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词条 (50719) 2000 EG140
释义

  1. Classification and orbit

  2. Physical characteristics

      Slow rotator    Diameter and albedo  

  3. Numbering and naming

  4. References

  5. External links

{{DISPLAYTITLE:{{mp|(50719) 2000 EG|140}}}}{{Infobox planet
| minorplanet = yes
| name = {{mp|(50719) 2000 EG|140}}
| background = #D6D6D6
| image =
| image_size =
| caption =
| discovery_ref =  
| discoverer = CSS
| discovery_site = Mount Lemmon Obs.
| discovered = 1 March 2000
| mpc_name = (50719) {{mp|2000 EG|140}}
| alt_names = {{mp|2000 EG|140}}{{·}}{{mp|2001 MV|3}}
| pronounced =
| named_after =
| mp_category = main-belt{{·}}Eunomia [2]
Maria
| orbit_ref =  
| epoch = 4 September 2017 (JD 2458000.5)
| uncertainty = 0
| observation_arc = 18.44 yr (6,735 days)
| aphelion = 2.9328 AU
| perihelion = 2.2361 AU
| semimajor = 2.5844 AU
| eccentricity = 0.1348
| period = 4.15 yr (1,518 days)
| mean_anomaly = 290.94°
| mean_motion = {{Deg2DMS|0.2372|sup=ms}} / day
| inclination = 14.297°
| asc_node = 262.85°
| arg_peri = 30.119°
| dimensions = 3.307 km[4][5]
3.40 km {{small|(calculated)}}[2]
| rotation = {{nowrap|{{val|1256.0159|63.4351}} h[7]}}
| albedo = 0.21 {{small|(assumed)}}[2]
{{val|0.370|0.065}}[4][5]
| spectral_type = S [2]
| abs_magnitude = 14.1[4]{{·}}14.2{{·}}{{val|14.204|0.004}} {{small|(R)}}[7]{{·}}{{val|14.40|0.18}}[15]{{·}}14.65[2]
}}{{mp|(50719) 2000 EG|140}} is a stony Eunomian asteroid and exceptionally slow rotator from the middle region of the asteroid belt, approximately 3.3 kilometers in diameter. It was discovered on 1 March 2000, by astronomers of the U.S. Catalina Sky Survey, at Mount Lemmon Observatory, Arizona.[17]

Classification and orbit

The stony S-type asteroid is a member of the Eunomia family, the most prominent family in the intermediate main-belt. It orbits the Sun at a distance of 2.2–2.9 AU once every 4 years and 2 months (1,518 days). Its orbit has an eccentricity of 0.13 and an inclination of 14° with respect to the ecliptic. A first precovery was taken at Lowell Observatory (LONEOS) in 1998, extending the asteroid's observation arc by 2 years prior to its discovery.[17]

Physical characteristics

Slow rotator

In August 2010, a rotational lightcurve was obtained for this asteroid from photometric observations at the U.S. Palomar Transient Factory (PTF) in California. It gave a rotation period of 1256 hours with a brightness variation of 0.42 magnitude ({{small|U=2}}).[7] This makes the asteroid the 5th slowest rotating minor planet known to exist.

Diameter and albedo

According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 3.3 kilometers in diameter and its surface has an albedo of 0.37,[4][5] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.21 and calculates a diameter of 3.4 kilometers with an absolute magnitude of 14.65.[2]

Numbering and naming

This minor planet was numbered by the Minor Planet Center on 20 November 2002.[24] As of 2018, it has not been named.[17]

