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Asteroid Near-Earth

2012 BV13

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(2012 BV13)

Where is it now

Distance from Sun
0.938 AU
True anomaly
268.17°
Distance from Earth
1.662 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.

Sun Earth — 0.995 AU from the Sun Earth 2012 BV13 — 0.938 AU from the Sun 2012 BV13
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2012 BV13 is 1.662 AU from Earth today (13.8 light-minutes).

In the sky

Right ascension
11h 54m 26s
Declination
-03° 31′ 24″
Constellation
Virgo
Distance from Earth
1.66 AU
Elongation from the Sun
29.68° — 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.

How do I find my coordinates?

Google Maps on a computer

  1. Right-click the spot where you'll be observing.
  2. The first line of the menu is the coordinates, e.g. 51.50722, -0.12758 — click it and they're copied.
  3. Paste them above.

Google Maps on a phone

  1. Press and hold the spot to drop a pin.
  2. The coordinates appear in the search bar (or on the pin's card) — tap to copy, then paste above.

A full Google Maps link works too, but the short maps.app.goo.gl share links don't carry coordinates — copy the numbers instead. We round to about a kilometre; that's all the sky calculation needs.

Know your what3words address? Paste it, e.g. ///filled.count.soap. This is optional — the three words are sent to what3words to convert them, and we don't store the address or the result.

Your location stays in your browser and is sent only for this calculation. Using a what3words address is optional; if you do, the three words go to what3words to be converted and we don't record them. Set a location first, then you can save an email alert for this object. See our privacy policy.

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
0.944 AU
Eccentricity
0.1007
Inclination
12.22°
Orbital period
335.1 days
Perihelion
0.849 AU
Aphelion
1.039 AU
Longitude of ascending node
295.41°
Argument of periapsis
305.16°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 3.0 LD
0.0076 AU
Tisserand (Jupiter)
6.339

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
240
Data arc
11.04 years
First observed
19 January 2012
Last observed
1 February 2023
Residual RMS
0.34 ″
Solution · Otto Matic
3 September 2024

Visual & observation

Absolute magnitude (H)
22.29

Discovery & classification

Aten Near-Earth Object

Close approaches 80 on record

Flyby geometry
Ecliptic flyby of 2012 BV13 at 2032-09-30 22:39 UTC Top-down view of the ecliptic, Earth at the centre, for the 2032-09-30 22:39 UTC close approach of 2012 BV13. Catalogue miss distance 174.4 LD · 6.7 × 10⁷ km. The curve is the geocentric path from 2032-09-27 to 2032-10-03, 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. Sun 174.4 LD · 6.7 × 10⁷ km 2032-09-30 22:39 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2032-09-30 22:39 UTC close approach of 2012 BV13. Catalogue miss distance 174.4 LD · 6.7 × 10⁷ km. The curve is the geocentric path from 2032-09-27 to 2032-10-03, 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.

JPL Horizons

When (UTC) Body Distance Lunar distances Relative speed
2032-09-30 22:39:00 Earth 0.4482 AU 174.4 LD 16.2 km/s
2033-07-31 10:01:00 Earth 0.1232 AU 48.0 LD 7.5 km/s
2034-01-12 12:16:00 Earth 0.094 AU 36.6 LD 6.5 km/s
2035-01-09 09:47:00 Earth 0.4086 AU 159.0 LD 16.8 km/s
2044-08-18 13:07:00 Earth 0.1457 AU 56.7 LD 8 km/s
2044-12-25 03:35:00 Earth 0.1985 AU 77.2 LD 7.1 km/s
2045-04-30 14:13:00 Earth 0.2448 AU 95.3 LD 4.9 km/s
2046-01-12 22:56:00 Earth 0.2904 AU 113.0 LD 13.4 km/s
2055-09-09 20:03:00 Earth 0.2434 AU 94.7 LD 10.3 km/s
2056-06-16 05:05:00 Earth 0.1981 AU 77.1 LD 7.3 km/s

Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.

Sources