective Energy and Material Resources, 151. Granvik et al. (2016), Nature, 530, 303. Harris & D’Abramo (2015), Icarus, 257, 302. Jedicke et al. (2018) FrASS, 5, A13. Kwiatkowski et al. (2009), A&A, 495, 967. Tricarico et al. (2017), Icarus, 284, 416. et al.: and Anlaug Amanda Djupvik (12), Daniel M. Faes (13), Dora Föhring (4), Joel Roediger (14), Tom Seccull (13) and Adam Smith (13) Powered by TCPDF (www.tcpdf.org).
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