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1050 Meta

1050 Meta, provisional designation 1925 RC, is a stony Eunomia asteroid from the central regions of the asteroid belt, approximately 10 kilometers (6 miles) in diameter. It was discovered on 14 September 1925, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany.[1] The meaning of the asteroids's name is unknown.[2] The presumably S-type asteroid has a rotation period of 6.14 hours and possibly an elongated shape.[4]

1050 Meta
Modelled shape of Meta from its lightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date14 September 1925
Designations
(1050) Meta
Named after
unknown[2]
1925 RC · A908 SE
main-belt[1][3] · (middle)
Eunomia[4][5]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc108.68 yr (39,694 d)
Aphelion3.0904 AU
Perihelion2.1599 AU
2.6252 AU
Eccentricity0.1772
4.25 yr (1,554 d)
233.12°
0° 13m 54.12s / day
Inclination12.496°
342.33°
66.282°
Physical characteristics
Mean diameter
8.773±0.115 km[6]
9.196±0.079 km[7]
10.03±0.65 km[8]
10.53 km (calculated)[4]
6.14188±0.00001 h[9]
6.142±0.001 h[10]
0.21 (assumed)[4]
0.294±0.042[8]
0.3346±0.0284[7]
0.364±0.062[6]
S (assumed)[4]
12.00[7][8] · 12.2[3][4]
12.34±0.09[11]

Orbit and classification edit

Meta is a member of the Eunomia family (502),[4][5] a prominent family of stony S-type asteroid and the largest one in the intermediate main belt with more than 5,000 members.[12]: 23  It orbits the Sun in the central asteroid belt at a distance of 2.2–3.1 AU once every 4 years and 3 months (1,554 days; semi-major axis of 2.63 AU). Its orbit has an eccentricity of 0.18 and an inclination of 12° with respect to the ecliptic.[3]

The body's observation arc begins with its first observation as A908 SE at Heidelberg in October 1908, or 17 years prior to its official discovery observation.[1]

Naming edit

Any reference of this minor planet's name to a person or occurrence is unknown.[2]

Unknown meaning edit

Among the many thousands of named minor planets, Meta is one of 120 asteroids, for which no official naming citation has been published. All of these asteroids have low numbers between 164 Eva and 1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.[13]

Physical characteristics edit

According to the overall spectral type for members of the Eunomia family, Meta is an assumed S-type asteroid.[4]

Rotation period and poles edit

In October 2006, a rotational lightcurve of Meta was obtained from photometric observations by French amateur astronomer René Roy. Lightcurve analysis gave a well-defined rotation period of 6.142 hours with a brightness amplitude of 0.46 magnitude, indicating that the asteroid has an elongated shape (U=3).[10]

A modeled lightcurve using photometric data from the Lowell Photometric Database was published in 2016. It gave a concurring period of 6.14188 hours, as well as two spin axes at (60.0°, −42.0°) and (198.0°, −79.0°) in ecliptic coordinates (λ, β).[9]

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, Meta measures between 8.773 and 10.03 kilometers in diameter and its surface has an albedo between 0.294 and 0.364.[6][7][8]

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from 15 Eunomia, the namesake and parent body of the Eunomia family – and calculates a diameter of 10.53 kilometers based on an absolute magnitude of 12.2.[4]

