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. (ACS). , . |
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1899 OF; 1943 XB |
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1 Ceres |
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| [2] | ||||
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: June 18, 2009 |
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381 028 000 |
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446 521 000 |
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| (a) |
413 767 000 |
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| (e) |
0,07934[2] |
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| (v) |
17,882 / |
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| (Mo) |
27,448° |
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| (i) | ||||
| (Ω) |
80,399°[2] |
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| (ω) |
2,825°[2] |
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487,3 ± 1.8 [4] |
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454,7 ± 1.6 [4] |
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| (m) |
9,43 ± 0,07·1020 [5] |
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| (ρ) |
2,077 /³ |
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| (g) | ||||
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3°[4] |
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| (α) |
19 24 |
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| (δ) |
59°[4] |
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0,090 ± 0,0033 (V-band geometric)[7] |
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| C |
G[8] |
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3,36 ± 0.02[7] |
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, |
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́[13] (1 Ceres) [14][15][16]. , 263 . 1 1801 [17]. ; 1802 [18], «» 24 2006 XXVI . .
950 (590 ), , -, (32 %) [19][20]. , , , - [7]. , , , [8]. , , [4], [21].
6,7 9,3 . , [9]. 27 2007 Dawn (20112012) (2015).
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[]
, 1772 [17]. , 1766 , , [22][17][23]. 1781 , , 2,8 . . ( )[23][22], 1800 24 , « »[22]. , , [17][23]. , , [23].
1 1801 [24], « », . «87- - », , « »[17]. , [25]. 24 ( 11 1801 ), [26][27]. 24 1801 : (Barnaba Oriani) [28]. , , « , , - »[17]. . «Monatliche Correspondenz» 1801 .
( - ), - . , . 24 [25]. ( , )[29]. . 31 1801 [25][26].
260 ( 1802 ) 2613 ( , 1811 )[30][31].
[]
(Ceres Ferdinandea), III[17][25][26]. «Ferdinandea» , . [32], (. Δήμητρα), [33]. (
)[34], , ; ①[25][35]. . , 1803 [36]. , ( ), [37].
[]
. « », , 419 (2,8 ..) [17]. ( 2 , 3 4 ), [17][25][38].
, , (. they resemble small stars so much as hardly to be distinguished from them, even by very good telescopes)[39]
[38].
) , .
) [42].
[43], 24 2006 , , «» , , , «, ». , «», , , [13]. .
11 2008 «»[44], , . - , , , 1 . . +1[45]. [45].
, , . , Space.com , «, , , , »[46], , « ( ) », « » , , - [47]. , [48]. , 2006 , , , , «», 2006 « », 2006 « » « ». (2011) , « , . [] [] , , , , , 1 , », , « - 1 »[49]. , [50][51], , , , «Dawn »[52].
[]
«»: ( 0,08) (10,6°) (17°) (7°) [2]. 2,76 . ., 2,54, 2,98 . . . 4,6 . 2,77 . . (413,9 ). ~ 263,8 [53]. 9 4 [54].
, , [55]. , , , . , (1272) [55]. , -, , [56].
( ) ( ). , . . (q) (Q) . , 2 10 . .
2011 , 8 , , , , , , [57], , [58].
| δe | δi | δθ | δω | δε | δχ | δα | ||
|---|---|---|---|---|---|---|---|---|
| 1:(8×106) | -0,000018 | +0,000044 | -0,000241 | +0,000484 | +0,071482 | +0,000488 | +3×10-7 | |
| 1:(41×104) | -0,000025 | +0,000227 | -0,027558 | +0,037903 | +1,446688 | +0,038375 | +3×10-6 | |
| 1:329390 | -0,000536 | +0,000011 | -0,106807 | +0,092360 | +1,887510 | +0,094189 | -4×10-7 | |
| 1:(3085×103) | +0,000069 | +0,000359 | -0,039992 | +0,064190 | +0,239440 | +0,064875 | +4×10-7 | |
| 1:(1047,35) | -0,6752 | -0,5772 | -52,184 | +55,909 | -56,053 | +56,802 | -2×10-4 | |
| 1:(3501,6) | -0,022 | -0,041 | -1,411 | +1,290 | -2,125 | +1,314 | -1×10-4 | |
| 1:22650 | +0,00025 | +0,000002 | -0,02712 | +0,02327 | -0,03735 | +0,02373 | +3×10-5 | |
| 1:19350 | +0,000013 | -0,000229 | -0,007816 | +0,007691 | -0,011239 | +0,007825 | -1×10-5 |
(Jacques Laskar) «Astronomy & Astrophysics»[60] , « , 0,2 % » « , 400 »[57][61]. .
