GNU Free Documentation License . .

(433)

: ,
(433)
Eros-433.jpg
. 14 2001 NEAR Shoemaker
. .
Urania
13 1898
1898 DQ; 1956 PC
()
27 2011
JD 2455800.5
(e) 0,2225305
(a) 218,103
(1,4579305 . .)
(q) 169,569
(1,133496497 . .)
(Q) 266,638
(1,782364503 . .)
(P) 642,989 (1,76 )
24,359 /
(i) 10,82798 °
(Ω) 304,34617 °
(ω) 178,77322 °
(M) 31,52822 °
[1][2]
34,4×11,2×11,2
16,84
(6,69 ± 0,002)·1015
2,670 ± 0,03 /³
0,0059 /²
2- 0,0103 /
5,270
S
715m
11,16 m
0,25
227 (46 °C)

(433) (.-. ρως , S. 13 1898 . .

, , [3]. , , , 14 2000 NEAR Shoemaker, .

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. 1996 2 . , . , , , , . 8 , , 3 , 2 . 1,14 . 105 , [4].

Asteroide Eros survole par sonde Near.gif
Eros rotation Dec. 3-4 2000.gif

, , (1036) . , , , , K-T , [5].

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, , , , : ( ), . , . , . , , , .

, , , [?]. , +100 °C ,   150 °C. YORP-. - YORP- - . , 2400 /³, , (5 16 ).

, 5 

(433) , , 1 . , 40% 0,5 . , , , , - . , 9 . , 9 [6].

, , , , [6].

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. 12 

. , NEAR Shoemaker, «» . , , , 20 [?]. .

, . , 3% . 3% 20 . , , . 2900 ³ , , , , . .

, [7].

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, . , 31 2012 0,179 . . (26,7  ) , 70 [8][9], +8,5m[10]. 846 , , 2,3 . , , 81 ( 1975 , 2056 ), +7,0m[2]  , , , , (4) , (2) , (7) .

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13 1898 : , [11]. , (185) [12]. 1902 .

. -, 19001901 . 1910 (. Arthur Robert Hinks) [13]. 19301931 [14]. 1968 , .

-, , , NEAR Shoemaker, .

, NEAR Shoemaker , . , . , , , , .

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3 2000 , NEAR Shoemaker 20 . [15].

[] .

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  1. Jim Baer. Recent Asteroid Mass Determinations. Personal Website (2008). 9 2012. 11 2008.
  2. 1 2 NEODys (433) Eros Ephemerides for 2137. Department of Mathematics, University of Pisa, Italy. 9 2012. 27 2010.
  3. Schmadel, Lutz D. Dictionary of Minor Planet Names (en).  Fifth Revised and Enlarged Edition.  B., Heidelberg, N. Y.: Springer, 2003.  P. 50.  992 p.  ISBN 3-540-00238-3
  4. Michel, P.; Farinella, P.; Froeschlé, Ch. (1996-04-25). «The orbital evolution of the asteroid Eros and implications for collision with the Earth». Nature 380 (6576): 689691. DOI:10.1038/380689a0. Bibcode1996Natur.380..689M. 2011-02-12.
  5. , , 3000 ³, , , 5 ( ), 520 ³. (. Dividing the mass of 433 Eros by its density gives a volume of 3000 km³, while the estimated 5 km radius of the (assumed spherical) Chicxulub Crater impactor yields a volume of only about 520 km³.)
  6. 1 2 Thomas PC, Robinson MS (1970). «Seismic resurfacing by a single impact on the asteroid 433 Eros». Nature 436 (7049): 366369. DOI:10.1038/nature03855. PMID 16034412. Bibcode2005Natur.436..366T.
  7. David Whitehouse. Gold rush in space?  (.). BBC News Online. 31 2012. 22 2010.
  8. JPL Close-Approach Data: 433 Eros (1898 DQ) (2011-11-13 last obs (arc=48.3 years days)). 31 2012. 14 2011.
  9. NEODyS-2 Close Approaches for (433) Eros. Near Earth Objects  Dynamic Site. 31 2012. 14 2011.
  10. AstDys (433) Eros Ephemerides for 2012. Department of Mathematics, University of Pisa, Italy. 31 2012. 27 2010.
  11. Scholl, Hans; Schmadel, Lutz D. (2002). «Discovery Circumstances of the First Near-Earth Asteroid (433) Eros». Acta Historica Astronomiae 15: 210220. Bibcode2002AcHA...15..210S.
  12. Donald K. Yeomans. Asteroid 433 Eros: The Target Body of the NEAR Mission. Jet Propulsion Laboratory/California Institute of Technology.
  13. Hinks, Arthur R. (1909). «Solar Parallax Papers No. 7: The General Solution from the Photographic Right Ascensions of Eros, at the Opposition of 1900». Month. Not. Roy. Astron. Soc. 69 (7): 54467. Bibcode1909MNRAS..69..544H.
  14. Jones, H. Spencer (1941). «The Solar Parallax and the Mass of the Moon from Observations of Eros at the Opposition of 1931». Mem. Roy. Astron. Soc. 66: 1166.
  15. . .

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