Where is it now
- Distance from Sun
- 0.657 AU
- True anomaly
- 130.21°
- Distance from Earth
- 1.363 AU
- As of
- 15 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
- 15h 07m 57s
- Declination
- -21° 03′ 16″
- Constellation
- Libra
- Distance from Earth
- 1.37 AU
- Elongation from the Sun
- 27.48° — near the Sun — look low at dusk or dawn
Favours the southern hemisphere; low or below the horizon from far north.
From your location
See how high it is right now, whether it is up after civil twilight, and when it rises and sets where you are.
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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
- 0.682 AU
- Eccentricity
- 0.6759
- Inclination
- 12.59°
- Orbital period
- 205.8 days
- Perihelion
- 0.221 AU
- Aphelion
- 1.143 AU
- Longitude of ascending node
- 306.51°
- Argument of periapsis
- 195.65°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 6.1 LD
- 0.0157 AU
- Tisserand (Jupiter)
- 8.149
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 123
- Data arc
- 13.1 years
- First observed
- 18 July 2010
- Last observed
- 22 August 2023
- Residual RMS
- 0.49 ″
- Solution · Otto Matic
- 23 August 2023
Physical properties
- Mean radius
- 0.07 km
Visual & observation
- Geometric albedo
- 0.138
- Absolute magnitude (H)
- 21.81
Discovery & classification
Close approaches 363 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-09-03 22:29 UTC close approach of 2010 PK9. Catalogue miss distance 53.9 LD · 2.07 × 10⁷ km. The curve is the geocentric path from 2027-08-31 to 2027-09-06, 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 |
|---|---|---|---|---|
| 2027-09-03 22:29:00 | Earth | 0.1384 AU | 53.9 LD | 17.6 km/s |
| 2027-10-27 08:34:00 | Merc | 0.0465 AU | 18.1 LD | 37.9 km/s |
| 2027-10-27 08:34:00 | Mercury | 0.0465 AU | 18.1 LD | 37.9 km/s |
| 2028-07-25 02:35:00 | Earth | 0.0461 AU | 17.9 LD | 18.1 km/s |
| 2029-07-06 02:17:00 | Merc | 0.0428 AU | 16.7 LD | 31.3 km/s |
| 2029-07-06 02:17:00 | Mercury | 0.0428 AU | 16.7 LD | 31.3 km/s |
| 2031-03-17 00:49:00 | Merc | 0.0796 AU | 31.0 LD | 28 km/s |
| 2031-03-17 00:49:00 | Mercury | 0.0796 AU | 31.0 LD | 28 km/s |
| 2031-08-28 10:32:00 | Earth | 0.3539 AU | 137.7 LD | 27.2 km/s |
| 2032-08-09 05:03:00 | Earth | 0.1366 AU | 53.1 LD | 14.3 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