Английская Википедия:(55637) 2002 UX25

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Шаблон:Short description Шаблон:Use dmy dates

Шаблон:Infobox planet

Шаблон:Mp is a trans-Neptunian object that orbits the Sun in the Kuiper belt beyond Neptune. It briefly garnered scientific attention when it was found to have an unexpectedly low density of about 0.82 g/cm3.[1]

Шаблон:Mp has an absolute magnitude of about 4.0,[2] and Spitzer Space Telescope results estimate it to be about 681 km in diameter.[3] The low density of this and many other mid sized TNOs implies that they have likely never compressed into fully solid bodies, let alone differentiated or collapsed into hydrostatic equilibrium, and so are highly unlikely to be dwarf planets.[4]

It was discovered on 30 October 2002, by the Spacewatch program.[5]

Numbering and naming

This minor planet was numbered (55637) by the Minor Planet Center on 16 February 2003 (Шаблон:Small).[6] Шаблон:As of, it has not been named.[7]

Classification

Файл:UX25-LB1-2009Nov19-06UT.jpg
Шаблон:Mp (vmag 19.9) as viewed with a 24" telescope

Шаблон:Mp has a perihelion of 36.7 AU,[2] which it will next reach in 2065.[2] As of 2020, Шаблон:Mp is 40 AU from the Sun.[8]

The Minor Planet Center classifies Шаблон:Mp as a cubewano[9] while the Deep Ecliptic Survey (DES) classifies it as scattered-extended.[10] The DES using a 10 My integration (last observation: 2009-10-22) shows it with a minimum perihelion (qmin) distance of 36.3 AU.[10]

It has been observed 212 times with precovery images dating back to 1991.[2]

Physical characteristics

A variability of the visual brightness was detected which could be fit to a period of 14.38 or 16.78 h (depending on a single-peaked or double peaked curve).[11] The light-curve amplitude is ΔM = Шаблон:Val.[12]

The analysis of combined thermal radiometry of Шаблон:Mp from measurements by the Spitzer Space Telescope and Herschel Space Telescope indicates an effective diameter of Шаблон:Nowrap and albedo of 0.107Шаблон:±. Assuming equal albedos for the primary and secondary it leads to the size estimates of ~664 km and ~190 km, respectively. If the albedo of the secondary is half of that of the primary the estimates become ~640 and ~260 km, respectively.[13] Using an improved thermophysical model slightly different sizes were obtained for UX25 and its satellite: 659 km and 230 km, respectively.[14]

Шаблон:Mp has red featureless spectrum in the visible and near-infrared but has a negative slope in the K-band, which may indicate the presence of the methanol compounds on the surface.[15] It is redder than Varuna, unlike its neutral-colored "twin" Шаблон:Mpl, in spite of similar brightness and orbital elements.

Composition

With a density of 0.82 g/cm3, assuming that the primary and satellite have the same density, Шаблон:Mp is one of the largest known solid objects in the Solar System that is less dense than water.[1] Why this should be is not well understood, because objects of its size in the Kuiper belt often contain a fair amount of rock and are hence pretty dense. To have a similar composition to others large KBOs, it would have to be exceptionally porous, which was believed to be unlikely given the compactability of water ice;[13] this low density thus astonished astronomers.[1] Studies by Grundy et al. suggest that at the low temperatures that prevail beyond Neptune, ice is brittle and can support significant porosity in objects significantly larger than Шаблон:Mp, particularly if rock is present; the low density could thus be a consequence of this object failing to warm sufficiently during its formation to significantly deform the ice and fill these pore spaces.[16]

Density comparison
What Density
(g/cm3) 		Notes
Settled snow 0.2–0.3 [17]
Slush/firn 0.7–0.8 [17]
Шаблон:Mp 0.82 [13]
Glacier ice 0.83–0.92 [17]
Tethys 0.984 [18]
Liquid water 1 [17]

