Английская Википедия:1412 Lagrula
1412 Lagrula, provisional designation Шаблон:Mp, is an asteroid from the inner regions of the asteroid belt, approximately 7 or 23 kilometers in diameter, depending on the body's divergent reflectivity measurements.
It was discovered on 19 January 1937, by French astronomer Louis Boyer at the North African Algiers Observatory in Algeria.[1] It was later named after French astronomer Philippe Lagrula.[2]
Classification and orbit
Lagrula is a presumed member of the Flora family, a large group of stony S-type asteroids in the inner main-belt. It orbits the Sun at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,204 days). Its orbit has an eccentricity of 0.11 and an inclination of 5° with respect to the ecliptic.[3] First identified as Шаблон:Mp at Lowell Observatory in 1929, the body's observation arc was extended by 8 years prior to its official discovery observation at Algiers.[1]
Physical characteristics
Photometry
During March and April 2013, photometric observations of Lagrula were made over ten nights by Italian astronomer Giovanni Casalnuovo at Eurac Observatory (Шаблон:Small) in Bolzano, Italy. Lightcurve analysis gave a rotation period of 5.9176 hours and a brightness variation of 0.28 magnitude (Шаблон:Small).[4] In January 2016, a more refined period of 5.882 hours with an amplitude of 0.44 magnitude was obtained from a bimodal lightcurve by Spanish astronomer group OBAS, Observadores de Asteroides (Шаблон:Small).[5]
Diameter and albedo
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Lagrula measures 7.8 kilometers in diameter, and its surface has an albedo of 0.318 and 0.36, respectively (most recent results only).[6][7] However, the Collaborative Asteroid Lightcurve Link assumes a carbonaceous albedo of 0.058 and calculates a diameter of 23.98 kilometers,[8] which is in agreement with Giovanni Casalnuovo, who published a diameter of Шаблон:Val and an albedo of 0.06 using an absolute magnitude of 11.81.[4] Casalnuovo assumed a C-type, rather than an S-type, because he found an average V–R color index of Шаблон:Val magnitude.[4]
Naming
This minor planet was named after French astronomer Joanny-Philippe Lagrula (1870–1941), discoverer of the minor planet 775 Lumière and director of the Quito Astronomical Observatory and Algiers Observatory.[2] Naming citation was neither published in The Names of the Minor Planets nor in the Minor Planet Circulars, but researched and compiled by astronomer and author Lutz D. Schmadel, based on his private communications with his colleges (Шаблон:Small).[9]
References
External links
- Asteroid Lightcurve Database (LCDB), query form (info Шаблон:Webarchive)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- Шаблон:AstDys
- Шаблон:JPL small body
Шаблон:Use dmy dates Шаблон:Minor planets navigator Шаблон:Small Solar System bodies
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- Английская Википедия
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- Discoveries by Louis Boyer (astronomer)
- Named minor planets
- Astronomical objects discovered in 1937
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