Английская Википедия:809 Lundia

Материал из Онлайн справочника
Версия от 14:09, 26 декабря 2023; EducationBot (обсуждение | вклад) (Новая страница: «{{Английская Википедия/Панель перехода}} {{Use dmy dates|date=October 2019}} {{Infobox planet | minorplanet=yes | background=#D6D6D6 | name=809 Lundia | image = 809Lun-LB1-mag17.jpg | image_size = 245 | caption=Asteroid 809 Lundia (apparent magnitude 16.6) near a mag 15.6 star | discoverer=Max Wolf | discovered=11 August 1915 | mpc_name=(809) Lundia | alt_names=1915 XP; 1936 VC | named_after=Lund Observat...»)
(разн.) ← Предыдущая версия | Текущая версия (разн.) | Следующая версия → (разн.)
Перейти к навигацииПерейти к поиску

Шаблон:Use dmy dates Шаблон:Infobox planet

809 Lundia is a small, binary, V-type asteroid[1] orbiting within the Flora family in the main belt. It is named after Lund Observatory, Sweden.

Characteristics

Lundia orbits within the Flora family. However, its V-type spectrum indicates that it is not genetically related to the Flora family, but rather is probably a fragment (two fragments, if its moon is included) ejected from the surface of 4 Vesta by a large impact in the past. Its orbit lies too far from Vesta for it to actually be a member of the Vesta family. It is not clear how it arrived at an orbit so far from Vesta, but other examples of V-type asteroids orbiting fairly far from their parent body are known. A mechanism of interplay between the Yarkovsky effect and nonlinear secular resonances (primarily involving Jupiter and Saturn) has been proposed.[2]

Binary system

Lightcurve observations in 2005 revealed that Lundia is a binary system of two similarly sized objects orbiting their common centre of gravity. "Lundia" now refers to one of the objects, the other being provisionally designated S/2005 (809) 1. The similarity of size between the two components is suspected because during mutual occultations the brightness drops by a similar amount independently of which component is hidden.[3] Due to the similar size of the primary and secondary the Minor Planet Center lists this as a binary companion.[4]

Assuming an albedo similar to 4 Vesta (around 0.4) suggests that the components are about 7 km across. They orbit each other in a period of 15.4 hours,[3] which roughly indicates that the separation between them is very close: to the order of 10–20 km if typical asteroid albedo and density values are assumed.

References

Шаблон:Reflist

External links

Шаблон:Minor planets navigator Шаблон:Small Solar System bodies Шаблон:Authority control