Satellite

Файл:2002 UX25 moon-orbit.png
A simulated circular orbit of 210-km-diameter moon at a distance of 4770 km

Шаблон:Anchor Шаблон:Infobox planet The discovery of a minor-planet moon was reported in IAUC 8812 on 22 February 2007.[19] The satellite was detected using the Hubble Space Telescope in August 2005.[19] The satellite was found at 0.16 arcsec from the primary with an apparent magnitude difference of 2.5.[20] It orbits the primary in Шаблон:Val days,[12] at a distance of Шаблон:Val, yielding a system mass of Шаблон:Val.[13][12] The eccentricity of the orbit is Шаблон:Val.[12]

This moon is estimated to be Шаблон:Val in diameter.[15] Assuming the same albedo as the primary, it would have a diameter of 190 km, assuming an albedo of 0.05 (typical of other cold, classical KBOs of similar size) a diameter of 260 km.[13]

References

Шаблон:Reflist

External links

Шаблон:Minor planets navigator Шаблон:Dwarf planets Шаблон:Solar System moons (compact) Шаблон:Small Solar System bodies Шаблон:Solar System Шаблон:Trans-Neptunian objects Шаблон:Authority control

Партнерские ресурсы
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Разное

  1. ↑ 1,0 1,1 1,2 Ошибка цитирования Неверный тег <ref>; для сносок cowen не указан текст
  2. ↑ 2,0 2,1 2,2 2,3 Ошибка цитирования Неверный тег <ref>; для сносок jpldata не указан текст
  3. ↑ Ошибка цитирования Неверный тег <ref>; для сносок spitzer не указан текст
  4. ↑ W.M. Grundy, K.S. Noll, M.W. Buie, S.D. Benecchi, D. Ragozzine & H.G. Roe, 'The Mutual Orbit, Mass, and Density of Transneptunian Binary Gǃkúnǁʼhòmdímà (Шаблон:Mp)', Icarus (forthcoming, available online 30 March 2019) Шаблон:Webarchive DOI: 10.1016/j.icarus.2018.12.037,
  5. ↑ Ошибка цитирования Неверный тег <ref>; для сносок MPEC2002-V08 не указан текст
  6. ↑ Ошибка цитирования Неверный тег <ref>; для сносок MPC-Circulars-Archive не указан текст
  7. ↑ Ошибка цитирования Неверный тег <ref>; для сносок MPC-object не указан текст
  8. ↑ Ошибка цитирования Неверный тег <ref>; для сносок AstDys не указан текст
  9. ↑ Ошибка цитирования Неверный тег <ref>; для сносок MPEC 2009-C70 не указан текст
  10. ↑ 10,0 10,1 Ошибка цитирования Неверный тег <ref>; для сносок Buie не указан текст
  11. ↑ Ошибка цитирования Неверный тег <ref>; для сносок Rousselot2005 не указан текст
  12. ↑ 12,0 12,1 12,2 12,3 Ошибка цитирования Неверный тег <ref>; для сносок Johnston не указан текст
  13. ↑ 13,0 13,1 13,2 13,3 13,4 Ошибка цитирования Неверный тег <ref>; для сносок Brown2013 не указан текст
  14. ↑ Ошибка цитирования Неверный тег <ref>; для сносок Brown2017 не указан текст
  15. ↑ 15,0 15,1 Ошибка цитирования Неверный тег <ref>; для сносок TNOsCool8 не указан текст
  16. ↑ Шаблон:Cite web
  17. ↑ 17,0 17,1 17,2 17,3 Ошибка цитирования Неверный тег <ref>; для сносок typ не указан текст
  18. ↑ Roatsch Jaumann et al. 2009, p. 765, Tables 24.1–2
  19. ↑ 19,0 19,1 Ошибка цитирования Неверный тег <ref>; для сносок IAUC8812 не указан текст
  20. ↑ Ошибка цитирования Неверный тег <ref>; для сносок EKO51 не указан текст
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