References

1. ^{{cite web |title = 50719 (2000 EG140) |work = Minor Planet Center |url = https://www.minorplanetcenter.net/db_search/show_object?object_id=50719 |accessdate = 3 September 2016}}
2. ^{{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 24 February 2018}}
3. ^{{cite web |title = LCDB Data for (50719) |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=50719%7C |accessdate = 3 September 2016}}
4. ^{{cite journal |display-authors = 6 |first1 = A. |last1 = Mainzer |first2 = T. |last2 = Grav |first3 = J. |last3 = Masiero |first4 = E. |last4 = Hand |first5 = J. |last5 = Bauer |first6 = D. |last6 = Tholen |first7 = R. S. |last7 = McMillan |first8 = T. |last8 = Spahr |first9 = R. M. |last9 = Cutri |first10 = E. |last10 = Wright |first11 = J. |last11 = Watkins |first12 = W. |last12 = Mo |first13 = C. |last13 = Maleszewski |date = November 2011 |title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results |url = https://arxiv.org/pdf/1109.6407v1.pdf |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 25 |bibcode = 2011ApJ...741...90M |doi = 10.1088/0004-637X/741/2/90 |arxiv = 1109.6407 |access-date= 3 September 2016}}
5. ^{{cite journal |display-authors = 6 |first1 = Adam |last1 = Waszczak |first2 = Chan-Kao |last2 = Chang |first3 = Eran O. |last3 = Ofek |first4 = Russ |last4 = Laher |first5 = Frank |last5 = Masci |first6 = David |last6 = Levitan |first7 = Jason |last7 = Surace |first8 = Yu-Chi |last8 = Cheng |first9 = Wing-Huen |last9 = Ip |first10 = Daisuke |last10 = Kinoshita |first11 = George |last11 = Helou |first12 = Thomas A. |last12 = Prince |first13 = Shrinivas |last13 = Kulkarni |date = September 2015 |title = Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W |journal = The Astronomical Journal |volume = 150 |issue = 3 |page = 35 |bibcode = 2015AJ....150...75W |doi = 10.1088/0004-6256/150/3/75 |arxiv = 1504.04041 |access-date= 3 September 2016}}
6. ^{{cite journal |display-authors = 6 |first1 = Peter |last1 = Veres |first2 = Robert |last2 = Jedicke |first3 = Alan |last3 = Fitzsimmons |first4 = Larry |last4 = Denneau |first5 = Mikael |last5 = Granvik |first6 = Bryce |last6 = Bolin |first7 = Serge |last7 = Chastel |first8 = Richard J. |last8 = Wainscoat |first9 = William S. |last9 = Burgett |first10 = Kenneth C. |last10 = Chambers |first11 = Heather |last11 = Flewelling |first12 = Nick |last12 = Kaiser |first13 = Eugen A. |last13 = Magnier |first14 = Jeff S. |last14 = Morgan |first15 = Paul A. |last15 = Price |first16 = John L. |last16 = Tonry |first17 = Christopher |last17 = Waters |date = November 2015 |title = Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V |journal = Icarus |volume = 261 |pages = 34–47 |bibcode = 2015Icar..261...34V |doi = 10.1016/j.icarus.2015.08.007 |arxiv = 1506.00762 |access-date= 3 September 2016}}
7. ^{{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = A. K. |last2 = Mainzer |first3 = T. |last3 = Grav |first4 = J. M. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = J. |last6 = Dailey |first7 = P. R. M. |last7 = Eisenhardt |first8 = R. S. |last8 = McMillan |first9 = T. B. |last9 = Spahr |first10 = M. F. |last10 = Skrutskie |first11 = D. |last11 = Tholen |first12 = R. G. |last12 = Walker |first13 = E. L. |last13 = Wright |first14 = E. |last14 = DeBaun |first15 = D. |last15 = Elsbury |first16 = T., IV |last16 = Gautier |first17 = S. |last17 = Gomillion |first18 = A. |last18 = Wilkins |date = November 2011 |title = Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 20 |bibcode = 2011ApJ...741...68M |doi = 10.1088/0004-637X/741/2/68 |arxiv = 1109.4096 |access-date= 14 December 2016}}
[1][2][3][4][5][6][7]

}}

External links

  • Asteroid Lightcurve Database (LCDB), query form (info)
  • [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
  • Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (50001)-(55000) – Minor Planet Center
  • {{JPL small body}}
{{Minor planets navigator |number=50719 |PageName={{mp|(50719) 2000 EG|140}} }}{{Small Solar System bodies}}{{DEFAULTSORT:050719}}

5 : Maria asteroids|Eunomia asteroids|Discoveries by CSS|Slow rotating minor planets|Astronomical objects discovered in 2000

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