References edit

  1. ^ a b c d "1050 Meta (1925 RC)". Minor Planet Center. Retrieved 21 March 2018.
  2. ^ a b c Schmadel, Lutz D. (2007). "(1050) Meta". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 90. doi:10.1007/978-3-540-29925-7_1051. ISBN 978-3-540-00238-3.
  3. ^ a b c d "JPL Small-Body Database Browser: 1050 Meta (1925 RC)" (2017-06-05 last obs.). Jet Propulsion Laboratory. Retrieved 21 March 2018.
  4. ^ a b c d e f g h i "LCDB Data for (1050) Meta". Asteroid Lightcurve Database (LCDB). Retrieved 21 March 2018.
  5. ^ a b "Asteroid 1050 Meta – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 24 October 2019.
  6. ^ 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.
  7. ^ 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.
  8. ^ 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)
  9. ^ a b Durech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016). "Asteroid models from the Lowell photometric database". Astronomy and Astrophysics. 587: 6. arXiv:1601.02909. Bibcode:2016A&A...587A..48D. doi:10.1051/0004-6361/201527573. Retrieved 21 March 2018.
  10. ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (1050) Meta". Geneva Observatory. Retrieved 21 March 2018.
  11. ^ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv:1506.00762. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 21 March 2018.
  12. ^ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131.
  13. ^ Schmadel, Lutz D. (2007). "Appendix 11 – Minor Planet Names with Unknown Meaning". Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision. Springer Berlin Heidelberg. pp. 927–929. ISBN 978-3-540-00238-3.

External links edit

  • Lightcurve Database Query (LCDB), at www.minorplanet.info
  • Dictionary of Minor Planet Names, Google books
  • Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
  • 1050 Meta at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 1050 Meta at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

