Skip to content
Public Universe
Asteroid Near-Earth

2012 BX34

Add to an observing list or journal →

(2012 BX34)

Where is it now

Distance from Sun
0.762 AU
True anomaly
248.7°
Distance from Earth
1.686 AU
As of
16 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 — 0.997 AU from the Sun Earth 2012 BX34 — 0.762 AU from the Sun 2012 BX34
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2012 BX34 is 1.686 AU from Earth today (14.0 light-minutes).

In the sky

Right ascension
12h 30m 16s
Declination
-06° 54′ 04″
Constellation
Virgo
Distance from Earth
1.69 AU
Elongation from the Sun
14.3° — too close to the Sun to observe

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
0.76 AU
Eccentricity
0.3582
Inclination
10.53°
Orbital period
242.2 days
Perihelion
0.488 AU
Aphelion
1.033 AU
Longitude of ascending node
306.67°
Argument of periapsis
335.98°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 0.1 LD
0.0002 AU
Tisserand (Jupiter)
7.545

Orbit quality

Orbit reasonably well determined (uncertainty code 3).

Observations used
129
Data arc
2 days
First observed
25 January 2012
Last observed
27 January 2012
Residual RMS
0.42 ″
Solution · Otto Matic
15 April 2021

Physical properties

Rotation period
1.81 hours

Visual & observation

Absolute magnitude (H)
27.6

Discovery & classification

Aten Near-Earth Object

Close approaches 193 on record

Flyby geometry
Ecliptic flyby of 2012 BX34 at 2027-08-16 16:04 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-08-16 16:04 UTC close approach of 2012 BX34. Catalogue miss distance 190.9 LD · 7.34 × 10⁷ km. The curve is the geocentric path from 2027-08-13 to 2027-08-19, 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. Sun 190.9 LD · 7.34 × 10⁷ km 2027-08-16 16:04 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-08-16 16:04 UTC close approach of 2012 BX34. Catalogue miss distance 190.9 LD · 7.34 × 10⁷ km. The curve is the geocentric path from 2027-08-13 to 2027-08-19, 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.

JPL Horizons

When (UTC) Body Distance Lunar distances Relative speed
2027-08-16 16:04:00 Earth 0.4905 AU 190.9 LD 18.3 km/s
2028-01-22 06:21:00 Earth 0.42 AU 163.5 LD 22.7 km/s
2030-01-19 07:37:00 Earth 0.4826 AU 187.8 LD 24.8 km/s
2042-02-23 22:17:00 Merc 0.091 AU 35.4 LD 18.6 km/s
2042-02-23 22:17:00 Mercury 0.091 AU 35.4 LD 18.6 km/s
2044-10-19 22:02:00 Merc 0.0751 AU 29.2 LD 17.3 km/s
2044-10-19 22:02:00 Mercury 0.0751 AU 29.2 LD 17.3 km/s
2047-06-16 01:15:00 Merc 0.0597 AU 23.2 LD 16.2 km/s
2047-06-16 01:15:00 Mercury 0.0597 AU 23.2 LD 16.2 km/s
2050-02-09 05:50:00 Mercury 0.0458 AU 17.8 LD 15.3 km/s

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

Sources