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Phocaea family
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Phocaea family (/foʊˈsiːə/ foh-SEE-ə; adj. Phocaean; FIN: 701) is a collisional family of asteroids located between 2.25 and 2.5 AU in the inner region ofMoons of Haumea (1,767 words) [view diff] exact match in snippet view article find links to article
in a number of ways. They are thought to be part of its extended collisional family, which formed billions of years ago from icy debris after a large571 Dulcinea (171 words) [view diff] exact match in snippet view article find links to article
S-type asteroid and it is the second largest member of the Erigone collisional family. "Dulcinea". Oxford English Dictionary (Online ed.). Oxford University163 Erigone (656 words) [view diff] exact match in snippet view article find links to article
composition. It is the largest member of the eponymously named Erigone collisional family. In the early morning hours of March 20, 2014, Erigone occulted the120347 Salacia (1,510 words) [view diff] exact match in snippet view article find links to article
Neptune. Salacia's orbit is within the parameter space of the Haumea collisional family, but Salacia is not part of it, as evidenced by its lack of the strong(202421) 2005 UQ513 (486 words) [view diff] exact match in snippet view article
it would have been a good candidate to be a member of the Haumea collisional family, given its red spectrum, it is not. As of December 2018, it is currently(145451) 2005 RM43 (626 words) [view diff] case mismatch in snippet view article
W. Tourtellotte (2008). "The Youthful Appearance of the 2003 EL61 Collisional Family". The Astronomical Journal. 136 (4): 1502–1509. arXiv:0804.2864. Bibcode:2008AJTrans-Neptunian object (3,938 words) [view diff] exact match in snippet view article find links to article
Barkume, Kristina M.; Ragozzine, Darin; Schaller, Emily L. (2007). "A collisional family of icy objects in the Kuiper belt" (PDF). Nature. 446 (7133): 294–296(90568) 2004 GV9 (476 words) [view diff] case mismatch in snippet view article
W. Tourtellotte (2008). "The Youthful Appearance of the 2003 EL61 Collisional Family". The Astronomical Journal. 136 (4): 1502–1509. arXiv:0804.2864. Bibcode:2008AJ31 Euphrosyne (690 words) [view diff] exact match in snippet view article find links to article
thick ejecta blanket from the collision that created its moon and collisional family. There are no deep basins. Any craters larger than 40 km in diameter3548 Eurybates (1,937 words) [view diff] exact match in snippet view article find links to article
Jovian asteroids; four of them in the Greek camp. This potentially collisional family was first characterized by Jakub Rozehnal and Miroslav Brož in 20113963 Paradzhanov (657 words) [view diff] exact match in snippet view article find links to article
September 2017. Dykhuis, Melissa J.; Greenberg, Richard (May 2015). "Collisional family structure within the Nysa-Polana complex". Icarus. 252: 199–211. arXiv:1501Effects of Planet Nine on trans-Neptunian objects (4,289 words) [view diff] exact match in snippet view article find links to article
well-known example is in the Haumea collisional family. Another, albeit less-studied case is that of Chiang's collisional family. At least one pair of extreme2708 Burns (817 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1684 Iguassú (815 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1474 Beira (888 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1655 Comas Solà (961 words) [view diff] exact match in snippet view article find links to article
de León, J.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics531 Zerlina (761 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1340 Yvette (993 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1213 Algeria (912 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1508 Kemi (1,173 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics3204 Lindgren (906 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1291 Phryne (1,021 words) [view diff] exact match in snippet view article find links to article
J.; et al. (January 2018). "Spin states of asteroids in the Eos collisional family". Icarus. 299: 84–96. arXiv:1707.05507. Bibcode:2018Icar..299...84H1768 Appenzella (968 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics2039 Payne-Gaposchkin (829 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1444 Pannonia (1,046 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids" (PDF). Astronomy and Astrophysics1796 Riga (1,219 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics988 Appella (1,020 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics3581 Alvarez (1,107 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and AstrophysicsList of minor planets (3,171 words) [view diff] exact match in snippet view article find links to article
(H), are labelled in italics (H), when they are not members of the collisional family near-Earth objects are divided into the Aten (ATE), Amor (AMO), Apollo1003 Lilofee (1,080 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1615 Bardwell (1,081 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1075 Helina (1,097 words) [view diff] exact match in snippet view article find links to article
J.; et al. (January 2018). "Spin states of asteroids in the Eos collisional family". Icarus. 299: 84–96. arXiv:1707.05507. Bibcode:2018Icar..299...84H555 Norma (1,157 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1154 Astronomia (993 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics2629 Rudra (1,079 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1364 Safara (999 words) [view diff] exact match in snippet view article find links to article
