The Asteroid 2014 JO25

Quijano-Vodniza, Alberto Y Rojas P., Mario (2017) The Asteroid 2014 JO25. In: 49th ANNUAL DIVISION FOR PLANETARY SCIENCES MEETING, 15 a 20 de Octubre del 2017, Provo, Utah, USA.

Text (POSTER DIGITALsustentado Oralmente) 2017DPS....4911702V/abstract - Accepted Version Download (38kB)

Resumen

The asteroid 2014 JO25 was discovered by A. D. Grauer at the Mt. Lemmon Survey on May 2014, and Joe Masiero used observations from the NEOWISE in 2014 to estimate a diameter of 650 meters [1]. However, using the radio telescope at Arecibo-Puerto Rico, astronomers obtained radar images on April 17-2017 and Edgar Rivera Valentín (scientist at Arecibo) said: “We found 2014 JO25 is a contact binary asteroid, two space rocks that were originally separate bodies, and each segment is about 640 meters and 670 meters, for a total of about 1.3 km long. Its rotation is of 3.5 hours” [2]. This asteroid flew past Earth on April 19 at a distance of about 4.6 lunar distances from the Earth. This was the closest approach by an asteroid since 4179 Toutatis. Toutatis flew past Earth on September 2004 at a distance of about 4 lunar distances from the Earth [3]. In April 12-2020 the asteroid will be at a minimum possible distance of 0.1617280 A.U from Earth [4]. From our observatory, located in Pasto-Colombia, we obtained a lot of pictures. Our data was published by the Minor Planet Center [5] and also appears at the web page of NEODyS [6]. Astrometry and photometry were carried out, and we calculated the orbital elements.

Tipo de Elemento:	Conferencia o Taller artículo (Poster)
Palabras Clave:	Asteroide, Observatorio Astronómico de Pasto, NASA, Alberto Quijano Vodniza
Asunto:	Q Ciencias > QB Astronomy Q Ciencias > QC Physics
Division:	Facultad de Ciencias Exactas y Naturales > Programa de Física > Productividad
Depósito de Usuario:	MASTER ALBERTO QUIJANO VODNIZA
Fecha Deposito:	19 Abr 2021 14:20
Ultima Modificación:	19 Abr 2021 14:20
URI:	http://sired.udenar.edu.co/id/eprint/7009

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