288P/300163
Appearance
![](https://cdn.statically.io/img/upload.wikimedia.org/wikipedia/commons/thumb/5/55/The_binary_asteroid_288P_%28artist%E2%80%99s_impression%29.jpg/220px-The_binary_asteroid_288P_%28artist%E2%80%99s_impression%29.jpg)
![](https://cdn.statically.io/img/upload.wikimedia.org/wikipedia/commons/thumb/c/c3/2006VW139.gif/220px-2006VW139.gif)
288P/300163 (2006 VW139) inter cometas, 300163 (2006 VW139) inter asteroides appellatus, est systema binarium asteroidum quod in cingulum principale circuitur, corporibus duobus massa fere aequalibus sibi 100 chm. distantibus, a quo systemate cauda (sicut a cometibus) eiicitur.
Asteroides, nondum in duos distinctus, die 15 Novembris 2006 ab Spacewatch observatorii Kitt Peak repertus est. Inter cometas classificatus est, observationibus Pan-STARRS, mense Novembri 2011. Res de systemate binario, ope imaginum telescopii Hubbleani recognito, die 21 Septembris 2017 divulgata est.
Bibliographia[recensere | fontem recensere]
- Jessica Agarwal, David Jewitt, Max Mutchler, Harold Weaver, Stephen Larson, "A binary main belt comet" in Nature vol. 549 pp. 357–359 (21 Septembris 2017)
Nexus externi[recensere | fontem recensere]
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Data astronomica: "20300163" apud JPL Small-Body Database. |