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17219 Gianninoto (2000 CV)
Classification: Main-belt Asteroid          SPK-ID: 2017219
Ephemeris | Orbit Diagram | Orbital Elements | Mission Design | Physical Parameters | Discovery Circumstances | Close-Approach Data ]

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Orbital Elements at Epoch 2459200.5 (2020-Dec-17.0) TDB
Reference: JPL 39 (heliocentric ecliptic J2000)
 Element Value Uncertainty (1-sigma)   Units 
e .1209714731197206 2.9748e-08  
a 2.693072948957316 1.2342e-08 au
q 2.367287947103079 8.415e-08 au
i 14.12569176561503 3.538e-06 deg
node 147.5270105909999 1.556e-05 deg
peri 338.4241693669464 2.347e-05 deg
M 275.9356121433497 1.8584e-05 deg
tp 2459577.446883762342
(2021-Dec-28.94688376)
8.4444e-05 TDB
period 1614.249286937594
4.42
1.1097e-05
3.038e-08
d
yr
n .2230138820026732 1.5331e-09 deg/d
Q 3.018857950811553 1.3835e-08 au
  Orbit Determination Parameters
   # obs. used (total)      2354  
   data-arc span      23687 days (64.85 yr)  
   first obs. used      1956-03-11  
   last obs. used      2021-01-16  
   planetary ephem.      DE431  
   SB-pert. ephem.      SB431-N16  
   condition code      0  
   norm. resid. RMS      .41133  
   source      ORB  
   producer      Otto Matic  
   solution date      2021-Feb-24 02:32:58  

Additional Information
 Earth MOID = 1.3867 au 
 Jupiter MOID = 2.03167 au 
 T_jup = 3.317 
[ show covariance matrix ]

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

Physical Parameter Table
Parameter Symbol Value Units Sigma Reference Notes
absolute magnitude H 13.02   n/a E2021B10  
diameter diameter 6.135 km 0.205 urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M)  
geometric albedo albedo 0.205   0.034 urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M)  

17219 Gianninoto           Discovered 2000 Feb. 1 by the Catalina Sky Survey.
Joe Gianninoto (b. 1947) is an avid amateur astronomer originally from New York, now living in Tucson, Arizona. He specializes in white light and H-alpha solar observing with the Association of Lunar and Planetary Observers.
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character)
Reference: MPC batch dated 2015-09-28Last Updated: 2015-10-05

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