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17779 Migomueller (1998 FK12)
Classification: Main-belt Asteroid          SPK-ID: 2017779
Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances | Close-Approach Data ]

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Orbital Elements at Epoch 2457400.5 (2016-Jan-13.0) TDB
Reference: JPL 17 (heliocentric ecliptic J2000)
 Element Value Uncertainty (1-sigma)   Units 
e .06156265046413871 4.4946e-08  
a 2.914341485535126 2.0472e-08 au
q 2.734926899327988 1.3097e-07 au
i 1.079636061563241 4.344e-06 deg
node 218.195860261512 0.00024306 deg
peri 100.3498873748918 0.00024614 deg
M 99.01003493256869 3.9021e-05 deg
tp 2456900.712030865706
(2014-Aug-31.21203087)
0.00019778 JED
period 1817.226597393728
4.98
1.9148e-05
5.242e-08
d
yr
n .1981040782235485 2.0874e-09 deg/d
Q 3.093756071742263 2.1732e-08 au
  Orbit Determination Parameters
   # obs. used (total)      1535  
   data-arc span      15127 days (41.42 yr)  
   first obs. used      1974-07-19  
   last obs. used      2015-12-18  
   planetary ephem.      DE431  
   SB-pert. ephem.      SB431-BIG16  
   condition code      0  
   fit RMS      .54855  
   data source      ORB  
   producer      Otto Matic  
   solution date      2016-Jan-04 13:37:49  

Additional Information
 Earth MOID = 1.71991 au 
 Jupiter MOID = 2.08229 au 
 T_jup = 3.279 
[ show covariance matrix ]

Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances | Close-Approach Data ]

Physical Parameter Table
Parameter Symbol Value Units Sigma Reference Notes
absolute magnitude H 13.5 mag n/a MPO358802  
rotation period rot_per 6.514 h n/a LCDB (Rev. 2015-December); Warner et al., 2009 Result based on less than full coverage, so that the period may be wrong by 30 percent or so.
Published Reference List:
[Waszczak, A.; Chang, C.-K.; Ofeck, E.O.; Laher, F.; et al. (2015) Astron. J. 150, A75.]

17779 Migomueller           Discovered 1998 Mar. 26 by the OCA-DLR Asteroid Survey at Caussols.
German physicist Michael ("Migo") Mueller (b. 1974) has advanced knowledge of the thermal properties of minor planets, including modeling the thermal behavior of an eclipsing binary. He determined the thermal inertia of a double minor planet from mid-infrared observations of mutual eclipses from the Spitzer Space Telescope.
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character)
Reference: 20070926/MPCPages.arcLast Updated: 2007-09-30

[ show close-approach data ]
Alternate Designations
 1998 FK12 = 1974 OL1 = 1998 HV64 = 1999 NX35 
Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances | Close-Approach Data ]
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