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Asteroid Near-Earth

2022 BV3

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(2022 BV3)

Where is it now

Distance from Sun
0.925 AU
True anomaly
112.39°
Distance from Earth
0.282 AU
As of
20 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 — 0.996 AU from the Sun Earth 2022 BV3 — 0.925 AU from the Sun 2022 BV3
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2022 BV3 is 0.282 AU from Earth today (2.3 light-minutes).

In the sky

Right ascension
17h 39m 45s
Declination
+26° 26′ 56″
Constellation
Hercules
Distance from Earth
0.28 AU
Elongation from the Sun
68.19° — well clear of the Sun

Favours the northern hemisphere; low or below the horizon from far south.

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
0.897 AU
Eccentricity
0.2872
Inclination
14.01°
Orbital period
310.5 days
Perihelion
0.64 AU
Aphelion
1.155 AU
Longitude of ascending node
305.87°
Argument of periapsis
320.05°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 18.5 LD
0.0477 AU
Tisserand (Jupiter)
6.57

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
45
Data arc
16 days
First observed
28 January 2022
Last observed
13 February 2022
Residual RMS
0.37 ″
Solution · Otto Matic
30 March 2024

Visual & observation

Absolute magnitude (H)
22.96

Discovery & classification

Aten Near-Earth Object

Close approaches 194 on record

Flyby geometry
Ecliptic flyby of 2022 BV3 at 2026-10-22 09:13 UTC Top-down view of the ecliptic, Earth at the centre, for the 2026-10-22 09:13 UTC close approach of 2022 BV3. Catalogue miss distance 105.9 LD · 4.07 × 10⁷ km. The curve is the geocentric path from 2026-10-19 to 2026-10-25, 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 105.9 LD · 4.07 × 10⁷ km 2026-10-22 09:13 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2026-10-22 09:13 UTC close approach of 2022 BV3. Catalogue miss distance 105.9 LD · 4.07 × 10⁷ km. The curve is the geocentric path from 2026-10-19 to 2026-10-25, 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
2026-10-22 09:13:00 Earth 0.2721 AU 105.9 LD 13.3 km/s
2027-06-22 01:45:00 Earth 0.3936 AU 153.2 LD 14.7 km/s
2028-02-04 00:38:00 Earth 0.1421 AU 55.3 LD 14 km/s
2032-09-09 16:02:00 Earth 0.2643 AU 102.9 LD 10.1 km/s
2032-12-06 00:45:00 Earth 0.2613 AU 101.7 LD 8.3 km/s
2033-05-12 21:45:00 Earth 0.3954 AU 153.9 LD 11.8 km/s
2034-01-25 11:16:00 Earth 0.4367 AU 170.0 LD 23 km/s
2037-09-01 19:07:00 Venus 0.1496 AU 58.2 LD 12.7 km/s
2037-11-06 10:10:00 Earth 0.4915 AU 191.3 LD 22.4 km/s
2038-07-28 07:50:00 Earth 0.3431 AU 133.5 LD 13.7 km/s

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

Sources