2025 BM2 is an asteroid in the Aten orbit class. Its orbit takes it from 0.82 AU to 1.14 AU from the Sun; one orbit takes 354.2 days. Orbit from the JPL solution of 11 February 2025.
Where is it now
- Distance from Sun
- 1.137 AU
- True anomaly
- 175.24°
- Distance from Earth
- 0.703 AU
- As of
- 24 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
- 08h 36m 54s
- Declination
- +07° 19′ 41″
- Constellation
- Cancer
- Distance from Earth
- 0.7 AU
- Elongation from the Sun
- 82.24° — 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
- 0.98 AU
- Eccentricity
- 0.1611
- Inclination
- 7.83°
- Orbital period
- 354.2 days
- Perihelion
- 0.822 AU
- Aphelion
- 1.137 AU
- Longitude of ascending node
- 127.41°
- Argument of periapsis
- 125.73°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 16.8 LD
- 0.0432 AU
- Tisserand (Jupiter)
- 6.16
Orbit quality
Orbit reasonably well determined (uncertainty code 4).
- Observations used
- 30
- Data arc
- 46 days
- First observed
- 27 December 2024
- Last observed
- 11 February 2025
- Residual RMS
- 0.73 ″
- Solution · Otto Matic
- 11 February 2025
Visual & observation
- Absolute magnitude (H)
- 25.31
Discovery & classification
Close approaches 70 on record
Top-down view of the ecliptic, Earth at the centre, for the 2053-09-08 08:02 UTC close approach of 2025 BM2. Catalogue miss distance 37.5 LD · 1.44 × 10⁷ km. The curve is the geocentric path from 2053-09-05 to 2053-09-11, 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 |
|---|---|---|---|---|
| 2043-11-01 02:06:00 | Venus | 0.125 AU | 48.7 LD | 2.3 km/s |
| 2050-07-07 14:29:00 | Venus | 0.1495 AU | 58.2 LD | 1.7 km/s |
| 2053-09-08 08:02:00 | Earth | 0.0962 AU | 37.5 LD | 6.6 km/s |
| 2054-07-28 20:12:00 | Earth | 0.1554 AU | 60.5 LD | 6.2 km/s |
| 2054-11-15 03:20:00 | Earth | 0.1947 AU | 75.8 LD | 4.6 km/s |
| 2056-01-02 21:54:00 | Earth | 0.1633 AU | 63.6 LD | 5.4 km/s |
| 2057-02-08 15:46:00 | Earth | 0.0525 AU | 20.4 LD | 5.8 km/s |
| 2058-02-11 09:12:00 | Earth | 0.1556 AU | 60.6 LD | 10.4 km/s |
| 2069-01-29 20:09:00 | Venus | 0.1342 AU | 52.2 LD | 2.9 km/s |
| 2075-10-01 12:06:00 | Venus | 0.1433 AU | 55.7 LD | 1.1 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