2013 BP15 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.89 AU to 1.19 AU from the Sun; one orbit takes 386.4 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 1.122 AU
- True anomaly
- 229.02°
- Distance from Earth
- 1.44 AU
- As of
- 4 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
- 11h 25m 43s
- Declination
- +01° 33′ 42″
- Constellation
- Leo
- Distance from Earth
- 1.44 AU
- Elongation from the Sun
- 51.01° — 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
- 1.038 AU
- Eccentricity
- 0.1426
- Inclination
- 15.87°
- Orbital period
- 386.4 days
- Perihelion
- 0.89 AU
- Aphelion
- 1.186 AU
- Longitude of ascending node
- 299.18°
- Argument of periapsis
- 320.09°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 36.8 LD
- 0.0946 AU
- Tisserand (Jupiter)
- 5.863
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 16
- Data arc
- 16 days
- First observed
- 16 January 2013
- Last observed
- 1 February 2013
- Residual RMS
- 0.55 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 24.3
Discovery & classification
Close approaches 19 on record
Top-down view of the ecliptic, Earth at the centre, for the 2030-02-15 15:05 UTC close approach of 2013 BP15. Catalogue miss distance 128.3 LD · 4.93 × 10⁷ km. The curve is the geocentric path from 2030-02-12 to 2030-02-18, 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 |
|---|---|---|---|---|
| 2030-02-15 15:05:00 | Earth | 0.3298 AU | 128.3 LD | 14.3 km/s |
| 2031-02-01 09:54:00 | Earth | 0.1429 AU | 55.6 LD | 9.1 km/s |
| 2031-12-28 07:37:00 | Earth | 0.2618 AU | 101.9 LD | 8.7 km/s |
| 2032-08-03 10:40:00 | Earth | 0.1019 AU | 39.6 LD | 9.9 km/s |
| 2033-09-06 17:00:00 | Earth | 0.3771 AU | 146.7 LD | 16.4 km/s |
| 2048-02-15 18:12:00 | Earth | 0.4079 AU | 158.7 LD | 16.6 km/s |
| 2049-02-07 09:53:00 | Earth | 0.1574 AU | 61.3 LD | 9.6 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