The Discovery and Characterization of Minimoon 2024 PT5
Minimoons are asteroids that become temporarily captured by the Earth–Moon system. We present the discovery of 2024 PT _5 , a minimoon discovered by the Asteroid Terrestrial-impact Last Alert System Sutherland telescope on 2024 August 7. The minimoon with heliocentric semimajor axis, a ~ 1.01 au, a...
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2025-01-01
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Online Access: | https://doi.org/10.3847/2041-8213/ada1d0 |
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author | Bryce T. Bolin Larry Denneau Laura-May Abron Robert Jedicke Kristin Chiboucas Carl Ingebretsen Brian C. Lemaux |
author_facet | Bryce T. Bolin Larry Denneau Laura-May Abron Robert Jedicke Kristin Chiboucas Carl Ingebretsen Brian C. Lemaux |
author_sort | Bryce T. Bolin |
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description | Minimoons are asteroids that become temporarily captured by the Earth–Moon system. We present the discovery of 2024 PT _5 , a minimoon discovered by the Asteroid Terrestrial-impact Last Alert System Sutherland telescope on 2024 August 7. The minimoon with heliocentric semimajor axis, a ~ 1.01 au, and perihelion, q ~ 0.99 au, became captured by the Earth–Moon system on 2024 September 29 and left on 2024 November 25 UTC. Visible g , r , i , and Z spectrophotometry was obtained using Gemini North/Gemini Multi-Object Spectrograph on 2024 September 27. The color indices are g − r = 0.58 ± 0.04, r − i = 0.29 ± 0.04, and i − Z = −0.27 ± 0.06, and the spectrum best matches lunar rock samples followed by S-complex asteroids. Assuming an albedo of 0.21 and using our measured absolute magnitude of 28.64 ± 0.04, 2024 PT _5 has a diameter of 5.4 ± 1.2 m. We also detect variations in the lightcurve of 2024 PT _5 with a 0.28 ± 0.07 mag amplitude and a double-peaked period of ~2600 ± 500 s. We improve the orbital solution of 2024 PT _5 with our astrometry and estimate the effect of radiation pressure on its deriving an area-to-mass ratio of 7.02 ± 2.05 × 10 ^−5 m ^2 kg ^−1 , implying a density of ~3.9 ± 2.1 g cm ^−3 , compatible with having a rocky composition. If we assume 2024 PT _5 is from the near-Earth object (NEO) population, its most likely sources are resonances in the inner Main Belt when we compare its orbit with the NEO population model though this does not exclude a lunar origin. |
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spelling | doaj-art-d31336b79b95498eaa406143f304b64e2025-01-09T13:55:46ZengIOP PublishingThe Astrophysical Journal Letters2041-82052025-01-019782L3710.3847/2041-8213/ada1d0The Discovery and Characterization of Minimoon 2024 PT5Bryce T. Bolin0https://orcid.org/0000-0002-4950-6323Larry Denneau1https://orcid.org/0000-0002-7034-148XLaura-May Abron2https://orcid.org/0009-0000-8709-5273Robert Jedicke3https://orcid.org/0000-0001-7830-028XKristin Chiboucas4https://orcid.org/0000-0002-9020-5004Carl Ingebretsen5https://orcid.org/0000-0002-7053-5495Brian C. Lemaux6https://orcid.org/0000-0002-1428-7036Eureka Scientific , Oakland, CA 94602, USAInstitute for Astronomy, University of Hawai‘i at Mānoa , Honolulu, HI 96822, USAGriffith Observatory , Los Angeles, CA 90027, USAInstitute for Astronomy, University of Hawai‘i at Mānoa , Honolulu, HI 96822, USAGemini Observatory/NSF NOIRLab , Hilo, HI 96720, USAWilliam H. Miller III Department of Physics and Astronomy, Johns Hopkins University , Baltimore, MD 21218, USAGemini Observatory/NSF NOIRLab , Hilo, HI 96720, USA; Department of Physics and Astronomy, University of California, Davis , 1 Shields Ave., Davis, CA 95616, USAMinimoons are asteroids that become temporarily captured by the Earth–Moon system. We present the discovery of 2024 PT _5 , a minimoon discovered by the Asteroid Terrestrial-impact Last Alert System Sutherland telescope on 2024 August 7. The minimoon with heliocentric semimajor axis, a ~ 1.01 au, and perihelion, q ~ 0.99 au, became captured by the Earth–Moon system on 2024 September 29 and left on 2024 November 25 UTC. Visible g , r , i , and Z spectrophotometry was obtained using Gemini North/Gemini Multi-Object Spectrograph on 2024 September 27. The color indices are g − r = 0.58 ± 0.04, r − i = 0.29 ± 0.04, and i − Z = −0.27 ± 0.06, and the spectrum best matches lunar rock samples followed by S-complex asteroids. Assuming an albedo of 0.21 and using our measured absolute magnitude of 28.64 ± 0.04, 2024 PT _5 has a diameter of 5.4 ± 1.2 m. We also detect variations in the lightcurve of 2024 PT _5 with a 0.28 ± 0.07 mag amplitude and a double-peaked period of ~2600 ± 500 s. We improve the orbital solution of 2024 PT _5 with our astrometry and estimate the effect of radiation pressure on its deriving an area-to-mass ratio of 7.02 ± 2.05 × 10 ^−5 m ^2 kg ^−1 , implying a density of ~3.9 ± 2.1 g cm ^−3 , compatible with having a rocky composition. If we assume 2024 PT _5 is from the near-Earth object (NEO) population, its most likely sources are resonances in the inner Main Belt when we compare its orbit with the NEO population model though this does not exclude a lunar origin.https://doi.org/10.3847/2041-8213/ada1d0Near-Earth objectsSmall Solar System bodies |
spellingShingle | Bryce T. Bolin Larry Denneau Laura-May Abron Robert Jedicke Kristin Chiboucas Carl Ingebretsen Brian C. Lemaux The Discovery and Characterization of Minimoon 2024 PT5 The Astrophysical Journal Letters Near-Earth objects Small Solar System bodies |
title | The Discovery and Characterization of Minimoon 2024 PT5 |
title_full | The Discovery and Characterization of Minimoon 2024 PT5 |
title_fullStr | The Discovery and Characterization of Minimoon 2024 PT5 |
title_full_unstemmed | The Discovery and Characterization of Minimoon 2024 PT5 |
title_short | The Discovery and Characterization of Minimoon 2024 PT5 |
title_sort | discovery and characterization of minimoon 2024 pt5 |
topic | Near-Earth objects Small Solar System bodies |
url | https://doi.org/10.3847/2041-8213/ada1d0 |
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