52768
Add to an observing list or journal →52768 (1998 OR2)
Where is it now
- Distance from Sun
- 2.944 AU
- True anomaly
- 217°
- Distance from Earth
- 2.273 AU
- As of
- 11 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
- 04h 51m 48s
- Declination
- +26° 33′ 01″
- Constellation
- Taurus
- Distance from Earth
- 2.26 AU
- Elongation from the Sun
- 124.19° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
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
- 2.379 AU
- Eccentricity
- 0.5758
- Inclination
- 5.88°
- Orbital period
- 3.67 years
- Perihelion
- 1.009 AU
- Aphelion
- 3.749 AU
- Longitude of ascending node
- 26.93°
- Argument of periapsis
- 174.57°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 2.8 LD
- 0.0072 AU
- Tisserand (Jupiter)
- 3.287
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 6,132
- Data arc
- 38.37 years
- First observed
- 30 June 1987
- Last observed
- 11 November 2025
- Residual RMS
- 0.23 ″
- Solution · Otto Matic
- 17 September 2026
Physical properties
- Mean radius
- 0.88 km
- Rotation period
- 4.11 hours
Visual & observation
- Absolute magnitude (H)
- 16.02
Discovery & classification
- Discovered by
- NEAT
- Discovery date
- 24 July 1998
- Discovery site
- Haleakala
Also known as 1998 OR2
Close approaches 19 on record
Top-down view of the ecliptic, Earth at the centre, for the 2031-05-18 06:56 UTC close approach of 52768. Catalogue miss distance 49.5 LD · 1.9 × 10⁷ km. The curve is the geocentric path from 2031-05-15 to 2031-05-21, 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 south 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 |
|---|---|---|---|---|
| 2031-05-18 06:56:00 | Earth | 0.1271 AU | 49.5 LD | 11.6 km/s |
| 2058-12-04 04:25:00 | Juptr | 1.1995 AU | 466.8 LD | 3.9 km/s |
| 2079-04-16 13:31:00 | Earth | 0.0118 AU | 4.6 LD | 8.2 km/s |
| 2079-04-16 14:37:00 | Moon | 0.0092 AU | 3.6 LD | 7.3 km/s |
| 2090-05-17 12:09:00 | Earth | 0.115 AU | 44.7 LD | 11.1 km/s |
| 2106-10-16 06:48:00 | Juptr | 1.8043 AU | 702.2 LD | 5.7 km/s |
| 2118-01-22 04:02:00 | Juptr | 1.2797 AU | 498.0 LD | 4.1 km/s |
| 2127-04-16 14:49:00 | Earth | 0.0168 AU | 6.5 LD | 8 km/s |
| 2138-05-20 21:53:00 | Earth | 0.1207 AU | 47.0 LD | 11.4 km/s |
| 2165-11-21 06:08:00 | Juptr | 1.3411 AU | 521.9 LD | 4.3 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)
- physical properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB