470310
Add to an observing list or journal →470310 (2007 LB15)
Where is it now
- Distance from Sun
- 1.291 AU
- True anomaly
- 191.93°
- Distance from Earth
- 1.205 AU
- As of
- 22 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
- 18h 30m 29s
- Declination
- +02° 02′ 22″
- Constellation
- Serpens
- Distance from Earth
- 1.2 AU
- Elongation from the Sun
- 71.13° — well clear of the Sun
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
- 0.938 AU
- Eccentricity
- 0.3952
- Inclination
- 25.19°
- Orbital period
- 332 days
- Perihelion
- 0.567 AU
- Aphelion
- 1.309 AU
- Longitude of ascending node
- 262.77°
- Argument of periapsis
- 237.37°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 2.6 LD
- 0.0067 AU
- Tisserand (Jupiter)
- 6.251
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 190
- Data arc
- 19.15 years
- First observed
- 13 June 2007
- Last observed
- 7 August 2026
- Residual RMS
- 0.58 ″
- Solution · Otto Matic
- 8 August 2026
Visual & observation
- Absolute magnitude (H)
- 19.61
Discovery & classification
- Discovered by
- CSS
- Discovery date
- 13 June 2007
- Discovery site
- Catalina
Also known as 2007 LB15
Close approaches 30 on record
Top-down view of the ecliptic, Earth at the centre, for the 2036-06-20 22:44 UTC close approach of 470310. Catalogue miss distance 77.1 LD · 2.96 × 10⁷ km. The curve is the geocentric path from 2036-06-17 to 2036-06-23, 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 |
|---|---|---|---|---|
| 2036-06-20 22:44:00 | Earth | 0.1981 AU | 77.1 LD | 21.2 km/s |
| 2041-09-03 02:30:00 | Venus | 0.1054 AU | 41.0 LD | 20.4 km/s |
| 2043-06-27 22:01:00 | Venus | 0.1176 AU | 45.8 LD | 25 km/s |
| 2056-06-21 00:11:00 | Earth | 0.1975 AU | 76.9 LD | 21.2 km/s |
| 2062-07-31 20:31:00 | Venus | 0.0711 AU | 27.7 LD | 21.2 km/s |
| 2083-06-30 13:47:00 | Venus | 0.062 AU | 24.1 LD | 21.5 km/s |
| 2104-05-31 10:38:00 | Venus | 0.0627 AU | 24.4 LD | 21.5 km/s |
| 2125-05-01 14:40:00 | Venus | 0.0656 AU | 25.5 LD | 21.3 km/s |
| 2127-06-14 09:27:00 | Earth | 0.1978 AU | 77.0 LD | 13.5 km/s |
| 2137-06-13 16:16:00 | Earth | 0.1811 AU | 70.5 LD | 13.6 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