Search: WFRF:(Fitzsimmons Alan) > (2010-2014) > A collision in 2009...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 03052naa a2200529 4500 | |
001 | oai:DiVA.org:uu-133854 | |
003 | SwePub | |
008 | 101116s2010 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-1338542 URI |
024 | 7 | a https://doi.org/10.1038/nature094532 DOI |
040 | a (SwePub)uu | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Snodgrass, Colin4 aut |
245 | 1 0 | a A collision in 2009 as the origin of the debris trail of asteroid P/2010 A2 |
264 | c 2010-10-13 | |
264 | 1 | b Springer Science and Business Media LLC,c 2010 |
338 | a print2 rdacarrier | |
520 | a The peculiar object P/2010 A2 was discovered(1) in January 2010 and given a cometary designation because of the presence of a trail of material, although there was no central condensation or coma. The appearance of this object, in an asteroidal orbit (small eccentricity and inclination) in the inner main asteroid belt attracted attention as a potential new member of the recently recognized(2) class of main-belt comets. If confirmed, this new object would expand the range in heliocentric distance over which main-belt comets are found. Here we report observations of P/2010 A2 by the Rosetta spacecraft. We conclude that the trail arose from a single event, rather than a period of cometary activity, in agreement with independent results(3). The trail is made up of relatively large particles of millimetre to centimetre size that remain close to the parent asteroid. The shape of the trail can be explained by an initial impact ejecting large clumps of debris that disintegrated and dispersed almost immediately. We determine that this was an asteroid collision that occurred around 10 February 2009. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a Physics | |
653 | a Fysik | |
700 | 1 | a Tubiana, Cecilia4 aut |
700 | 1 | a Vincent, Jean-Baptiste4 aut |
700 | 1 | a Sierks, Holger4 aut |
700 | 1 | a Hviid, Stubbe4 aut |
700 | 1 | a Moissl, Richard4 aut |
700 | 1 | a Boehnhardt, Hermann4 aut |
700 | 1 | a Barbieri, Cesare4 aut |
700 | 1 | a Koschny, Detlef4 aut |
700 | 1 | a Lamy, Philippe4 aut |
700 | 1 | a Rickman, Hansu Uppsala universitet,Teoretisk astrofysik4 aut0 (Swepub:uu)hansrick |
700 | 1 | a Rodrigo, Rafael4 aut |
700 | 1 | a Carry, Benoit4 aut |
700 | 1 | a Lowry, Stephen C.4 aut |
700 | 1 | a Laird, Ryan J. M.4 aut |
700 | 1 | a Weissman, Paul R.4 aut |
700 | 1 | a Fitzsimmons, Alan4 aut |
700 | 1 | a Marchi, Simone4 aut |
710 | 2 | a Uppsala universitetb Teoretisk astrofysik4 org |
773 | 0 | t Natured : Springer Science and Business Media LLCg 467:7317, s. 814-816q 467:7317<814-816x 0028-0836x 1476-4687 |
856 | 4 | u http://arxiv.org/pdf/1010.2883 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-133854 |
856 | 4 8 | u https://doi.org/10.1038/nature09453 |
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
Copy and save the link in order to return to this view