1294 Antwerpia
Dark background asteroid
1294 Antwerpia (prov. designation : 1933 UB1 ) is a dark background asteroid from the central regions of the asteroid belt . It was discovered on 24 October 1933, by astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle.[ 3] The carbonaceous C-type asteroid has a rotation period of 6.6 hours and measures approximately 35 kilometers (22 miles) in diameter. It was named for the Belgian city of Antwerp .[ 2]
Orbit and classification
Antwerpia is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements .[ 4] [ 5] It orbits the Sun in the central main belt at a distance of 2.1–3.3 AU once every 4 years and 5 months (1,608 days). Its orbit has an eccentricity of 0.23 and an inclination of 9° with respect to the ecliptic .[ 1] the asteroid was first observed as A917 DB at Heidelberg Observatory in February 2017, where the body's observation arc begins one month later in March 2017.[ 3]
Naming
This minor planet was named after the city of Antwerp in Flanders , the Dutch-speaking part of Belgium. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 118 ).[ 2]
Physical characteristics
In the SMASS classification , Antwerpia is a carbonaceous C-type asteroid .[ 1] It is also a C-type in both the Tholen- and SMASS-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2).[ 5] [ 13]
Rotation period and poles
Several rotational lightcurves of Antwerpia have been obtained from photometric observations since 2005. Lightcurve analysis gave a rotation period of 6.63 hours with a brightness variation of 0.42 magnitude (U=1/3/3-/3-/3/2 ).[ 15] [ 16] [ 17] [ 14] [ 18] [ 12] [ a]
A 2016-published lightcurve, using modeled photometric data from the Lowell Photometric Database (LPD), gave a concurring period of 6.62521 hours (U=n.a. ), as well as two spin axis of (128.0°, −66.0°) and (246.0°, −76.0°) in ecliptic coordinates (λ, β).[ 19]
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS , the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer , Antwerpia measures between 27.82 and 40.717 kilometers in diameter and its surface has an albedo between 0.0887 and 0.125.[ 6] [ 7] [ 8] [ 9] [ 10] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0783 and a diameter of 34.40 kilometers based on an absolute magnitude of 10.7.[ 11]
Notes
References
^ a b c d e f g "JPL Small-Body Database Browser: 1294 Antwerpia (1933 UB1)" (2016-11-02 last obs.). Jet Propulsion Laboratory . Archived from the original on 19 August 2020. Retrieved 14 September 2017 .
^ a b c Schmadel, Lutz D. (2007). "(1294) Antwerpia". Dictionary of Minor Planet Names . Springer Berlin Heidelberg . p. 106. doi :10.1007/978-3-540-29925-7_1295 . ISBN 978-3-540-00238-3 .
^ a b c "1294 Antwerpia (1933 UB1)" . Minor Planet Center . Retrieved 14 September 2017 .
^ a b "Asteroid 1294 Antwerpia – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved 16 March 2020 .
^ a b c d e "Asteroid 1294 Antwerpia" . Small Bodies Data Ferret . Retrieved 16 March 2020 .
^ a b c d Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos" . The Astrophysical Journal . 814 (2): 13. arXiv :1509.02522 . Bibcode :2015ApJ...814..117N . doi :10.1088/0004-637X/814/2/117 . Retrieved 14 September 2017 .
^ a b c d Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0" . NASA Planetary Data System . 12 : IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode :2004PDSS...12.....T . Retrieved 22 October 2019 .
^ 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 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 . Retrieved 14 September 2017 .
^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal . 741 (2): 25. arXiv :1109.6407 . Bibcode :2011ApJ...741...90M . doi :10.1088/0004-637X/741/2/90 .
^ a b c "LCDB Data for (1294) Antwerpia" . Asteroid Lightcurve Database (LCDB). Retrieved 14 September 2017 .
^ a b Lecrone, Crystal; Addleman, Don; Butler, Thomas; Hudson, Erin; Mulvihill, Alex; Reichert, Chris; et al. (September 2005). "2004-2005 winter observing campaign at Rose-Hulman Institute: results for 1098 Hakone, 1182 Ilona, 1294 Antwerpia, 1450 Raimonda, 2251 Tikhov, and 2365 Interkosmos" (PDF) . Minor Planet Bulletin . 32 (3): 46–48. Bibcode :2005MPBu...32...46L . ISSN 1052-8091 . Retrieved 16 March 2020 .
^ a b Lazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004). "S3OS2: the visible spectroscopic survey of 820 asteroids" (PDF) . Icarus . 172 (1): 179–220. Bibcode :2004Icar..172..179L . doi :10.1016/j.icarus.2004.06.006 . Retrieved 16 March 2020 .
^ a b Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry" . The Astronomical Journal . 150 (3): 35. arXiv :1504.04041 . Bibcode :2015AJ....150...75W . doi :10.1088/0004-6256/150/3/75 . Retrieved 14 September 2017 .
^ Almeida, R.; Angeli, C. A.; Duffard, R.; Lazzaro, D. (February 2004). "Rotation periods for small main-belt asteroids" . Astronomy and Astrophysics . 415 : 403–406. Bibcode :2004A&A...415..403A . doi :10.1051/0004-6361:20034585 .
^ Stephens, Robert D. (July 2014). "Asteroids Observed from CS3: 2014 January - March" (PDF) . Minor Planet Bulletin . 41 (3): 171–175. Bibcode :2014MPBu...41..171S . ISSN 1052-8091 . Retrieved 16 March 2020 .
^ Klinglesmith, Daniel A. III; Hanowell, Jesse; Risley, Ethan; Turk, Janek; Vargas, Angelica; Warren, Curtis Alan (July 2014). "Lightcurves for Inversion Model Candidates" (PDF) . Minor Planet Bulletin . 41 (3): 139–143. Bibcode :2014MPBu...41..139K . ISSN 1052-8091 . Retrieved 16 March 2020 .
^ Behrend, Raoul. "Asteroids and comets rotation curves – (1294) Antwerpia" . Geneva Observatory . Retrieved 14 September 2017 .
^ Ďurech, J.; Hanuš, J.; Oszkiewicz, D.; Vančo, R. (March 2016). "Asteroid models from the Lowell photometric database". Astronomy and Astrophysics . 587 : A48. arXiv :1601.02909 . Bibcode :2016A&A...587A..48D . doi :10.1051/0004-6361/201527573 . ISSN 0004-6361 .
External links