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Asteroid Near-Earth

2022 BV6

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(2022 BV6)

Where is it now

Distance from Sun
0.838 AU
True anomaly
137.29°
Distance from Earth
1.253 AU
As of
15 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 2022 BV6 — 0.838 AU from the Sun 2022 BV6
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2022 BV6 is 1.253 AU from Earth today (10.4 light-minutes).

In the sky

Right ascension
10h 48m 08s
Declination
+05° 58′ 44″
Constellation
Sextans
Distance from Earth
1.26 AU
Elongation from the Sun
42.08° — 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
0.71 AU
Eccentricity
0.5208
Inclination
8.37°
Orbital period
218.3 days
Perihelion
0.34 AU
Aphelion
1.079 AU
Longitude of ascending node
124.4°
Argument of periapsis
206.18°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 1.8 LD
0.0046 AU
Tisserand (Jupiter)
7.957

Orbit quality

Orbit very well determined (uncertainty code 2).

Observations used
40
Data arc
3.02 years
First observed
29 January 2022
Last observed
6 February 2025
Residual RMS
0.43 ″
Solution · Otto Matic
6 February 2025

Visual & observation

Absolute magnitude (H)
25.51

Discovery & classification

Aten Near-Earth Object

Close approaches 342 on record

Flyby geometry
Ecliptic flyby of 2022 BV6 at 2028-02-11 15:28 UTC Top-down view of the ecliptic, Earth at the centre, for the 2028-02-11 15:28 UTC close approach of 2022 BV6. Catalogue miss distance 39.3 LD · 1.51 × 10⁷ km. The curve is the geocentric path from 2028-02-08 to 2028-02-14, 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 39.3 LD · 1.51 × 10⁷ km 2028-02-11 15:28 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2028-02-11 15:28 UTC close approach of 2022 BV6. Catalogue miss distance 39.3 LD · 1.51 × 10⁷ km. The curve is the geocentric path from 2028-02-08 to 2028-02-14, 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
2027-09-23 15:58:00 Venus 0.1303 AU 50.7 LD 14.4 km/s
2028-02-11 15:28:00 Earth 0.1009 AU 39.3 LD 10.8 km/s
2028-05-04 10:27:00 Venus 0.0733 AU 28.5 LD 19.8 km/s
2031-02-20 12:13:00 Earth 0.1139 AU 44.3 LD 10.8 km/s
2034-03-01 04:02:00 Earth 0.1138 AU 44.3 LD 11 km/s
2037-03-08 06:49:00 Earth 0.1078 AU 42.0 LD 11.6 km/s
2037-06-03 09:30:00 Mercury 0.0341 AU 13.3 LD 28 km/s
2037-06-03 09:30:00 Merc 0.0341 AU 13.3 LD 28 km/s
2038-08-10 23:56:00 Mercury 0.0554 AU 21.6 LD 20 km/s
2038-08-10 23:56:00 Merc 0.0554 AU 21.6 LD 20 km/s

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

Sources