[]
, , , . , ( 2006 2010 ). 1953 2051 , 1814 2081 , 767 2684[62].
[]
, [8]. Ÿ . [63]. , 2008 , , 9,4·1020 [5][63], (3.0 ± 0.2·1021 )[64], 6000 4 % . , , , , [4], 975×909 . , 2 [65], 3 [66], , , 10 [67], , , .
[]
, , . [4]. , 100 (2328 % ; 50 % )[68], , 200 , [69]. , 2002 [5][21]. , (, , , ), [5].
. 7- . , XX «». , . (9,07 ) ( 4°). (. ) «». , , . , 167 (106 °C), 240 (33 °C). . , , , . . , «» 1020 .
[]
Dawn (NASA), 27 2007 . 2011 «Dawn» , 2015 .
[] .
[]
- Schmadel Lutz Dictionary of minor planet names. fifth. Germany: Springer, 2003. P. 15. ISBN 3-540-00238-3
- 1 2 3 4 5 6 Yeomans, Donald K. 1 Ceres. JPL Small-Body Database Browser (July 5, 2007). 10 2009.The listed values were rounded at the magnitude of uncertainty (1-sigma).
- The MeanPlane (Invariable plane) of the Solar System passing through the barycenter (3 2009). 10 2009. (produced with Solex 10 written by Aldo Vitagliano; see also Invariable plane)
- 1 2 3 4 5 6 7 8 Thomas, P. C.; Parker, J. Wm.; McFadden, L. A.; et al. (2005). «Differentiation of the asteroid Ceres as revealed by its shape». Nature 437 (7056): 224226. DOI:10.1038/nature03938. PMID 16148926. 2007-12-09.
- 1 2 3 4 Carry, Benoit; et al. (November 2007). «Near-Infrared Mapping and Physical Properties of the Dwarf-Planet Ceres» (PDF). Astronomy & Astrophysics 478: 235244. DOI:10.1051/0004-6361:20078166.
- 1 2 Calculated based on the known parameters
- 1 2 3 Li, Jian-Yang; McFadden, Lucy A.; Parker, Joel Wm. (2006). «Icar.182.143.pdf Photometric analysis of 1 Ceres and surface mapping from HST observations» (PDF). Icarus 182: 143160. DOI:10.1016/j.icarus.2005.12.012. 2007-12-08.
- 1 2 3 Rivkin, A. S.; Volquardsen, E. L.; Clark, B. E. (2006). «The surface composition of Ceres:Discovery of carbonates and iron-rich clays» (PDF). Icarus 185: 563567. DOI:10.1016/j.icarus.2006.08.022. 2007-12-08.
- 1 2 Menzel, Donald H.; and Pasachoff, Jay M. A Field Guide to the Stars and Planets. 2nd. Boston, MA: Houghton Mifflin, 1983. P. 391. ISBN 0395348358
- APmag and AngSize generated with Horizons (Ephemeris: Observer Table: Quantities = 9,13,20,29)
- Ceres Angular Size @ Feb 2009 Opposition: 974 km diam. / (1.58319 AU * 149 597 870 km) * 206265 = 0.84"
- 1 2 Saint-Pé, O.; Combes, N.; Rigaut F. (1993). «Ceres surface properties by high-resolution imaging from Earth». Icarus 105: 271281. DOI:10.1006/icar.1993.1125.
- 1 2 (). megabook.ru. 13 2011.
