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( T o p )
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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
2020 PP1 is a sub-kilometer asteroid , classified as a near-Earth object of the Apollo group , that is a temporary quasi-satellite of the Earth . There are over a dozen known Earth quasi-satellites, some of which switch periodically between the quasi-satellite and horseshoe co-orbital states.[6]
Discovery
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2020 PP1 was discovered on 12 August 2020 by the Pan-STARRS 1 survey at the Haleakalā Observatory .[1] It was later recovered by the Karl Schwarzschild Observatory in August 2021, which allowed for precovery in earlier Pan-STARRS observations from 24 July 2017.[7]
Orbit and orbital evolution
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2020 PP1 is currently an Apollo asteroid (Earth-crossing but with a period longer than a year). Its semi-major axis (currently 1.001715 AU ) is similar to that of Earth (0.999789 AU ), but it has both low eccentricity (0.07384) and low orbital inclination (5.827°). It alternates between being an Aten asteroid and being an Apollo asteroid , although its orbital evolution is not fully stable and it can be considered as a temporary quasi-satellite of the Earth; its orbital evolution is akin to that of 469219 Kamoʻoalewa .[6]
Physical properties
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With an absolute magnitude of 26.6, it has a diameter in the range 10–30 meters (for an assumed albedo range of 0.20–0.04 respectively).[5]
See also
[ edit ]
54509 YORP
(419624) 2010 SO16
469219 Kamoʻoalewa
2015 SO2
2015 XX169
2015 YQ1
2015 YA
References
[ edit ]
^ a b "2020 PP1" . Minor Planet Center . International Astronomical Union. Retrieved 3 August 2021 .
^ "2020 PP1" . NEO Exchange . Las Cumbres Observatory . 13 August 2020. Retrieved 3 August 2021 .
^ a b c d "JPL Small-Body Database Browser: 2020 PP1" (2021-08-01 last obs.). Jet Propulsion Laboratory . Retrieved 3 August 2021 .
^ a b Bruton, Dan. "Conversion of Absolute Magnitude to Diameter for Minor Planets" . Department of Physics, Engineering, and Astronomy . Stephen F. Austin State University. Archived from the original on 23 July 2011. Retrieved 3 August 2021 .
^ a b de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (March 2021). "Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space" . Monthly Notices of the Royal Astronomical Society . 501 (4 ): 6007–6025. arXiv :2101.02563 . Bibcode :2021MNRAS.501.6007D . doi :10.1093/mnras/stab062 .
^ "MPEC 2021-P17 : 2020 PP1" . Minor Planet Electronic Circular . Minor Planet Center . 3 August 2021. Retrieved 3 August 2021 .
Further reading
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Understanding the Distribution of Near-Earth Asteroids Bottke, W. F., Jedicke, R., Morbidelli, A., Petit, J.-M., Gladman, B. 2000, Science , Vol. 288, Issue 5474, pp. 2190–2194.
A Numerical Survey of Transient Co-orbitals of the Terrestrial Planets Christou, A. A. 2000, Icarus , Vol. 144, Issue 1, pp. 1–20.
Debiased Orbital and Absolute Magnitude Distribution of the Near-Earth Objects Bottke, W. F., Morbidelli, A., Jedicke, R., Petit, J.-M., Levison, H. F., Michel, P., Metcalfe, T. S. 2002, Icarus , Vol. 156, Issue 2, pp. 399–433.
Transient co-orbital asteroids Brasser, R., Innanen, K. A., Connors, M., Veillet, C., Wiegert, P., Mikkola, S., Chodas, P. W. 2004, Icarus , Vol. 171, Issue 1, pp. 102–109.
A trio of horseshoes: past, present and future dynamical evolution of Earth co-orbital asteroids 2015 XX169 , 2015 YA and 2015 YQ1 de la Fuente Marcos, C., de la Fuente Marcos, R. 2016, Astrophysics and Space Science , Vol. 361, Issue 4, article 121 (13 pp).
External links
[ edit ]
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=2020_PP1&oldid=1187136828 "
C a t e g o r i e s :
● A p o l l o a s t e r o i d 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 ( u n n u m b e r e d )
● E a r t h - c r o s s i n g a s t e r o i d s
● E a r t h c o - o r b i t a l a s t e r o i d 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 2 0
● H o r s e s h o e o r b i t
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 A u g u s t 2 0 2 1
● J P L S m a l l - B o d y D a t a b a s e I D s a m e a s 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
● T h i s p a g e w a s l a s t e d i t e d o n 2 7 N o v e m b e r 2 0 2 3 , a t 1 8 : 1 6 ( 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