Size, Shape, Density, and Atmospheric Limit of (50000) Quaoar Revealed from 14 years of Stellar Occultation


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Margoti G., Braga-Ribas F., Ortiz J. L., Sicardy B., Desmars J., Morgado B., ...Daha Fazla

Astrophysical Journal, cilt.1008, sa.2, 2026 (SCI-Expanded, Scopus)

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 1008 Sayı: 2
  • Basım Tarihi: 2026
  • Doi Numarası: 10.3847/1538-4357/ae907e
  • Dergi Adı: Astrophysical Journal
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus, INSPEC, zbMATH, Directory of Open Access Journals, Academic Search Ultimate (EBSCO)
  • Anahtar Kelimeler: Classical Kuiper belt objects (250), Kuiper belt (893), Small Solar System bodies (1469), Stellar occultation (2135), Trans-Neptunian objects (1705)
  • Açık Arşiv Koleksiyonu: AVESİS Açık Erişim Koleksiyonu
  • Ankara Üniversitesi Adresli: Evet

Özet

We present results from 28 stellar occultations by the large trans-Neptunian object (50000) Quaoar registered between 2018 and 2025. By performing a joint analysis of this occultation dataset, along with nine other published events, we were able to fit an oblate ellipsoid shape, with equatorial semiaxes a and b of (Formula presented) 566.1−2.2+2.5 km, and a polar semiaxis, c, of (Formula presented) 511.2−3.7+3.6 km. It provides an equivalent volumetric diameter of 1094.4 ± 4.6 km and polar oblateness of 0.097 ± 0.011. Considering an absolute magnitude of H = 2.79 ± 0.35, we derive a geometric albedo of pV = 0.125 ± 0.038. We have derived new upper limits to the surface pressure of a CH4 atmosphere of 0.15 nbar (1σ) and 0.65 nbar (3σ). We also provide a table with the 36 new astrometric positions for Quaoar. Using the new system mass derived from Weywot’s orbit around Quaoar, we calculated a density of 1.760 ± 0.109 g cm−3. Moreover, from the derived size and rotation period (8.8394 ± 0.0002 hr, we calculated that, if Quaoar is in Maclaurin hydrostatic equilibrium state, it would have a density of 1.859 ± 0.200 g cm−3. This result, within the error bars, is compatible with the value we found. Therefore, this work shows that Quaoar can be a Maclaurin object, being eligible as a dwarf planet.