2001 SH276 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.84 AU to 1.21 AU from the Sun; one orbit takes 380.8 days. Orbit from the JPL solution of 2 November 2026.
Where is it now
- Distance from Sun
- 1.175 AU
- True anomaly
- 148.26°
- Distance from Earth
- 0.252 AU
- As of
- 3 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
- 01h 41m 13s
- Declination
- -31° 35′ 34″
- Constellation
- Sculptor
- Distance from Earth
- 0.26 AU
- Elongation from the Sun
- 130.98° — well clear of the Sun
Favours the southern hemisphere; low or below the horizon from far north.
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
- 1.028 AU
- Eccentricity
- 0.1807
- Inclination
- 20.4°
- Orbital period
- 380.8 days
- Perihelion
- 0.842 AU
- Aphelion
- 1.214 AU
- Longitude of ascending node
- 194.94°
- Argument of periapsis
- 54.3°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 35.9 LD
- 0.0923 AU
- Tisserand (Jupiter)
- 5.88
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 645
- Data arc
- 25.1 years
- First observed
- 26 September 2001
- Last observed
- 2 November 2026
- Residual RMS
- 0.37 ″
- Solution · Otto Matic
- 2 November 2026
Visual & observation
- Absolute magnitude (H)
- 19.69
Discovery & classification
Close approaches 38 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-09-29 22:11 UTC close approach of 2001 SH276. Catalogue miss distance 64.9 LD · 2.49 × 10⁷ km. The curve is the geocentric path from 2027-09-26 to 2027-10-02, 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 |
|---|---|---|---|---|
| 2026-10-05 03:48:00 | Earth | 0.1398 AU | 54.4 LD | 10.8 km/s |
| 2027-09-29 22:11:00 | Earth | 0.1668 AU | 64.9 LD | 13.7 km/s |
| 2048-03-14 14:03:00 | Earth | 0.1997 AU | 77.7 LD | 15.2 km/s |
| 2049-04-06 04:30:00 | Earth | 0.1167 AU | 45.4 LD | 11.9 km/s |
| 2051-10-01 02:39:00 | Earth | 0.0992 AU | 38.6 LD | 11.7 km/s |
| 2073-03-26 08:20:00 | Earth | 0.0987 AU | 38.4 LD | 12.8 km/s |
| 2075-10-04 19:58:00 | Earth | 0.1309 AU | 50.9 LD | 10.8 km/s |
| 2076-09-29 08:43:00 | Earth | 0.1779 AU | 69.3 LD | 14 km/s |
| 2097-03-15 21:10:00 | Earth | 0.1891 AU | 73.6 LD | 15 km/s |
| 2098-04-07 20:56:00 | Earth | 0.1237 AU | 48.1 LD | 11.8 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