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

[ show orbit diagram ]
Orbital Elements at Epoch 2459396.5 (2021-Jul-01.0) TDB
Reference: JPL 40 (heliocentric ecliptic J2000)
 Element Value Uncertainty (1-sigma)   Units 
e .05863413019073369 2.8105e-08  
a 2.915764661732999 1.0941e-08 au
q 2.744801336951406 8.0996e-08 au
i 1.081829237009792 3.1496e-06 deg
node 218.1509029172443 0.00015928 deg
peri 100.2204292470153 0.00016173 deg
M 134.3242775804078 2.7619e-05 deg
tp 2458717.954238840095
(2019-Aug-22.45423884)
0.00014005 TDB
period 1818.557884082716
4.98
1.0236e-05
2.802e-08
d
yr
n .1979590548923246 1.1142e-09 deg/d
Q 3.086727986514592 1.1583e-08 au
  Orbit Determination Parameters
   # obs. used (total)      2638  
   data-arc span      17039 days (46.65 yr)  
   first obs. used      1974-07-19  
   last obs. used      2021-03-13  
   planetary ephem.      DE441  
   SB-pert. ephem.      SB441-N16  
   condition code      0  
   norm. resid. RMS      .5136  
   source      ORB  
   producer      Otto Matic  
   solution date      2021-Jul-08 17:55:00  

Additional Information
 Earth MOID = 1.73107 au 
 Jupiter MOID = 2.08509 au 
 T_jup = 3.279 
[ 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 13.53   n/a E2021B10  
rotation period rot_per 6.514 h n/a LCDB (Rev. 2020-October); 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

Alternate Designations
 1998 FK12 = 1974 OL1 = 1998 HV64 = 1999 NX35 
Ephemeris | Orbit Diagram | Orbital Elements | Mission Design | Physical Parameters | Discovery Circumstances ]
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