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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 41 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .1250543628289681 | 4.1895e-08 | |
a | 2.687334059782415 | 1.0998e-08 | au |
q | 2.351271211227741 | 1.1398e-07 | au |
i | 11.28689835515871 | 4.5913e-06 | deg |
node | 334.0404005035406 | 1.4345e-05 | deg |
peri | 200.2591348250272 | 1.8862e-05 | deg |
M | 206.211255946641 | 1.3939e-05 | deg |
tp | 2459887.889606236277 (2022-Nov-04.38960624) | 6.3727e-05 | TDB |
period | 1609.092133291629 4.41 | 9.8775e-06 2.704e-08 | d yr |
n | .2237286433459645 | 1.3734e-09 | deg/d |
Q | 3.023396908337089 | 1.2373e-08 | au |
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| | Orbit Determination Parameters
Additional Information
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Orbital Elements at Epoch 2457097.5 (2015-Mar-16.0) TDB
Reference: JPL 41 (heliocentric ecliptic J2000)
Element | Value | Uncertainty (1-sigma) | Units |
e | .1232853700402987 | 4.198e-08 | |
q | 2.357733603328203 | 1.1406e-07 | au |
tp | 2456666.819565559300 (2014-Jan-09.31956556) | 6.0202e-05 | TDB |
node | 334.1539258919584 | 1.4355e-05 | deg |
peri | 200.1472762021012 | 1.8954e-05 | deg |
i | 11.27853764292463 | 4.5887e-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 |
1.762285877194E-15 |
-4.77107341183206E-15 |
-7.52846023275007E-13 |
-1.369550304006745E-15 |
-1.451076355537377E-13 |
1.395334113828548E-15 |
q |
-4.77107341183206E-15 |
1.30098282089596E-14 |
2.049599069257839E-12 |
3.94664066139814E-15 |
3.993669844982277E-13 |
-3.639448874280613E-15 |
tp |
-7.52846023275007E-13 |
2.049599069257839E-12 |
3.624288892853983E-9 |
-1.819127733436907E-12 |
7.51012024374808E-10 |
6.021650491595226E-13 |
node |
-1.369550304006745E-15 |
3.94664066139814E-15 |
-1.819127733436907E-12 |
2.060784019165603E-10 |
-2.021221277234479E-10 |
1.01044610261833E-11 |
peri |
-1.451076355537377E-13 |
3.993669844982277E-13 |
7.51012024374808E-10 |
-2.021221277234479E-10 |
3.592597674906739E-10 |
-9.795366087157481E-12 |
i |
1.395334113828548E-15 |
-3.639448874280613E-15 |
6.021650491595226E-13 |
1.01044610261833E-11 |
-9.795366087157481E-12 |
2.105612142196042E-11 |
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Physical Parameter Table
Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
absolute magnitude |
H |
12.59 |
|
n/a |
E2021B10 |
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diameter |
diameter |
19.838 |
km |
0.134 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M) |
|
rotation period |
rot_per |
7.801 |
h |
n/a |
LCDB (Rev. 2020-October); Warner et al., 2009 |
Published Reference List: [Klinglesmith, D.A.; Jamieson, Q.; Pilcher, F. (2005) Minor Planet Bull. 32, 75-76.] |
geometric albedo |
albedo |
0.058 |
|
0.003 |
urn:nasa:pds:neowise_diameters_albedos::2.0[mainbelt] (http://adsabs.harvard.edu/abs/2011ApJ...741...68M) |
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|
3445 Pinson | Discovered 1983 Mar. 16 by E. Barr at the Anderson Mesa Station of the Lowell Observatory. |
William Hamet Pinson, Jr. (b. 1919), emeritus professor of geology at the Massachusetts Institute of Technology, is known in particular for his extensive studies of the rubidium-strontium ratio in lunar rocks and soil, tektites, meteorites and meteorite craters. The name was suggested by P. Topalian. |
NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
Reference: 20000523/MPCPages.arc | Last Updated: 2013-03-29 |
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Alternate Designations
1983 FC = 1952 DF = 1974 CK1 |
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