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  Photometric Analysis of the Nucleus of the Main-belt Comet 2010 LH15

Mastropietro, M., Krishna, H., Kim, Y., & Agarwal, J. (2024). Photometric Analysis of the Nucleus of the Main-belt Comet 2010 LH15. Research Notes of the American Astronomical Society, 8, 104. doi:10.3847/2515-5172/ad3e85.

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 Creators:
Mastropietro, M.1, Author           
Krishna, H., Author
Kim, Y., Author
Agarwal, J.2, Author           
Affiliations:
1IMPRS for Solar System Science at the University of Göttingen, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832290              
2Planetary Science Department, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              

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Free keywords: Comet nuclei; Astronomy data analysis; Small Solar System bodies; Main-belt comets; Comets; Asteroids; 2160; 1858; 1469; 2131; 280; 72
 Abstract: We analyzed the inactive nucleus of the main-belt comet 2010 LH15 at a true anomaly of 262°. Observations using the Gemini North Telescope in 2023 July yielded an absolute R-band magnitude of (18.4 ± 0.2) mag. Assuming a C-type geometric albedo and phase function, we estimated the nucleus radius to be (0.5 ± 0.1) km. The examination of the lightcurve profile did not yield clear evidence for a rotational period shorter than 2 hr.

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 Dates: 2024
 Publication Status: Issued
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 Identifiers: DOI: 10.3847/2515-5172/ad3e85
ISSN: 2515-5172
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Title: Research Notes of the American Astronomical Society
Source Genre: Journal
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Publ. Info: IOP
Pages: - Volume / Issue: 8 Sequence Number: - Start / End Page: 104 Identifier: -