J.; et al. (January 2018). "Spin states of asteroids in the Eos collisional family". Icarus. 299: 84–96. arXiv:1707.05507. Bibcode:2018Icar..299...84H1109 Tata (1,187 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1717 Arlon (1,141 words) [view diff] exact match in snippet view article find links to article
provincial capital, Arlon. Arlon is a member of the Flora family, a collisional family of S-type asteroids asteroids, and one of the largest populations1576 Fabiola (1,077 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics7 Iris (1,185 words) [view diff] exact match in snippet view article find links to article
equatorial excavation, suggesting it is a remnant planetesimal. No collisional family can be associated with Iris, likely because the excavating impact251 Sophia (1,109 words) [view diff] exact match in snippet view article find links to article
J.; et al. (January 2018). "Spin states of asteroids in the Eos collisional family". Icarus. 299: 84–96. arXiv:1707.05507. Bibcode:2018Icar..299...84H468 Lina (1,277 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1388 Aphrodite (1,229 words) [view diff] exact match in snippet view article find links to article
J.; et al. (January 2018). "Spin states of asteroids in the Eos collisional family". Icarus. 299: 84–96. arXiv:1707.05507. Bibcode:2018Icar..299...84H461 Saskia (1,122 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids" (PDF). Astronomy and Astrophysics90482 Orcus (3,594 words) [view diff] exact match in snippet view article find links to article
of any Kuiper belt object that is not associated with the Haumea collisional family. The large icy satellites of Uranus have infrared spectra quite similar1353 Maartje (1,165 words) [view diff] exact match in snippet view article find links to article
J.; et al. (January 2018). "Spin states of asteroids in the Eos collisional family". Icarus. 299: 84–96. arXiv:1707.05507. Bibcode:2018Icar..299...84H1021 Flammario (1,471 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1484 Postrema (1,197 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics1148 Rarahu (1,357 words) [view diff] exact match in snippet view article find links to article
J.; et al. (January 2018). "Spin states of asteroids in the Eos collisional family". Icarus. 299: 84–96. arXiv:1707.05507. Bibcode:2018Icar..299...84H1724 Vladimir (1,179 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics4388 Jürgenstock (1,061 words) [view diff] exact match in snippet view article find links to article
Link. Jürgenstock is a member of the Phocaea family (701), a large collisional family of nearly 2000 stony asteroids, which is named after 25 Phocaea.: 2389 Julia (552 words) [view diff] exact match in snippet view article find links to article
body approximately 8 kilometers in diameter may have created the collisional family. Noah Webster (1884) A Practical Dictionary of the English Language1493 Sigrid (1,368 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids" (PDF). Astronomy and Astrophysics1076 Viola (1,222 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics5148 Giordano (1,009 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics9799 Thronium (1,034 words) [view diff] exact match in snippet view article find links to article
Jovian asteroids; four of them in the Greek camp. This potentially collisional family was first characterized by Jakub Rozehnal and Miroslav Brož in 20143000 Leonardo (1,545 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics5258 Rhoeo (1,000 words) [view diff] exact match in snippet view article find links to article
asteroids; with four of them in the Greek camp. This potentially collisional family was first characterized by Jakub Rozehnal and Miroslav Brož in 2011Controversy over the discovery of Haumea (2,680 words) [view diff] exact match in snippet view article find links to article
Barkume, Kristina M.; Ragozzine, Darin; Schaller, Emily L. (2007). "A collisional family of icy objects in the Kuiper belt" (PDF). Nature. 446 (7133): 294–2961362 Griqua (1,627 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics7517 Alisondoane (1,147 words) [view diff] exact match in snippet view article find links to article
; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and AstrophysicsDwarf planet (8,992 words) [view diff] exact match in snippet view article find links to article
to have albedos much greater than this are fragments in the Haumea collisional family and possibly 2005 QU182 (albedo between 0.2 and 0.5). Grundy, W. MKuiper belt (13,220 words) [view diff] exact match in snippet view article find links to article
priority scientific target due to its status as the parent body of a collisional family that includes several other TNOs, as well as Haumea's ring and two225088 Gonggong (6,145 words) [view diff] exact match in snippet view article find links to article
based on his assumption that it may be a member of the icy Haumea collisional family. The nickname also fit because, by that time, Brown's team had discoveredOrbital resonance (10,244 words) [view diff] exact match in snippet view article find links to article
M. E.; Barkume, K. M.; Ragozzine, D.; Schaller, E. L. (2007). "A collisional family of icy objects in the Kuiper belt" (PDF). Nature. 446 (7133): 294–296Jumping-Jupiter scenario (13,549 words) [view diff] exact match in snippet view article find links to article
magnitude produced by the Yarkovsky effect. The survival of the Hilda collisional family, a subset of the Hilda group thought to have formed during the LHBStreaming instability (7,642 words) [view diff] exact match in snippet view article find links to article
the low albedo asteroids that have not been identified as part of a collisional family are larger than 35 km. A change in the slope of the size distribution