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For accurate long-term ephemerides, please instead use our Horizons system.This orbit viewer was implemented using two-body methods, and hence should not be used for determining accurate long-term trajectories (over several years or decades) or planetary encounter circumstances.
Orbital Elements at Epoch 2459200.5 (2020-Dec-17.0) TDB
Reference: JPL 24 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .2430280602392932 | 3.4934e-08 | |
a | 2.386253881567407 | 9.0344e-09 | au |
q | 1.806327229491596 | 8.3192e-08 | au |
i | 3.964287789291169 | 3.6641e-06 | deg |
node | 210.1153399297175 | 5.9553e-05 | deg |
peri | 106.5693082343044 | 6.0221e-05 | deg |
M | 237.681890236268 | 7.3064e-06 | deg |
tp | 2459657.968988595906 (2022-Mar-19.46898860) | 2.791e-05 | TDB |
period | 1346.397816420127 3.69 | 7.6462e-06 2.093e-08 | d yr |
n | .267380112779139 | 1.5185e-09 | deg/d |
Q | 2.966180533643217 | 1.123e-08 | au |
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| | Orbit Determination Parameters
Additional Information
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[ hide covariance matrix ]
Orbital Elements at Epoch 2457141.5 (2015-Apr-29.0) TDB
Reference: JPL 24 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .2441034332825286 | 3.5007e-08 | |
q | 1.803280687207541 | 8.3459e-08 | au |
tp | 2456964.667240452928 (2014-Nov-03.16724045) | 2.7624e-05 | TDB |
node | 210.1740223911625 | 5.9629e-05 | deg |
peri | 106.4533639748158 | 6.0286e-05 | deg |
i | 3.961557069100428 | 3.6639e-06 | deg |
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| | Orbit Determination Parameters
Additional Information
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Orbit Covariance (6×6)
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|
e |
q |
tp |
node |
peri |
i |
e |
1.225503339127303E-15 |
-2.912011065402171E-15 |
1.605775214397633E-13 |
-9.87558822305118E-15 |
7.086363592592938E-14 |
-2.144297686404751E-15 |
q |
-2.912011065402171E-15 |
6.96533960866995E-15 |
-4.35595143778619E-13 |
2.465773739695801E-14 |
-1.846197382255575E-13 |
5.024700201198765E-15 |
tp |
1.605775214397633E-13 |
-4.35595143778619E-13 |
7.630842679897307E-10 |
-1.606828235748042E-11 |
2.606907660825089E-10 |
-3.566435023976834E-13 |
node |
-9.87558822305118E-15 |
2.465773739695801E-14 |
-1.606828235748042E-11 |
3.555609282081801E-9 |
-3.551588802662013E-9 |
-2.745329116911009E-11 |
peri |
7.086363592592938E-14 |
-1.846197382255575E-13 |
2.606907660825089E-10 |
-3.551588802662013E-9 |
3.634371534528541E-9 |
2.728962991605237E-11 |
i |
-2.144297686404751E-15 |
5.024700201198765E-15 |
-3.566435023976834E-13 |
-2.745329116911009E-11 |
2.728962991605237E-11 |
1.34240016730215E-11 |
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Physical Parameter Table
Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
absolute magnitude |
H |
15.65 |
|
n/a |
E2021B10 |
|
diameter |
diameter |
4.963 |
km |
0.032 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M) |
|
geometric albedo |
albedo |
0.041 |
|
0.004 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M) |
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|
35270 Molinari | Discovered 1996 Sept. 7 by V. Giuliani and P. Chiavenna at Sormano. |
Emilio Molinari (b. 1963), developed his astronomical career in Brera Observatory, Milan, beginning with the study of distant clusters of galaxies then shifting to technology group. He now serves as director of the Telescopio Nazionale Galileo and Rapid Eye Mount observatories. |
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
Reference: 20111210/MPCPages.arc | Last Updated: 2011-12-12 |
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