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 p r o p e r t i e s
3 S e e a l s o
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
( 1 4 4 8 9 7 ) 2 0 0 4 U X 10
1 0 l a n g u a g e s
● ا ل ع ر ب ي ة ● D e u t s c h ● Ε λ λ η ν ι κ ά ● E s p e r a n t o ● F r a n ç a i s ● 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
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
(144897) 2004 UX10 provisional designation 2004 UX10 Kuiper-belt object . It has a diameter of about 360 kilometres (220 mi )[5] Apache Point Observatory in Sunspot , New Mexico.[2] cubewano .[3] [4] Neptune .[5] [7]
It is estimated by astronomer Michael E. Brown to likely be a dwarf planet based on its presumed size, calculated from its absolute magnitude (H ) and assumed albedo .[10]
Orbit and rotation [ edit ]
Based on an integration of its motion over 10 million years, (144897) 2004 UX10 has been classified as a classical Kuiper belt object (cubewano).[3] [5] Sun .[9]
The rotational period of (144897) 2004 UX10 is 7.58 hours.[8]
Physical properties [ edit ]
The size of (144897) 2004 UX10 was measured by the Herschel Space Telescope to be +124 km [5] × 10 19 [7]
(144897) 2004 UX10 has a moderately red slope in the visible spectral range. Its visible spectrum does not show any features, although there is a small departure from the linearity near 0.8 μm.[11]
See also [ edit ]
References [ edit ]
^ a b c d "144897 (2004 UX10)" . JPL Small-Body Database Browser (2018-10-31 last obs). 13 July 2019. Retrieved 3 November 2019 .
^ a b c Buie, M. (3 November 2019). "Orbit Fit and Astrometric record for 144897" . SwRI (Space Science Department). Archived from the original on 3 November 2019. Retrieved 3 November 2019 .
^ a b Johnston, W. R. (13 July 2019). "List of Known Trans-Neptunian Objects" . Retrieved 3 November 2019 .
^ a b c d e f g h i Mommert, Michael; Harris, A. W.; Kiss, C.; Pál, A.; Santos-Sanz, P.; Stansberry, J.; Delsanti, A.; Vilenius, E.; Müller, T. G.; Peixinho, N.; Lellouch, E.; Szalai, N.; Henry, F.; Duffard, R.; Fornasier, S.; Hartogh, P.; Mueller, M.; Ortiz, J. L.; Protopapa, S.; Rengel, M.; Thirouin, A. (May 2012). "TNOs are cool: A survey of the trans-Neptunian region—V. Physical characterization of 18 Plutinos using Herschel -PACS observations". Astronomy & Astrophysics 541 : A93. arXiv :1202.3657 Bibcode :2012A&A...541A..93M . doi :10.1051/0004-6361/201118562 . S2CID 119253817 .
^ a b "LCDB Data for (144897)" . Asteroid Lightcurve Database (LCDB). Retrieved 6 September 2016 .
^ a b c Thirouin, A.; Ortiz, J. L.; Duffard, R.; Santos-Sanz, P.; Aceituno, F. J.; Morales, N. (2010). "Short-term variability of a sample of 29 trans-Neptunian objects and Centaurs". Astronomy & Astrophysics . 522 : A93. arXiv :1004.4841 Bibcode :2010A&A...522A..93T . doi :10.1051/0004-6361/200912340 . S2CID 54039561 .
^ a b Perna, D.; Dotto, E.; Barucci, M. A.; Rossi, A.; Fornasier, S.; de Bergh, C. (December 2009). "Rotations and densities of trans-Neptunian objects". Astronomy & Astrophysics 508 : 451–455. Bibcode :2009A&A...508..451P . doi :10.1051/0004-6361/200911970 .
^ a b "AstDys (144897) 2004UX10 Ephemerides" . Department of Mathematics, University of Pisa, Italy. Retrieved 2012-01-21 .
^ Michael E. Brown . "How many dwarf planets are there in the outer solar system? (updates daily)" . California Institute of Technology . Archived from the original on 2011-10-18. Retrieved 2011-08-25 .
^ 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". Astronomy and Astrophysics 508 (1 ): 457–465. arXiv :0910.0450 Bibcode :2009A&A...508..457F . doi :10.1051/0004-6361/200912582 . S2CID 8479334 .
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=(144897)_2004_UX10&oldid=1210127665 " 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 A n d r e w C . B e c k e r ● D i s c o v e r i e s b y A n d r e w W . P u c k e t t ● D i s c o v e r i e s b y J e r e m y M a r t i n K u b i c a ● 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 4 H i d d e n c a t e g o r i e s : ● A r t i c l e s w i t h s h o r t d e s c r i p t i o n ● S h o r t d e s c r i p t i o n i s d i f f e r e n t f r o m W i k i d a t a ● 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 2 5 F e b r u a r y 2 0 2 4 , a t 0 3 : 1 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
