Английская Википедия:15094 Polymele

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Шаблон:Infobox planet

15094 Polymele Шаблон:IPAc-en is a primitive Jupiter trojan from the Greek camp, approximately Шаблон:Convert in diameter. It is a target of the Lucy mission with a close flyby planned to occur in September 2027.[1][2] It was discovered on 17 November 1999, by astronomers with the Catalina Sky Survey at Mount Lemmon Observatory, Arizona, in the United States. The P-type asteroid has a rotation period of 5.9 hours and highly flattened shape.[3][4] It was named after Polymele from Greek mythology, the wife of Menoetius and the mother of Patroclus.[5] In 2022, it was reported to have a natural satellite approximately Шаблон:Convert in diameter.[6]

Orbit and classification

Polymele is a Jupiter trojan asteroid orbiting in the leading Greek camp at Jupiter's Шаблон:L4 Lagrangian point, 60° ahead of the gas giant's orbit (see Trojans in astronomy). It orbits the Sun at a distance of 4.7–5.7 AU once every 11 years and 9 months (4,289 days; semi-major axis of 5.17 AU). Its orbit has an eccentricity of 0.09 and an inclination of 13° with respect to the ecliptic.[7] The asteroid's observation arc begins 48 years prior to its official discovery observation at Mount Lemmon, with a precovery taken at Palomar Observatory in 1951, and published by the Digitized Sky Survey later on.[5]

Naming

This minor planet was named after Polymele, the daughter of Peleus from Greek mythology. According to the Latin author Gaius Julius Hyginus (Шаблон:Circa 64 BC – AD 17), she is the wife of the Argonaut Menoetius and the mother of Patroclus, who participated in the Trojan War.[5] Polymele is also known as "Philomela"; that name was previously used for the asteroid 196 Philomela. The approved naming citation was published by the Minor Planet Center on 22 February 2016 (Шаблон:Small).[8]

Physical characteristics

Polymele has been characterized as a primitive P-type asteroid by the investigators of the Lucy mission.[1] P-type asteroids are known for their low albedo. It has a V–I color index of 0.799,[9] which is lower than that for most larger Jupiter trojans (see table below).

Size, shape, and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Polymele measures 21.075 kilometers in diameter and its surface has an albedo of 0.091,[10][11][12] while in 2018, Marc Buie published an albedo of 0.073 and an absolute magnitude of 11.691 in the S- and/or R band.[13] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a larger diameter of 26.64 kilometers based on an absolute magnitude of 11.6.[14]

On 27 March 2022, multiple astronomers observed a stellar occultation by Polymele, which revealed an apparently elongated projected shape with projected dimensions of Шаблон:Cvt.[3] Additional occultation observations of Polymele from 2020–2023 revealed that Polymele's true shape is a highly flattened disk with dimensions Шаблон:Cvt, similar to the large flat lobe of the Kuiper belt object 486958 Arrokoth.[4] This unusual flattened shape of Polymele implies that it had retained its original shape from when it formed by accretion.[4]

Rotation

In March 2016, a rotational lightcurve of Polymele was obtained from photometric observations by Marc Buie and colleges. Lightcurve analysis gave a rotation period of Шаблон:Val hours with a small brightness amplitude of Шаблон:Val magnitude (Шаблон:Small), which indicates the body is being viewed pole-on.[13] Previously, the Lucy mission team published spin rates of 6.1 and 4 hours, respectively.[1][2]

The resolved observation of Polymele's shape in multiple occultation events allowed the Lucy team to determine the orientation of Polymele's rotational pole.[15] Polymele's rotational north pole points toward ecliptic latitude –80.9°, which corresponds to an axial tilt of 170.9° with respect to the ecliptic, making Polymele a retrograde rotator.[15]

Satellite

Файл:Polymele occultation satellite discovery.png
Discovery of Polymele's satellite in the 26 March 2022 occultation

Following observations of an occultation on 26 March 2022, the Lucy mission team reported the discovery of a natural satellite around Polymele. The satellite is a smaller asteroid about Шаблон:Convert in diameter, orbiting nearly in the equatorial plane of Polymele at a distance of Шаблон:Cvt.[3][15] Assuming Polymele has a density of Шаблон:Val, the satellite should have an orbital period between 14.4 and 16.6 days.[15] It will not be assigned a formal name until further observations determine its orbit.[16] The Lucy team refers to the companion by the temporary informal name "Shaun," after Aardman Animations' animated sheep.[6] The satellite was detected again in an occultation on 4 February 2023,[4] in the largest organized occultation expedition in history. Nearly 200 astronomers across two continents participated in the campaign.[17]

Exploration

Lucy mission target

Polymele is planned to be visited by the Lucy spacecraft which launched in 2021. The flyby is scheduled for 15 September 2027, and will approach the asteroid to a distance of Шаблон:Cvt at a relative velocity of Шаблон:Cvt.[1]

References

Шаблон:Reflist

External links

Шаблон:Use dmy dates Шаблон:Minor planets navigator Шаблон:Small Solar System bodies

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  1. ↑ 1,0 1,1 1,2 1,3 Ошибка цитирования Неверный тег <ref>; для сносок Levison-2017 не указан текст
  2. ↑ 2,0 2,1 Ошибка цитирования Неверный тег <ref>; для сносок Buie-2016 не указан текст
  3. ↑ 3,0 3,1 3,2 Ошибка цитирования Неверный тег <ref>; для сносок Buie2022 не указан текст
  4. ↑ 4,0 4,1 4,2 4,3 Ошибка цитирования Неверный тег <ref>; для сносок Buie2023 не указан текст
  5. ↑ 5,0 5,1 5,2 Ошибка цитирования Неверный тег <ref>; для сносок MPC-object не указан текст
  6. ↑ 6,0 6,1 Ошибка цитирования Неверный тег <ref>; для сносок Polymele-companion не указан текст
  7. ↑ Ошибка цитирования Неверный тег <ref>; для сносок jpldata не указан текст
  8. ↑ Ошибка цитирования Неверный тег <ref>; для сносок MPC-Circulars-Archive не указан текст
  9. ↑ Ошибка цитирования Неверный тег <ref>; для сносок Hainaut-2012 не указан текст
  10. ↑ Ошибка цитирования Неверный тег <ref>; для сносок Grav-2012 не указан текст
  11. ↑ Ошибка цитирования Неверный тег <ref>; для сносок Mainzer-2016 не указан текст
  12. ↑ Ошибка цитирования Неверный тег <ref>; для сносок WISE не указан текст
  13. ↑ 13,0 13,1 Ошибка цитирования Неверный тег <ref>; для сносок Buie-2018 не указан текст
  14. ↑ Ошибка цитирования Неверный тег <ref>; для сносок lcdb не указан текст
  15. ↑ 15,0 15,1 15,2 15,3 Ошибка цитирования Неверный тег <ref>; для сносок Levison2023 не указан текст
  16. ↑ Шаблон:Cite web
  17. ↑ Шаблон:Cite web
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