877685
Add to an observing list or journal →877685 (2010 VD72)
Where is it now
- Distance from Sun
- 0.89 AU
- True anomaly
- 269.32°
- Distance from Earth
- 0.871 AU
- As of
- 21 October 2026
Two-body Kepler propagation — accurate to ~0.1% for major planets over decades, less so for highly-perturbed bodies. Use JPL Horizons for high precision.
In the sky
- Right ascension
- 10h 02m 59s
- Declination
- -01° 21′ 32″
- Constellation
- Sextans
- Distance from Earth
- 0.87 AU
- Elongation from the Sun
- 56.39° — near the Sun — look low at dusk or dawn
Visible from both hemispheres.
From your location
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Two-body approximation, good to about a degree for the planets — enough to find the constellation and know whether it is up.
Orbital elements
- Semi-major axis
- 0.918 AU
- Eccentricity
- 0.1813
- Inclination
- 19.2°
- Orbital period
- 321.5 days
- Perihelion
- 0.752 AU
- Aphelion
- 1.085 AU
- Longitude of ascending node
- 224.05°
- Argument of periapsis
- 310.32°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 5.1 LD
- 0.0132 AU
- Tisserand (Jupiter)
- 6.446
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 82
- Data arc
- 14.97 years
- First observed
- 9 November 2010
- Last observed
- 28 October 2025
- Residual RMS
- 0.48 ″
- Solution · Otto Matic
- 14 March 2026
Physical properties
- Mean radius
- 0.06 km
Visual & observation
- Geometric albedo
- 0.29
- Absolute magnitude (H)
- 21.55
Discovery & classification
- Discovered by
- CSS
- Discovery date
- 9 November 2010
- Discovery site
- Catalina
Also known as 2010 VD72
Close approaches 51 on record
Top-down view of the ecliptic, Earth at the centre, for the 2032-11-06 15:51 UTC close approach of 877685. Catalogue miss distance 23.8 LD · 9.14 × 10⁶ km. The curve is the geocentric path from 2032-11-03 to 2032-11-09, with a mark at UTC midnights and an arrow for the direction of motion. The circle is the Moon’s mean orbit; the Moon is plotted at closest approach. A ray shows the Sun’s direction. The labelled distance is the full separation. The drawn radius is the part that lies in the ecliptic plane. At closest approach the object is north of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2031-06-14 00:14:00 | Venus | 0.1269 AU | 49.4 LD | 15.9 km/s |
| 2032-11-06 15:51:00 | Earth | 0.0611 AU | 23.8 LD | 10.1 km/s |
| 2047-11-07 13:18:00 | Earth | 0.0883 AU | 34.4 LD | 12 km/s |
| 2054-11-02 20:43:00 | Earth | 0.1692 AU | 65.8 LD | 10 km/s |
| 2057-11-25 14:10:00 | Venus | 0.1446 AU | 56.3 LD | 13.4 km/s |
| 2064-01-20 01:30:00 | Venus | 0.0861 AU | 33.5 LD | 13.7 km/s |
| 2069-11-07 13:55:00 | Earth | 0.0231 AU | 9.0 LD | 10.9 km/s |
| 2070-03-16 09:02:00 | Venus | 0.079 AU | 30.7 LD | 14.5 km/s |
| 2076-05-10 10:26:00 | Venus | 0.0821 AU | 31.9 LD | 14.6 km/s |
| 2076-11-02 10:24:00 | Earth | 0.1665 AU | 64.8 LD | 10 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- physical properties: JPL SBDB (lookup)
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB