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767 Bondia (prov. designation :A913 SD or 1913 SX ) is a Themis asteroid from the outer regions of the asteroid belt , approximately 43 kilometers (27 miles) in diameter. It was discovered on 23 September 1913, by American astronomer Joel Hastings Metcalf at his observatory (799 [1] B-type asteroid has a rotation period of 8.3 hours. It was named after William Cranch Bond (1789–1859) and his son George Phillips Bond (1825–1865), both American astronomers and directors of the Harvard College Observatory in Cambridge, Massachusetts.[2]
Orbit and classification [ edit ]
Bondia is a core member the Themis family (602 family of carbonaceous asteroids, named after 24 Themis .[4] [5] [6] [12] : 24 outer main-belt at a distance of 2.6–3.7 AU semi-major axis of 3.12 AU ). Its orbit has an eccentricity of 0.18 and an inclination of 2° with respect to the ecliptic .[3]
The Themistian asteroid was first observed as A902 SA (1902 SA ) at Heidelberg Observatory on 26 September 1902. The body's observation arc begins at Bergedorf Observatory in September 1915, or two years after its official discovery observation by Metcalf at Winchester Observatory .[1]
This minor planet was named after American astronomers William Cranch Bond (1789–1859) and his son George Phillips Bond (1825–1865), both directors of the Harvard College Observatory in Cambridge, Massachusetts. Former co-discovered Comet 1850 II and pioneered the use of photographic plates in astronomy. The latter is best known for his 1848 co-discovery of Hyperion , a moon of Saturn . He also discovered Saturn's faint C Ring, also known as Crepe Ring . The naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 77 [2] W. Bond G. Bond [13] [14] Bond [15]
Physical characteristics [ edit ]
In the Bus–Binzel SMASS classification , Bondia is a B-type asteroid , a brighter variant of the common carbonaceous C-type asteroid .[3]
Rotation period [ edit ]
In October 2018, a rotational lightcurve of Bondia was obtained from photometric observations by Mexican astronomers at the National Astronomical Observatory in San Pedro Mártir (OAN-SPM). Lightcurve analysis gave a well defined rotation period of ± 0.0007± 0.02magnitude (U=3 Szabó from 2016, who determined a period of at least 60 U=2 [10] [11]
Diameter and albedo [ edit ]
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), Bondia measures ± 0.396± 0.66albedo between ± 0.022[7] [8] [9] Collaborative Asteroid Lightcurve Link derives an albedo of 0.0857 and a diameter of 41.40 kilometers based on an absolute magnitude of 10.2.[11] mean diameter measurements published by the WISE team include (± 0.730 km ± 4.5 km ± 15.23 km 47 ± 5 km ± 0.0179± 0.02± 0.02± 0.01[11] [16]
References [ edit ]
^ a b c Schmadel, Lutz D. (2007). "(767) Bondia". Dictionary of Minor Planet Names . Springer Berlin Heidelberg. p. 73. doi :10.1007/978-3-540-29925-7_768 . ISBN 978-3-540-00238-3
^ a b c d e f "JPL Small-Body Database Browser: 767 Bondia (A913 SD)" (2020-04-28 last obs.). Jet Propulsion Laboratory . Retrieved 28 May 2020 .
^ a b "Asteroid 767 Bondia – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved 28 May 2020 .
^ a b "Asteroid 767 Bondia – Nesvorny HCM Asteroid Families V3.0" . Small Bodies Data Ferret . Retrieved 28 May 2020 .
^ a b Zappalà, V.; Bendjoya, Ph.; Cellino, A.; Farinella, P.; Froeschle, C. (1997). "Asteroid Dynamical Families" . NASA Planetary Data System : EAR-A-5-DDR-FAMILY-V4.1. Retrieved 28 May 2020 . PDS main page )
^ a b c d Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016). "NEOWISE Diameters and Albedos V1.0" . NASA Planetary Data System . Bibcode :2016PDSS..247.....M . Retrieved 28 May 2020 .
^ a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal . 791 (2 ): 11. arXiv :1406.6645 Bibcode :2014ApJ...791..121M . doi :10.1088/0004-637X/791/2/121 .
^ a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey" . Publications of the Astronomical Society of Japan . 63 5 ): 1117–1138. Bibcode :2011PASJ...63.1117U . doi :10.1093/pasj/63.5.1117 online , AcuA catalog p. 153 )
^ a b Contreras, M. E.; Olguín, L.; Loera-González, P.; Saucedo, J. C.; Schuster, W. J.; Valdés-Sada, P.; et al. (October 2019). "Six Asteroids from the 2018 Mexican Asteroid Photometry Campaign" (PDF) . Minor Planet Bulletin . 46 4 ): 381–383. Bibcode :2019MPBu...46..381C . ISSN 1052-8091 . Archived from the original (PDF) on 8 June 2021. Retrieved 28 May 2020 .
^ a b c d "LCDB Data for (767) Bondia" . Asteroid Lightcurve Database (LCDB). Retrieved 28 May 2020 .
^ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV : 297–321. arXiv :1502.01628 Bibcode :2015aste.book..297N . doi :10.2458/azu_uapress_9780816532131-ch016 .
^ "Lunar crater G. Bond" . Gazetteer of Planetary Nomenclature . USGS Astrogeology Research Program.
^ "Lunar crater W. Bond" . Gazetteer of Planetary Nomenclature . USGS Astrogeology Research Program.
^ "Martian crater Bond" . Gazetteer of Planetary Nomenclature . USGS Astrogeology Research Program.
^ "Asteroid 767 Bondia" . Small Bodies Data Ferret . Retrieved 28 May 2020 .
External links [ edit ]
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=767_Bondia&oldid=1229659381 " 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 J o e l H a s t i n g s M e t c a l f ● N a m e d m i n o r p l a n e t s ● B - 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 9 1 3 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 O c t o b e r 2 0 1 9 ● 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 u n e 2 0 2 4 , a t 0 1 : 0 8 ( 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