- NASA Dawn at a Glance. NASA. 14 2011.
- Shiga, David Dawn captures first orbital image of asteroid Vesta. New Scientist. 7 2011.
- Space Telescope Science Institute Hubble 2008: Science year in review. NASA Goddard Space Flight Center, 2009. P. 66.
- 1 2 3 4 5 6 7 8 9 10 Hoskin, Michael Bodes' Law and the Discovery of Ceres. Observatorio Astronomico di Palermo "Giuseppe S. Vaiana" (26 1992). 5 2007.
- Coffey, Jerry The First Asteroid Discovered. universetoday.com. 2 2011.
- Pitjeva, E. V.; Precise determination of the motion of planets and some astronomical constants from modern observations, in Kurtz, D. W. (Ed.), Proceedings of IAU Colloquium No. 196: Transits of Venus: New Views of the Solar System and Galaxy, 2004
- Moomaw, Bruce Ceres As An Abode Of Life. spaceblooger.com (2 2007). 6 2007.
- 1 2 McCord, Thomas B. (2005). «Ceres: Evolution and current state». Journal of Geophysical Research 110 (E5). DOI:10.1029/2004JE002244. Bibcode: 2005JGRE..11005009M.
- 1 2 3 . «». 7 2011.
- 1 2 3 4 Hogg, Helen Sawyer (1948). «The Titius-Bode Law and the Discovery of Ceres». Journal of the Royal Astronomical Society of Canada 242: 241246. Bibcode: 1948JRASC..42..241S.
- Hoskin Michael The Cambridge Concise History of Astronomy. Cambridge University press, 1999. P. 160161. ISBN 0-521-57600-8
- 1 2 3 4 5 6 Forbes, Eric G. (1971). «Gauss and the Discovery of Ceres». Journal for the History of Astronomy 2: 195199. Bibcode: 1971JHA.....2..195F.
- 1 2 3 - 1 . " ". 10 2011.
- . solarsystem. 7 2011.
- Clifford J. Cunningham The first asteroid: Ceres, 18012001. Star Lab Press, 2001. ISBN 978-0-9708162-1-4
- . - . 10 2011.
- Hilton, James L Asteroid Masses and Densities (PDF). U.S. Naval Observatory. 23 2008.
- Hughes, D. W. (1994). «The Historical Unravelling of the Diameters of the First Four Asteroids». R.A.S. Quarterly Journal 35 (3). Bibcode: 1994QJRAS..35..331H.(Page 335)
- Foderà Serio, G.; Manara, A.; Sicoli, P. Giuseppe Piazzi and the Discovery of Ceres // Asteroids III / W. F. Bottke Jr., A. Cellino, P. Paolicchi, and R. P. Binzel. Tucson, Arizona: University of Arizona Press, 2002. P. 1724.
- All other languages but one use a variant of Ceres: Russian Tserera, Persian Seres, Japanese Keresu. The exception is Chinese, which uses 'grain-god(dess) star' (星 gǔshénxīng). Note that this is unlike the goddess Ceres, where Chinese does use the Latin name (刻斯 kèruìsī).
- Unicode value U+26B3
- Gould, B. A. (1852). «On the symbolic notation of the asteroids». Astronomical Journal 2 (34). DOI:10.1086/100212. Bibcode: 1852AJ......2...80G.
- Staff Cerium: historical information. Adaptive Optics. 27 2007.
- Amalgamator Features 2003: 200 Years Ago (30 2003). 7 2006. 21 2006.
- 1 2 3 Hilton, James L. When Did the Asteroids Become Minor Planets? (17 2001). 16 2006. ( )
- Herschel, William Observations on the two lately discovered celestial Bodies. (May 6, 1802).
- Battersby, Stephen Planet debate: Proposed new definitions. New Scientist (16 2006). 27 2007.
- Connor, Steve. Solar system to welcome three new planets, NZ Herald (16 2006). 27 2007.
- The IAU draft definition of "Planet" and "Plutons". IAU (16 2006). 27 2007.
