Where is it now
- Distance from Sun
- 0.824 AU
- True anomaly
- 94.02°
- Distance from Earth
- 0.681 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
- 17h 25m 42s
- Declination
- -23° 36′ 41″
- Constellation
- Ophiuchus
- Distance from Earth
- 0.68 AU
- Elongation from the Sun
- 55.3° — 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
- 0.85 AU
- Eccentricity
- 0.2101
- Inclination
- 4.3°
- Orbital period
- 286.1 days
- Perihelion
- 0.671 AU
- Aphelion
- 1.028 AU
- Longitude of ascending node
- 348.77°
- Argument of periapsis
- 260.87°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 21.2 LD
- 0.0546 AU
- Tisserand (Jupiter)
- 6.912
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 41
- Data arc
- 81 days
- First observed
- 22 October 2023
- Last observed
- 11 January 2024
- Residual RMS
- 0.58 ″
- Solution · Otto Matic
- 16 January 2024
Visual & observation
- Absolute magnitude (H)
- 22.31
Discovery & classification
Close approaches 163 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-06-13 09:38 UTC close approach of 2023 UO9. Catalogue miss distance 135.2 LD · 5.2 × 10⁷ km. The curve is the geocentric path from 2027-06-10 to 2027-06-16, 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 |
|---|---|---|---|---|
| 2027-06-13 09:38:00 | Earth | 0.3473 AU | 135.2 LD | 10.5 km/s |
| 2027-12-28 22:58:00 | Earth | 0.4952 AU | 192.7 LD | 21 km/s |
| 2030-10-25 22:00:00 | Earth | 0.1217 AU | 47.4 LD | 8.9 km/s |
| 2031-03-29 19:20:00 | Earth | 0.2691 AU | 104.7 LD | 7.1 km/s |
| 2032-03-20 09:14:00 | Venus | 0.051 AU | 19.8 LD | 9.2 km/s |
| 2034-07-29 16:03:00 | Earth | 0.2946 AU | 114.6 LD | 7.8 km/s |
| 2035-01-10 11:20:00 | Earth | 0.1854 AU | 72.1 LD | 10.9 km/s |
| 2037-07-12 01:47:00 | Venus | 0.1069 AU | 41.6 LD | 10.8 km/s |
| 2037-11-06 09:52:00 | Earth | 0.4486 AU | 174.6 LD | 19.6 km/s |
| 2038-05-20 22:12:00 | Earth | 0.3438 AU | 133.8 LD | 10.5 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