| 164215 Doloreshill (2004 MF6) |
| Classification: Amor [NEO] SPK-ID: 2164215 |
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| Orbit Diagram
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| Note:
Make sure you have Java enabled on your browser to see the applet.
This applet is provided as a 3D orbit visualization tool.
The applet was implemented using 2-body methods,
and hence should not be used for determining accurate long-term trajectories
(over several years or decades) or planetary encounter circumstances.
For accurate long-term ephemerides, please instead use our Horizons system. |
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Additional Notes: the orbits shown in the applet are color coded. The planets are white lines, and the asteroid/comet is a blue line. The bright white line indicates the portion of the orbit that is above the ecliptic plane, and the darker portion is below the ecliptic plane. Likewise for the asteroid/comet orbit, the light blue indicates the portion above the ecliptic plane, and the dark blue the portion below the ecliptic plane.
Orbit Viewer applet originally written and kindly provided by
Osamu Ajiki (AstroArts),
and further modified by
Ron Baalke (JPL).
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Orbital Elements at Epoch 2455200.5 (2010-Jan-04.0) TDB
Reference: JPL 35 (heliocentric ecliptic J2000)
| Element | Value | Uncertainty (1-sigma) | Units |
| e | .3969202750726624 | 1.9005e-07 | |
| a | 2.114730595281432 | 9.506e-08 | AU |
| q | 1.275351145697751 | 4.3856e-07 | AU |
| i | 4.879132707478044 | 7.6329e-06 | deg |
| node | 236.3012077863161 | 0.00019086 | deg |
| peri | 76.19656110486974 | 0.00023795 | deg |
| M | 275.9869526553928 | 6.1487e-05 | deg |
| tp | 2455462.635136066998 (2010-Sep-23.13513607) | 0.00020623 | JED |
| period | 1123.261826190342 3.08 | 7.5739e-05 2.074e-07 | d yr |
| n | .320495178956608 | 2.161e-08 | deg/d |
| Q | 2.954110044865113 | 1.3279e-07 | AU |
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| | Orbit Determination Parameters
Additional Information
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[ show covariance matrix ]
Physical Parameter Table
| Parameter |
Symbol |
Value |
Units |
Sigma |
Reference |
Notes |
| absolute magnitude |
H |
19.935 |
mag |
.49821 |
35 |
autocmod 2.4a |
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| 164215 Doloreshill | Discovered 2004 June 25 by the Catalina Sky Survey. |
| Dolores H. Hill (b. 1956) is a meteoriticist with the University of Arizona's Lunar and Planetary Laboratory, where she has, since 1981, classified meteorites using microprobe analysis, neutron activation methods and inductively coupled plasma mass spectrometry. |
| NOTE: some special characters may not display properly (any characters within {} are an attempt to place the proper accent above a character) |
| Reference: 20071124/MPCPages.arc | Last Updated: 2007-11-26 |
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