+ View the NASA Portal + Center for Near-Earth Object Studies JPL Small-Body Database Browser Search: [ help ]   14429 Coyne (1991 XC) Classification: Main-belt Asteroid          SPK-ID: 2014429 [ Ephemeris | Orbit Diagram | Orbital Elements | Mission Design | Physical Parameters | Discovery Circumstances ] [ show orbit diagram ] Orbital Elements at Epoch 2459200.5 (2020-Dec-17.0) TDB Reference: JPL 20 (heliocentric ecliptic J2000)  Element Value Uncertainty (1-sigma)   Units  e .2993547416987785 1.5643e-08   a 2.4433741222174 9.8319e-09 au q 1.71193849298753 3.7022e-08 au i 21.39278861590061 7.0197e-07 deg node .6431411186833593 2.0397e-06 deg peri 92.66863387140624 2.4781e-06 deg M 220.9890952073143 4.2104e-06 deg tp 2459739.178635185641 (2022-Jun-08.67863519) 1.9399e-05 TDB period 1395.0294687747 3.82 8.4202e-06 2.305e-08 d yr n .2580590647423383 1.5576e-09 deg/d Q 3.174809751447269 1.2775e-08 au   Orbit Determination Parameters    # obs. used (total)      1165      data-arc span      10056 days (27.53 yr)      first obs. used      1991-12-03      last obs. used      2019-06-15      planetary ephem.      DE441      SB-pert. ephem.      SB441-N16      condition code      0      norm. resid. RMS      .46353      source      ORB      producer      Otto Matic      solution date      2021-Apr-13 00:28:51   Additional Information  Earth MOID = .872249 au   Jupiter MOID = 2.38534 au   T_jup = 3.347  [ show covariance matrix ] [ Ephemeris | Orbit Diagram | Orbital Elements | Mission Design | Physical Parameters | Discovery Circumstances ] Physical Parameter Table Parameter Symbol Value Units Sigma Reference Notes absolute magnitude H 14.0   n/a MPO473962   diameter diameter 3.728 km 0.355 urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2012ApJ...759L...8M)   geometric albedo albedo 0.196   0.105 urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2015ApJ...814..117N)   14429 Coyne           Discovered 1991 Dec. 3 by C. S. Shoemaker and D. H. Levy at Palomar. George Coyne (b. 1933), S.J., has been an astronomer at the Vatican Observatory since 1969 and its director since 1978. He has helped with the completion of the large Vatican telescope on Mt. Graham, Arizona. His polarimetric studies have centered on cataclysmic variables, among other subjects. NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) Reference: 20001111/MPCPages.arc Last Updated: 2013-03-29 [ Ephemeris | Orbit Diagram | Orbital Elements | Mission Design | Physical Parameters | Discovery Circumstances ] 2021-Apr-16 18:30 UT (server date/time)   Site Manager:   Ryan S. Park Webmaster:   Alan B. Chamberlin