745311
Add to an observing list or journal →745311 (2010 XC15)
Where is it now
- Distance from Sun
- 0.921 AU
- True anomaly
- 214.83°
- Distance from Earth
- 1.295 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
- 10h 42m 14s
- Declination
- +09° 42′ 47″
- Constellation
- Leo
- Distance from Earth
- 1.29 AU
- Elongation from the Sun
- 44.96° — near the Sun — look low at dusk or dawn
Visible from both hemispheres.
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
- 0.732 AU
- Eccentricity
- 0.4199
- Inclination
- 8.24°
- Orbital period
- 229 days
- Perihelion
- 0.425 AU
- Aphelion
- 1.04 AU
- Longitude of ascending node
- 94.4°
- Argument of periapsis
- 158.12°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.9 LD
- 0.0023 AU
- Tisserand (Jupiter)
- 7.778
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 279
- Data arc
- 12.06 years
- First observed
- 5 December 2010
- Last observed
- 28 December 2022
- Residual RMS
- 0.32 ″
- Solution · Otto Matic
- 14 December 2024
Physical properties
- Rotation period
- 2.67 hours
Visual & observation
- Absolute magnitude (H)
- 21.48
Discovery & classification
- Discovered by
- CSS
- Discovery date
- 5 December 2010
- Discovery site
- Catalina
Also known as 2010 XC15
Close approaches 215 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-12-18 20:37 UTC close approach of 745311. Catalogue miss distance 19.8 LD · 7.62 × 10⁶ km. The curve is the geocentric path from 2027-12-15 to 2027-12-21, 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 |
|---|---|---|---|---|
| 2026-12-25 09:48:00 | Merc | 0.0603 AU | 23.5 LD | 15.6 km/s |
| 2026-12-25 09:48:00 | Mercury | 0.0603 AU | 23.5 LD | 15.6 km/s |
| 2027-12-18 20:37:00 | Earth | 0.0509 AU | 19.8 LD | 8.9 km/s |
| 2030-02-16 13:42:00 | Merc | 0.0486 AU | 18.9 LD | 16 km/s |
| 2030-02-16 13:42:00 | Mercury | 0.0486 AU | 18.9 LD | 16 km/s |
| 2032-12-01 21:54:00 | Earth | 0.0823 AU | 32.0 LD | 8.8 km/s |
| 2033-02-20 15:51:00 | Venus | 0.1042 AU | 40.6 LD | 20.2 km/s |
| 2033-04-09 16:40:00 | Merc | 0.0318 AU | 12.4 LD | 18.4 km/s |
| 2033-04-09 16:40:00 | Mercury | 0.0318 AU | 12.4 LD | 18.4 km/s |
| 2033-10-05 21:27:00 | Venus | 0.0378 AU | 14.7 LD | 16 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)
- orbital elements: JPL SBDB