Where is it now
- Distance from Sun
- 0.833 AU
- True anomaly
- 146.75°
- Distance from Earth
- 0.821 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
- 17h 04m 19s
- Declination
- -17° 34′ 00″
- Constellation
- Ophiuchus
- Distance from Earth
- 0.82 AU
- Elongation from the Sun
- 53.81° — 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
- 0.645 AU
- Eccentricity
- 0.5606
- Inclination
- 8.79°
- Orbital period
- 189.2 days
- Perihelion
- 0.283 AU
- Aphelion
- 1.006 AU
- Longitude of ascending node
- 186.35°
- Argument of periapsis
- 356.78°
- Epoch · J2000
- 2459486.5
- Orbit class · ATE
- Aten
- Earth MOID · 1.0 LD
- 0.0026 AU
- Tisserand (Jupiter)
- 8.644
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 8).
- Observations used
- 5
- First observed
- 29 September 2021
- Last observed
- 29 September 2021
- Residual RMS
- 0.1 ″
- Solution · Otto Matic
- 10 January 2024
Visual & observation
- Absolute magnitude (H)
- 30.92
Discovery & classification
Close approaches 100 on record
Top-down view of the ecliptic, Earth at the centre, for the 2032-10-01 18:32 UTC close approach of 2021 SJ88. Catalogue miss distance 171.2 LD · 6.58 × 10⁷ km. The curve is the geocentric path from 2032-09-28 to 2032-10-04, 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 |
|---|---|---|---|---|
| 2031-10-04 07:41:00 | Venus | 0.1083 AU | 42.2 LD | 24.5 km/s |
| 2032-10-01 18:32:00 | Earth | 0.4398 AU | 171.2 LD | 26.1 km/s |
| 2033-10-09 08:48:00 | Earth | 0.2387 AU | 92.9 LD | 18.7 km/s |
| 2036-09-12 10:40:00 | Earth | 0.1724 AU | 67.1 LD | 16.3 km/s |
| 2050-09-14 14:16:00 | Earth | 0.2519 AU | 98.0 LD | 19.4 km/s |
| 2051-09-21 14:09:00 | Earth | 0.4406 AU | 171.5 LD | 26.4 km/s |
| 2053-10-03 08:46:00 | Venus | 0.1181 AU | 46.0 LD | 20.3 km/s |
| 2056-09-29 15:47:00 | Mercury | 0.0889 AU | 34.6 LD | 34.5 km/s |
| 2056-09-29 15:47:00 | Merc | 0.0889 AU | 34.6 LD | 34.5 km/s |
| 2058-03-20 06:10:00 | Venus | 0.0516 AU | 20.1 LD | 20.4 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