J u m p t o c o n t e n t
M a i n m e n u
M a i n m e n u
N a v i g a t i o n
● M a i n p a g e ● C o n t e n t s ● C u r r e n t e v e n t s ● R a n d o m a r t i c l e ● A b o u t W i k i p e d i a ● C o n t a c t u s ● D o n a t e
C o n t r i b u t e
● H e l p ● L e a r n t o e d i t ● C o m m u n i t y p o r t a l ● R e c e n t c h a n g e s ● U p l o a d f i l e
S e a r c h
Search
A p p e a r a n c e
● C r e a t e a c c o u n t ● L o g i n
P e r s o n a l t o o l s
● C r e a t e a c c o u n t ● L o g i n
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 O r b i t a n d r o t a t i o n
2 P h y s i c a l c h a r a c t e r i s t i c s
3 N o t e s
4 R e f e r e n c e s
5 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
( 4 5 5 5 0 2 ) 2 0 0 3 U Z 4 1 3
9 l a n g u a g e s
● D e u t s c h ● Ε λ λ η ν ι κ ά ● F r a n ç a i s ● G a e i l g e ● B a h a s a I n d o n e s i a ● M i n a n g k a b a u ● P o r t u g u ê s ● Р у с с к и й ● 中 文
E d i t l i n k s
● A r t i c l e ● T a l k
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
● W h a t l i n k s h e r e ● R e l a t e d c h a n g e s ● U p l o a d f i l e ● S p e c i a l p a g e s ● P e r m a n e n t l i n k ● P a g e i n f o r m a t i o n ● C i t e t h i s p a g e ● G e t s h o r t e n e d U R L ● D o w n l o a d Q R c o d e ● W i k i d a t a i t e m
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
2003 UZ413 has been observed 79 times over 15 oppositions , with precovery images back to 27 July 1954.[2]
Orbit and rotation [ edit ]
Precovery image of 2003 UZ413 taken by the Siding Spring Observatory in 1996.[11]
2003 UZ413 is in a 2:3 resonance with Neptune, which means that when it makes two revolutions around the Sun, Neptune makes exactly three.[3]
The object rotates very fast. In fact, with a period of about 4.13 hours, it is the fastest rotator known in the Kuiper belt after Haumea .[6] [8]
Physical characteristics [ edit ]
The mean diameter of 2003 UZ413 is estimated to be +1 km [5]
Given its rapid rotation, it must have a density higher than 0.72 g/cm3 .[6] Jacobi ellipsoids with an axis ratio of a/b ≥ ± 0.03Δm = ± 0.032.29−3.00 g/cm3 .[6] Johnston's Archive settles on 2.64 g/cm3 ,[7] km × 10 20 kg [12] dwarf planet , but confirmation would require additional observation to refine the size and light curve details, preferably with discovery of a satellite to determine its mass.
In visible light, this object is neutral or slightly red in color and has a flat, featureless reflectance spectrum.[8]
^ Buie page actually says 3:2 resonance... thus, also "Plutino"
^ very approximate figure, assuming equivalent spherical diameter of ≈600 km and density ≈2.64 g/cc3
^ equivalent to V-I=± 0.06± 0.06± 0.05
References [ edit ]
^ a b c d e
"JPL Small-Body Database Browser: (2003 UZ413)" (last observation: 2017-10-29). Retrieved 19 August 2019 .
^ a b c
Marsden, B. G. (2008-07-17). "Distant Minor Planets" . Minor Planet Electronic Circulars . Retrieved 3 December 2010 .
^
Marc W. Buie (2015-09-24). "Orbit Fit and Astrometric record for 2003 UZ413" . SwRI (Space Science Department). Archived from the original on 2015-09-23. Retrieved 2019-08-19 .
^ a b c d e f g h Farkas-Takács, A.; Kiss, Cs.; Vilenius, E.; Marton, G.; Müller, T. G.; Mommert, M.; et al. (28 February 2020). "Astronomy & Astrophysics . 638 : A23. arXiv :2002.12712 doi :10.1051/0004-6361/201936183 . S2CID 216193564 .
^ a b c d e
Perna, D.; Dotto, E.; Barucci, M. A.; Rossi, A.; Fornasier, S.; de Bergh, C. (2009). "Rotations and densities of trans-Neptunian objects" . Astronomy & Astrophysics . 508 (1 ): 451–455. Bibcode :2009A&A...508..451P . doi :10.1051/0004-6361/200911970 . Retrieved 1 June 2019 .
^ a b c
William Robert Johnston. "List of known trans-Neptunian objects" . Johnston's Archive. Retrieved 2019-08-19 .
^ a b c
Fornasier, S.; Barucci, M. A.; de Bergh, C.; Alvarez-Candal, A.; Demeo, F.; Merlin, F.; Perna, D.; Guilbert, A.; Delsanti, A.; Dotto, E.; Doressoundiram, A. (2009). "Visible spectroscopy of the new ESO large programme on trans-Neptunian objects and centaurs: Final results" (PDF) . Astronomy and Astrophysics 508 (1 ): 457–465. arXiv :0910.0450 Bibcode :2009A&A...508..457F . doi :10.1051/0004-6361/200912582
^ a b
Perna, D.; Barucci, M.A.; Fornasier, S.; et al. (2010). "Colors and taxonomy of centaurs and trans-Neptunian objects" . Astronomy and Astrophysics 510 : A53. arXiv :0912.2621 Bibcode :2010A&A...510A..53P . doi :10.1051/0004-6361/200913654
^ "2003 UZ413 Ephemerides" . Asteroids Dynamic Site. Archived from the original on 2019-08-19. Retrieved 2019-08-19 .
^ a b
"(455502) 2003 UZ413 Precovery Images" . Andrew Lowe's Minor Planet . Retrieved 28 April 2019 .
^ Grundy, W.M.; Noll, K.S.; Buie, M.W.; Benecchi, S.D.; Ragozzine, D.; Roe, H.G. (December 2019). "The Mutual Orbit, Mass, and Density of Transneptunian Binary Gǃkúnǁʼhòmdímà ((229762) 2007 UK126 )" . Icarus . 334 : 30–38. Bibcode :2019Icar..334...30G . doi :10.1016/j.icarus.2018.12.037 . S2CID 126574999 . Archived from the original on 2019-04-07. Retrieved 2019-11-06 .
External links [ edit ]
t
e
Consensus
Possible
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=(455502)_2003_UZ413&oldid=1196890405 " 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 ) ● P l u t i n o s ● D i s c o v e r i e s b y t h e P a l o m a r O b s e r v a t o r y ● P o s s i b l e d w a r f p l a n e t 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 2 0 0 3 H i d d e n c a t e g o r i e s : ● C S 1 : l o n g v o l u m e v a l u e ● J P L S m a l l - B o d y D a t a b a s e I D d i f f e r e n t f r o m W i k i d a t a ● 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
● T h i s p a g e w a s l a s t e d i t e d o n 1 8 J a n u a r y 2 0 2 4 , a t 2 0 : 1 2 ( 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
