Where is it now
- Distance from Sun
- 0.695 AU
- True anomaly
- 55.77°
- Distance from Earth
- 1.62 AU
- As of
- 19 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
- 14h 29m 22s
- Declination
- -16° 44′ 19″
- Constellation
- Libra
- Distance from Earth
- 1.62 AU
- Elongation from the Sun
- 13.9° — too close to the Sun to observe
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
- 0.838 AU
- Eccentricity
- 0.2404
- Inclination
- 6.42°
- Orbital period
- 280 days
- Perihelion
- 0.636 AU
- Aphelion
- 1.039 AU
- Longitude of ascending node
- 16.88°
- Argument of periapsis
- 167.43°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 10.3 LD
- 0.0266 AU
- Tisserand (Jupiter)
- 6.986
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 19
- Data arc
- 10 days
- First observed
- 30 September 2021
- Last observed
- 10 October 2021
- Residual RMS
- 0.59 ″
- Solution · Otto Matic
- 11 October 2021
Visual & observation
- Absolute magnitude (H)
- 26.51
Discovery & classification
Close approaches 85 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-04-13 19:45 UTC close approach of 2021 SP5. Catalogue miss distance 139.8 LD · 5.37 × 10⁷ km. The curve is the geocentric path from 2028-04-10 to 2028-04-16, 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 |
|---|---|---|---|---|
| 2028-04-13 19:45:00 | Earth | 0.3592 AU | 139.8 LD | 12.1 km/s |
| 2028-10-19 19:03:00 | Earth | 0.4986 AU | 194.0 LD | 21 km/s |
| 2031-06-12 00:20:00 | Earth | 0.2886 AU | 112.3 LD | 6.8 km/s |
| 2031-10-31 17:47:00 | Earth | 0.1151 AU | 44.8 LD | 8.7 km/s |
| 2034-09-01 08:06:00 | Earth | 0.1186 AU | 46.2 LD | 8.1 km/s |
| 2037-09-08 17:42:00 | Earth | 0.478 AU | 186.0 LD | 20.2 km/s |
| 2038-03-16 08:00:00 | Earth | 0.3585 AU | 139.5 LD | 12.1 km/s |
| 2041-05-05 17:48:00 | Earth | 0.3435 AU | 133.7 LD | 10.8 km/s |
| 2041-10-26 10:36:00 | Earth | 0.3395 AU | 132.1 LD | 15.9 km/s |
| 2047-09-02 04:04:00 | Earth | 0.2763 AU | 107.5 LD | 13.6 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