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P a g e s f o r l o g g e d o u t e d i t o r s l e a r n m o r e ● C o n t r i b u t i o n s ● T a l k
( T o p )
1 N o t e s
2 R e f e r e n c e s
3 E x t e r n a l l i n k s
T o g g l e t h e t a b l e o f c o n t e n t s
1 7 1 O p h e l i a
4 0 l a n g u a g e s
● A s t u r i a n u ● 閩 南 語 / B â n - l â m - g ú ● Б е л а р у с к а я ● C a t a l à ● D e u t s c h ● Ε λ λ η ν ι κ ά ● E s p a ñ o l ● E s p e r a n t o ● E u s k a r a ● ف ا ر س ی ● F r a n ç a i s ● Հ ա յ ե ր ե ն ● I t a l i a n o ● L a t i n a ● L ë t z e b u e r g e s c h ● M a g y a r ● م ص ر ى ● 日 本 語 ● Н о х ч и й н ● N o r s k b o k m å l ● N o r s k n y n o r s k ● O c c i t a n ● P l a t t d ü ü t s c h ● P o l s k i ● P o r t u g u ê s ● R o m â n ă ● Р у с с к и й ● S l o v e n č i n a ● S l o v e n š č i n a ● С р п с к и / s r p s k i ● S r p s k o h r v a t s k i / с р п с к о х р в а т с к и ● S u o m i ● S v e n s k a ● T a g a l o g ● Т а т а р ч а / t a t a r ç a ● T ü r k ç e ● У к р а ї н с ь к а ● T i ế n g V i ệ t ● 粵 語 ● 中 文
E d i t l i n k s
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E n g l i s h
● R e a d ● E d i t ● V i e w h i s t o r y
T o o l s
T o o l s
A c t i o n s
● R e a d ● E d i t ● V i e w h i s t o r y
G e n e r a l
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P r i n t / e x p o r t
● D o w n l o a d a s P D F ● P r i n t a b l e v e r s i o n
I n o t h e r p r o j e c t s
● W i k i m e d i a C o m m o n s
A p p e a r a n c e
F r o m W i k i p e d i a , t h e f r e e e n c y c l o p e d i a
Ophelia (minor planet designation : 171 Ophelia ) is a large, dark Themistian asteroid [5] Alphonse Borrelly on 13 January 1877, and named after Ophelia in Shakespeare 's Hamlet [6]
This asteroid is a member of the Themis family of asteroids that share similar orbital elements .[7] carbonaceous chondrite meteorites .
A 1979 study of the Algol -like light curve produced by this asteroid concluded that it was possible to model the brightness variation by assuming a binary system with a circular orbit, a period of 13.146 hours, and an inclination of 15° to the line of sight from the Earth.[8] Photometric observations of this asteroid at the Leura Observatory in Leura , Australia during 2006 gave a rotation period of 6.6666 ± 0.0002 hours and a brightness variation of 0.50 ± 0.02 in magnitude . This is in agreement with previous studies.[9]
Ophelia is also the name of a moon of Uranus .
Notes
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^ Assuming a diameter of 105.01 ± 3.54 km.
References
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^ a b Yeomans, Donald K., "171 Ophelia" , JPL Small-Body Database Browser , NASA Jet Propulsion Laboratory , retrieved 6 May 2016 .
^ a b Fienga, A.; Avdellidou, C.; Hanuš, J. (February 2020). "Asteroid masses obtained with INPOP planetary ephemerides" . Monthly Notices of the Royal Astronomical Society . 492 (1 ). doi :10.1093/mnras/stz3407
^ Florczak, M.; et al. (February 1999). "A spectroscopic study of the THEMIS family" . Astronomy and Astrophysics Supplement . 134 (3 ): 463–471. Bibcode :1999A&AS..134..463F . doi :10.1051/aas:1999150
^ Schmadel, Lutz (2003). Dictionary of Minor Planet Names ISBN 9783540002383 . Retrieved 17 July 2019 .
^ Moore, Patrick ; Rees, Robin, eds. (2011), Patrick Moore's Data Book of Astronomy Cambridge University Press , p. 165, ISBN 9781139495226
^ Wijesinghe, M. P.; Tedesco, E. F. (December 1979), "A test of plausibility of eclipsing binary asteroids", Icarus , 40 3 ): 383–393, Bibcode :1979Icar...40..383W , doi :10.1016/0019-1035(79 )90031-9 .
^ Oey, Julian (December 2006), "Lightcurves analysis of 10 asteroids from Leura Observatory", The Minor Planet Bulletin , 33 4 ): 96–99, Bibcode :2006MPBu...33...96O .
External links
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R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=171_Ophelia&oldid=1217092416 " C a t e g o r i e s : ● M i n o r p l a n e t o b j e c t a r t i c l e s ( n u m b e r e d ) ● T h e m i s a s t e r o i d s ● D i s c o v e r i e s b y A l p h o n s e B o r r e l l y ● N a m e d m i n o r p l a n e t s ● C - t y p e a s t e r o i d s ( T h o l e n ) ● C - t y p e a s t e r o i d s ( S M A S S ) ● A s t r o n o m i c a l o b j e c t s d i s c o v e r e d i n 1 8 7 7 ● O p h e l i a ● C - t y p e m a i n - b e l t - a s t e r o i d s t u b s H i d d e n c a t e g o r i e s : ● U s e d m y d a t e s f r o m J u l y 2 0 1 8 ● A r t i c l e s w i t h J P L S B D B i d e n t i f i e r s ● A r t i c l e s w i t h M P C i d e n t i f i e r s ● A l l s t u b a r t i c l e s
● T h i s p a g e w a s l a s t e d i t e d o n 3 A p r i l 2 0 2 4 , a t 2 0 : 0 5 ( U T C ) . ● T e x t i s a v a i l a b l e u n d e r t h e C r e a t i v e C o m m o n s A t t r i b u t i o n - S h a r e A l i k e L i c e n s e 4 . 0 ;
a d d i t i o n a l t e r m s m a y a p p l y . B y u s i n g t h i s s i t e , y o u a g r e e t o t h e T e r m s o f U s e a n d P r i v a c y P o l i c y . W i k i p e d i a ® i s a r e g i s t e r e d t r a d e m a r k o f t h e W i k i m e d i a F o u n d a t i o n , I n c . , a n o n - p r o f i t o r g a n i z a t i o n . ● P r i v a c y p o l i c y ● A b o u t W i k i p e d i a ● D i s c l a i m e r s ● C o n t a c t W i k i p e d i a ● C o d e o f C o n d u c t ● D e v e l o p e r s ● S t a t i s t i c s ● C o o k i e s t a t e m e n t ● M o b i l e v i e w