1050, meta, provisional, designation, 1925, stony, eunomia, asteroid, from, central, regions, asteroid, belt, approximately, kilometers, miles, diameter, discovered, september, 1925, german, astronomer, karl, reinmuth, heidelberg, observatory, southwest, germa. 1050 Meta provisional designation 1925 RC is a stony Eunomia asteroid from the central regions of the asteroid belt approximately 10 kilometers 6 miles in diameter It was discovered on 14 September 1925 by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany 1 The meaning of the asteroids s name is unknown 2 The presumably S type asteroid has a rotation period of 6 14 hours and possibly an elongated shape 4 1050 MetaModelled shape of Meta from its lightcurveDiscovery 1 Discovered byK ReinmuthDiscovery siteHeidelberg Obs Discovery date14 September 1925DesignationsMPC designation 1050 MetaNamed afterunknown 2 Alternative designations1925 RC A908 SEMinor planet categorymain belt 1 3 middle Eunomia 4 5 Orbital characteristics 3 Epoch 23 March 2018 JD 2458200 5 Uncertainty parameter 0Observation arc108 68 yr 39 694 d Aphelion3 0904 AUPerihelion2 1599 AUSemi major axis2 6252 AUEccentricity0 1772Orbital period sidereal 4 25 yr 1 554 d Mean anomaly233 12 Mean motion0 13m 54 12s dayInclination12 496 Longitude of ascending node342 33 Argument of perihelion66 282 Physical characteristicsMean diameter8 773 0 115 km 6 9 196 0 079 km 7 10 03 0 65 km 8 10 53 km calculated 4 Synodic rotation period6 14188 0 00001 h 9 6 142 0 001 h 10 Geometric albedo0 21 assumed 4 0 294 0 042 8 0 3346 0 0284 7 0 364 0 062 6 Spectral typeS assumed 4 Absolute magnitude H 12 00 7 8 12 2 3 4 12 34 0 09 11 Contents 1 Orbit and classification 2 Naming 2 1 Unknown meaning 3 Physical characteristics 3 1 Rotation period and poles 3 2 Diameter and albedo 4 References 5 External linksOrbit and classification editMeta is a member of the Eunomia family 502 4 5 a prominent family of stony S type asteroid and the largest one in the intermediate main belt with more than 5 000 members 12 23 It orbits the Sun in the central asteroid belt at a distance of 2 2 3 1 AU once every 4 years and 3 months 1 554 days semi major axis of 2 63 AU Its orbit has an eccentricity of 0 18 and an inclination of 12 with respect to the ecliptic 3 The body s observation arc begins with its first observation as A908 SE at Heidelberg in October 1908 or 17 years prior to its official discovery observation 1 Naming editAny reference of this minor planet s name to a person or occurrence is unknown 2 Unknown meaning edit Among the many thousands of named minor planets Meta is one of 120 asteroids for which no official naming citation has been published All of these asteroids have low numbers between 164 Eva and 1514 Ricouxa and were discovered between 1876 and the 1930s predominantly by astronomers Auguste Charlois Johann Palisa Max Wolf and Karl Reinmuth 13 Physical characteristics editAccording to the overall spectral type for members of the Eunomia family Meta is an assumed S type asteroid 4 Rotation period and poles edit In October 2006 a rotational lightcurve of Meta was obtained from photometric observations by French amateur astronomer Rene Roy Lightcurve analysis gave a well defined rotation period of 6 142 hours with a brightness amplitude of 0 46 magnitude indicating that the asteroid has an elongated shape U 3 10 A modeled lightcurve using photometric data from the Lowell Photometric Database was published in 2016 It gave a concurring period of 6 14188 hours as well as two spin axes at 60 0 42 0 and 198 0 79 0 in ecliptic coordinates l b 9 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 Meta measures between 8 773 and 10 03 kilometers in diameter and its surface has an albedo between 0 294 and 0 364 6 7 8 The Collaborative Asteroid Lightcurve Link assumes an albedo of 0 21 derived from 15 Eunomia the namesake and parent body of the Eunomia family and calculates a diameter of 10 53 kilometers based on an absolute magnitude of 12 2 4 References edit a b c d 1050 Meta 1925 RC Minor Planet Center Retrieved 21 March 2018 a b c Schmadel Lutz D 2007 1050 Meta Dictionary of Minor Planet Names Springer Berlin Heidelberg p 90 doi 10 1007 978 3 540 29925 7 1051 ISBN 978 3 540 00238 3 a b c d JPL Small Body Database Browser 1050 Meta 1925 RC 2017 06 05 last obs Jet Propulsion Laboratory Retrieved 21 March 2018 a b c d e f g h i LCDB Data for 1050 Meta Asteroid Lightcurve Database LCDB Retrieved 21 March 2018 a b Asteroid 1050 Meta Nesvorny HCM Asteroid Families V3 0 Small Bodies Data Ferret Retrieved 24 October 2019 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 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 d Usui Fumihiko Kuroda Daisuke Muller 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 Durech J Hanus J Oszkiewicz D Vanco R March 2016 Asteroid models from the Lowell photometric database Astronomy and Astrophysics 587 6 arXiv 1601 02909 Bibcode 2016A amp A 587A 48D doi 10 1051 0004 6361 201527573 Retrieved 21 March 2018 a b Behrend Raoul Asteroids and comets rotation curves 1050 Meta Geneva Observatory Retrieved 21 March 2018 Veres Peter Jedicke Robert Fitzsimmons Alan Denneau Larry Granvik Mikael Bolin Bryce et al November 2015 Absolute magnitudes and slope parameters for 250 000 asteroids observed by Pan STARRS PS1 Preliminary results Icarus 261 34 47 arXiv 1506 00762 Bibcode 2015Icar 261 34V doi 10 1016 j icarus 2015 08 007 Retrieved 21 March 2018 Nesvorny D Broz M Carruba V December 2014 Identification and Dynamical Properties of Asteroid Families Asteroids IV pp 297 321 arXiv 1502 01628 Bibcode 2015aste book 297N doi 10 2458 azu uapress 9780816532131 ch016 ISBN 9780816532131 Schmadel Lutz D 2007 Appendix 11 Minor Planet Names with Unknown Meaning Dictionary of Minor Planet Names Fifth Revised and Enlarged revision Springer Berlin Heidelberg pp 927 929 ISBN 978 3 540 00238 3 External links editLightcurve Database Query LCDB at www minorplanet info Dictionary of Minor Planet Names Google books Asteroids and comets rotation curves CdR Geneva Observatory Raoul Behrend Discovery Circumstances Numbered Minor Planets 1 5000 Minor Planet Center 1050 Meta at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 1050 Meta at the JPL Small Body Database nbsp Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters Retrieved from https en wikipedia org w index php title 1050 Meta amp oldid 1195679907, wikipedia, wiki, book, books, library,

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