Английская Википедия:4007 Euryalos
4007 Euryalos Шаблон:IPAc-en is a larger Jupiter trojan from the Greek camp, approximately Шаблон:Convert in diameter. It was discovered on 19 September 1973, by Dutch astronomers Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observatory in California.[1] The likely spherical Jovian asteroid is the principal body of the proposed Euryalos family and has a rotation period of 6.4 hours.[2] It was named after the warrior Euryalus from Greek mythology.[1]
Orbit and classification
Euryalos is a dark Jovian asteroid in a 1:1 orbital resonance with Jupiter. It is located in the leading Greek camp at the Gas Giant's Шаблон:L4 Lagrangian point, 60° ahead on its orbit Шаблон:Cross reference.[3] It orbits the Sun at a distance of 4.9–5.5 AU once every 11 years and 9 months (4,301 days; semi-major axis of 5.18 AU). Its orbit has an eccentricity of 0.06 and an inclination of 11° with respect to the ecliptic.[4] The body's observation arc begins with its official discovery observation at Palomar in September 1976.[1]
Euryalos family
Fernando Roig and Ricardo Gil-Hutton identified Euryalos as the principal body of a small Jovian asteroid family, using the hierarchical clustering method (HCM), which looks for groupings of neighboring asteroids based on the smallest distances between them in the proper orbital element space. According to the astronomers, the Euryalos family belongs to the larger Menelaus clan, an aggregation of Jupiter trojans which is composed of several families, similar to the Flora family in the inner asteroid belt.[5]Шаблон:Rp
However this family is not included in David NesvornýШаблон:'s HCM-analysis from 2014.[6] Instead, Euryalos is listed as a non-family asteroid of the Jovian background population on the Asteroids Dynamic Site (AstDyS) which based on another analysis by Milani and Knežević.[7]
Palomar–Leiden Trojan survey
Despite being discovered during the second Palomar–Leiden Trojan survey in 1973, Euryalos has not received a provisional survey designation prefixed with "T-2". The survey was a fruitful collaboration between the Palomar and Leiden observatories during the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand asteroids.[8]
Naming
This minor planet was named from Greek mythology after the warrior Euryalos, the leader of the Greek contingent from Argos during the Trojan War.[1] The official naming citation was published by the Minor Planet Center on 11 March 1990 (Шаблон:Small).[9]
Physical characteristics
Euryalos is an assumed C-type asteroid, while the majority of larger Jupiter trojans are D-type asteroids.[2]
Rotation period
In August 1995, a rotational lightcurve of Euryalos was obtained from photometric observations over four nights by Italian astronomer Stefano Mottola using the Bochum 0.61-metre Telescope at ESO's La Silla Observatory in Chile. Lightcurve analysis gave a well-defined rotation period of Шаблон:Val hours with a low brightness amplitude of 0.07 magnitude (Шаблон:Small), indicative of a spherical rather than elongated shape.[2][10]
Diameter and albedo
According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer and the Japanese Akari satellite, Euryalos measures 45.52 and 53.89 kilometers in diameter and its surface has an albedo of 0.065 and 0.061, respectively.[11][12] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 48.48 kilometers based on an absolute magnitude of 10.3.[2]
Шаблон:Largest Jupiter trojans
References
External links
- Asteroid Lightcurve Database (LCDB), query form (info Шаблон:Webarchive)
- Dictionary of Minor Planet Names, Google books
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- Asteroid 4007 Euryalos at the Small Bodies Data Ferret
- Шаблон:AstDys
- Шаблон:JPL small body
Шаблон:Use dmy dates Шаблон:Minor planets navigator Шаблон:Small Solar System bodies
- ↑ 1,0 1,1 1,2 1,3 Ошибка цитирования Неверный тег
<ref>
; для сносокMPC-object
не указан текст - ↑ 2,0 2,1 2,2 2,3 Ошибка цитирования Неверный тег
<ref>
; для сносокlcdb
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокMPC-Jupiter-Trojans
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокjpldata
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокRoig-2008
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокNesvorny-2014
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокAstDys-object
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокMPC-discoverers
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокMPC-Circulars-Archive
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокMottola-2011
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокGrav-2012
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокAKARI
не указан текст
- Английская Википедия
- Jupiter trojans (Greek camp)
- Discoveries by Cornelis Johannes van Houten
- Discoveries by Ingrid van Houten-Groeneveld
- Discoveries by Tom Gehrels
- Named minor planets
- Astronomical objects discovered in 1973
- Страницы, где используется шаблон "Навигационная таблица/Телепорт"
- Страницы с телепортом
- Википедия
- Статья из Википедии
- Статья из Английской Википедии
- Страницы с ошибками в примечаниях