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8417 Lancetaylor (1996 VG8)
Classification: Main-belt Asteroid          SPK-ID: 2008417
Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances ]

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Orbital Elements at Epoch 2456400.5 (2013-Apr-18.0) TDB
Reference: MPO250293 (heliocentric ecliptic J2000)
 Element Value Uncertainty (1-sigma)   Units 
e 0.1936245 n/a  
a 2.2120746 n/a AU
q 1.7837628 n/a AU
i 5.80755 n/a deg
node 262.58093 n/a deg
peri 26.82798 n/a deg
M 95.70555 n/a deg
tp 2456081.0280735
(2012-Jun-02.52807350)
n/a JED
period 1201.7055807
3.29
n/a
n/a
d
yr
n 0.29957421 n/a deg/d
Q 2.6403864 n/a AU
  Orbit Determination Parameters
   # obs. used (total)      1029  
   first obs. used      1986-??-??  
   last obs. used      2013-01-22  
   # oppositions      14  
   planetary ephem.      DE403  
   condition code      0  
   fit RMS      0.53  
   data source      MPC:mpn  
   producer      MPCLINUX  

Additional Information
 T_jup = 3.625 

Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances ]

Physical Parameter Table
Parameter Symbol Value Units Sigma Reference Notes
absolute magnitude H 14.0 mag n/a PDS3 (MPC 31369)  
rotation period rot_per 6.538 h n/a Asteroid Lightcurve DataBase (Rev. 2013-May-01) Result based on less than full coverage, so that the period may be wrong by 30 percent or so.
Published Reference List:
[Clark, M.; Joyce, B. (2003) Minor Planet Bul. 30, 4-7.]

8417 Lancetaylor           Discovered 1996 Nov. 7 by K. Endate and K. Watanabe at Kitami.
Lance Taylor (b. 1956) is a science educator who teaches at high school and college in Western Australia. He is a leading member of Chiro Observatory, established and jointly operated by Australian and Japanese amateur astronomers.
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character)
Reference: 20000320/MPCPages.arcLast Updated: 2013-03-29

Alternate Designations
 1996 VG8 = 1986 TU5 
Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances ]
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