Skip Page Navigation
NASA JPL Caltech
NASA Logo - Jet Propulsion Laboratory + View the NASA Portal
+ Near-Earth Object (NEO) Program
Search JPL
JPL Home Earth Solar System Stars & Galaxies Technology
JPL Solar System Dynamics
BODIES ORBITS EPHEMERIDES TOOLS PHYSICAL DATA DISCOVERY FAQ SITE MAP
JPL Small-Body Database Browser
Search: [ help ]  
78125 Salimbeni (2002 NU6)
Classification: Main-belt Asteroid          SPK-ID: 2078125
Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances | Close-Approach Data ]

[ show orbit diagram ]
Orbital Elements at Epoch 2456800.5 (2014-May-23.0) TDB
Reference: JPL 4 (heliocentric ecliptic J2000)
 Element Value Uncertainty (1-sigma)   Units 
e .1627593057552821 1.1178e-07  
a 2.686938987830571 3.5148e-08 AU
q 2.249614663564467 2.904e-07 AU
i 16.08684005913337 1.6813e-05 deg
node 298.9392235253213 2.7764e-05 deg
peri 73.50067836473708 6.7136e-05 deg
M 196.1436116660867 5.3987e-05 deg
tp 2457532.727459939178
(2016-May-24.22745994)
0.00024235 JED
period 1608.737311119817
4.40
3.1566e-05
8.642e-08
d
yr
n .2237779888062705 4.3909e-09 deg/d
Q 3.124263312096675 4.0869e-08 AU
  Orbit Determination Parameters
   # obs. used (total)      311  
   data-arc span      8406 days (23.01 yr)  
   first obs. used      1991-01-13  
   last obs. used      2014-01-18  
   planetary ephem.      DE431  
   SB-pert. ephem.      SB431-BIG16  
   condition code      0  
   fit RMS      .57052  
   data source      ORB  
   producer      Otto Matic  
   solution date      2014-Feb-19 19:40:21  

Additional Information
 Earth MOID = 1.30528 AU 
 T_jup = 3.299 
[ 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 14.9 mag n/a MPO259813  

78125 Salimbeni           Discovered 2002 July 11 by the Campo Imperatore Near Earth Object Survey.
Sara Salimbeni (b. 1977) obtained her degree in physics at "La Sapienza" University of Rome in 2003, with a thesis on the cosmological evolution of the deep field galaxy luminosity function. As a Ph.D. student at the University of Rome at Tor Vergata, she is continuing her studies of galaxies and structures evolution.
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character)
Reference: 20050919/MPCPages.arcLast Updated: 2005-09-26

[ show close-approach data ]
Ephemeris | Orbit Diagram | Orbital Elements | Physical Parameters | Discovery Circumstances | Close-Approach Data ]
ABOUT SSD CREDITS/AWARDS PRIVACY/COPYRIGHT GLOSSARY LINKS
FirstGov 2014-Apr-23 11:03 UT
(server date/time)  
NASA Home Page
Site Manager:   Donald K. Yeomans
Webmaster  Alan B. Chamberlin