- Staff Writers The IAU Draft Definition Of Planets And Plutons. SpaceDaily (16 2006). 27 2007.
- Plutoid chosen as name for Solar System objects like Pluto // International Astronomical Union (News Release - IAU0804). 11.06.2008.
- 1 2 . gazeta.ru (18.08.08 15:38). 15 2011.
- Geoff Gaherty, «How to Spot Giant Asteroid Vesta in Night Sky This Week», 03 August 2011 [1]
- Question and answers 2. IAU. 31 2008.
- MPEC 2006-R19: EDITORIAL NOTICE. Minor Planet Center (7 2006). «the numbering of "dwarf planets" does not preclude their having dual designations in possible separate catalogues of such bodies.» 31 2008.
- Lang Kenneth The Cambridge Guide to the Solar System. Cambridge University Press, 2011. P. 372, 442.
- de Pater & Lissauer, 2010. Planetary Sciences, 2nd ed. Cambridge University Press
- Mann, Nakamura, & Mukai, 2009. Small bodies in planetary systems. Lecture Notes in Physics 758. Springer-Verlag.
- NASA/JPL, Dawn Views Vesta, 2011 Aug 02
- http://dic.academic.ru/dic.nsf/es/92436/%D0%A6%D0%95%D0%A0%D0%95%D0%A0%D0%90 (),
- Williams, David R. (2004). «Asteroid Fact Sheet».
- 1 2 Cellino, A. et al.' Spectroscopic Properties of Asteroid Families // Asteroids III. University of Arizona Press, 2002. P. 633643 (Table on p. 636).
- Kelley, M. S.; Gaffey, M. J. (1996). «A Genetic Study of the Ceres (Williams #67) Asteroid Family». Bulletin of the American Astronomical Society 28. Bibcode: 1996BAAS...28R1097K.
- 1 2 . , 15 - . (15/07/2011). 16 2011.
- , , // " ". 25.07.2011. . №4 (4).
- . . . 14 1935.
- J. Laskar, M. Gastineau, J.-B. Delisle, A. Farrés and A. Fienga Strong chaos induced by close encounters with Ceres and Vesta (.) // Astronomy & Astrophysics. 14 July 2011. . A&A 532, L4 (2011). DOI:10.1051/0004-6361/201117504
- (18 11 12:23). 16 2011.
- Solex. 2009-03-03 numbers generated by Solex.
- 1 2 (2007) «A New Determination of the Mass of (1) Ceres». Earth, Moon, and Planets 100 (12): 117123. DOI:10.1007/s11038-006-9124-4. Bibcode: 2007EM&P..100..117K.
- Pitjeva, E. V. (2005). «High-Precision Ephemerides of PlanetsEPM and Determination of Some Astronomical Constants» (PDF). Solar System Research 39 (3). DOI:10.1007/s11208-005-0033-2. Bibcode: 2005SoSyR..39..176P. 2007-12-09.
- Carry, B.; Kaasalainen, M.; Dumas, C.; et al. (2007). «Asteroid 2 Pallas Physical Properties from Near-Infrared High-Angular Resolution Imagery» (PDF). ISO (ESO Planetary Group: Journal Club). 2011-09-04.
- Kaasalainen, M.; Torppa, J.; Piironen, J. (2002). «Models of Twenty Asteroids from Photometric Data» (PDF). Icarus 159 (2): 369395. DOI:10.1006/icar.2002.6907. Bibcode: 2002Icar..159..369K. 2009-06-25.
- (2002) «10 Hygiea: ISO Infrared Observations». Icarus 156 (1). DOI:10.1006/icar.2001.6775. Bibcode: 2002Icar..156..202B.
- 0.72-0.77 anhydrous rock by mass, per William B. McKinnon, 2008, «On The Possibility Of Large KBOs Being Injected Into The Outer Asteroid Belt». American Astronomical Society, DPS meeting #40, #38.03
- Carey, Bjorn. Largest Asteroid Might Contain More Fresh Water than Earth, SPACE.com (7 September 2005). 16 2006.
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