2020 BN10
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Where is it now
- Distance from Sun
- 1.011 AU
- True anomaly
- 123.72°
- Distance from Earth
- 0.202 AU
- As of
- 21 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
- 20h 28m 40s
- Declination
- -43° 18′ 39″
- Constellation
- Microscopium
- Distance from Earth
- 0.21 AU
- Elongation from the Sun
- 89.63° — well clear of the Sun
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
- 0.928 AU
- Eccentricity
- 0.3443
- Inclination
- 20.52°
- Orbital period
- 326.4 days
- Perihelion
- 0.608 AU
- Aphelion
- 1.247 AU
- Longitude of ascending node
- 185.74°
- Argument of periapsis
- 69.02°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 18.6 LD
- 0.0479 AU
- Tisserand (Jupiter)
- 6.351
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 57
- Data arc
- 10.27 years
- First observed
- 30 September 2010
- Last observed
- 5 January 2021
- Residual RMS
- 0.47 ″
- Solution · Otto Matic
- 1 March 2023
Visual & observation
- Absolute magnitude (H)
- 20.99
Discovery & classification
Close approaches 185 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-07-21 10:23 UTC close approach of 2020 BN10. Catalogue miss distance 177.7 LD · 6.83 × 10⁷ km. The curve is the geocentric path from 2027-07-18 to 2027-07-24, 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 north 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 |
|---|---|---|---|---|
| 2026-10-10 07:08:00 | Earth | 0.1494 AU | 58.1 LD | 18.3 km/s |
| 2027-07-21 10:23:00 | Earth | 0.4566 AU | 177.7 LD | 12.1 km/s |
| 2027-11-15 21:56:00 | Earth | 0.4369 AU | 170.0 LD | 10.2 km/s |
| 2028-04-19 00:13:00 | Venus | 0.1292 AU | 50.3 LD | 21.7 km/s |
| 2028-04-23 23:53:00 | Earth | 0.3882 AU | 151.1 LD | 15.6 km/s |
| 2029-02-13 21:36:00 | Earth | 0.2753 AU | 107.1 LD | 19.3 km/s |
| 2034-10-21 04:54:00 | Earth | 0.3982 AU | 155.0 LD | 25.4 km/s |
| 2035-09-30 06:32:00 | Earth | 0.247 AU | 96.1 LD | 10.9 km/s |
| 2036-05-26 17:05:00 | Earth | 0.4716 AU | 183.5 LD | 16.1 km/s |
| 2037-03-07 05:32:00 | Earth | 0.2114 AU | 82.3 LD | 14.8 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