2012 HP13 is an asteroid in the Aten orbit class. Its orbit takes it from 0.81 AU to 1.16 AU from the Sun; one orbit takes 357.9 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 1.146 AU
- True anomaly
- 199.46°
- Distance from Earth
- 1.88 AU
- As of
- 2 November 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
- 13h 01m 32s
- Declination
- +05° 25′ 11″
- Constellation
- Virgo
- Distance from Earth
- 1.88 AU
- Elongation from the Sun
- 30.81° — near the Sun — look low at dusk or dawn
Visible from both hemispheres.
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
- 0.986 AU
- Eccentricity
- 0.1761
- Inclination
- 23.02°
- Orbital period
- 357.9 days
- Perihelion
- 0.813 AU
- Aphelion
- 1.16 AU
- Longitude of ascending node
- 37.07°
- Argument of periapsis
- 286.53°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.0 LD
- 0.0001 AU
- Tisserand (Jupiter)
- 6.064
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 199
- Data arc
- 744 days
- First observed
- 22 April 2012
- Last observed
- 6 May 2014
- Residual RMS
- 0.39 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 24.2
Discovery & classification
Close approaches 102 on record
Top-down view of the ecliptic, Earth at the centre, for the 2051-11-27 18:03 UTC close approach of 2012 HP13. Catalogue miss distance 155.4 LD · 5.97 × 10⁷ km. The curve is the geocentric path from 2051-11-24 to 2051-11-30, 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. 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 |
|---|---|---|---|---|
| 2051-11-27 18:03:00 | Earth | 0.3992 AU | 155.4 LD | 21.4 km/s |
| 2052-11-20 07:58:00 | Earth | 0.2795 AU | 108.8 LD | 18.4 km/s |
| 2053-11-13 11:20:00 | Earth | 0.1641 AU | 63.9 LD | 15.9 km/s |
| 2054-11-05 22:03:00 | Earth | 0.0794 AU | 30.9 LD | 13.9 km/s |
| 2055-10-28 04:27:00 | Earth | 0.1242 AU | 48.3 LD | 12.7 km/s |
| 2056-10-16 00:20:00 | Earth | 0.2301 AU | 89.5 LD | 12.5 km/s |
| 2057-04-21 06:28:00 | Earth | 0.4109 AU | 159.9 LD | 12.8 km/s |
| 2057-09-29 01:35:00 | Earth | 0.3388 AU | 131.8 LD | 12.8 km/s |
| 2058-04-30 08:07:00 | Earth | 0.2964 AU | 115.4 LD | 12 km/s |
| 2059-05-01 13:49:00 | Earth | 0.1771 AU | 68.9 LD | 11.7 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB