Skip to content
Public Universe
Asteroid Near-Earth

2022 CG1

Add to an observing list or journal →

(2022 CG1)

Where is it now

Distance from Sun
0.748 AU
True anomaly
50.57°
Distance from Earth
0.322 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 CG1 — 0.748 AU from the Sun 2022 CG1
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2022 CG1 is 0.322 AU from Earth today (2.7 light-minutes).

In the sky

Right ascension
12h 11m 52s
Declination
+14° 30′ 12″
Constellation
Coma Berenices
Distance from Earth
0.32 AU
Elongation from the Sun
33.62° — 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
0.877 AU
Eccentricity
0.198
Inclination
6.17°
Orbital period
299.9 days
Perihelion
0.703 AU
Aphelion
1.05 AU
Longitude of ascending node
311.48°
Argument of periapsis
37.56°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 3.3 LD
0.0084 AU
Tisserand (Jupiter)
6.735

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
27
Data arc
8 days
First observed
4 February 2022
Last observed
12 February 2022
Residual RMS
0.32 ″
Solution · Otto Matic
12 February 2022

Visual & observation

Absolute magnitude (H)
27.6

Discovery & classification

Aten Near-Earth Object

Close approaches 97 on record

Flyby geometry
Ecliptic flyby of 2022 CG1 at 2027-04-15 02:46 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-04-15 02:46 UTC close approach of 2022 CG1. Catalogue miss distance 97.8 LD · 3.76 × 10⁷ km. The curve is the geocentric path from 2027-04-12 to 2027-04-18, 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 south of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate. Sun 97.8 LD · 3.76 × 10⁷ km 2027-04-15 02:46 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-04-15 02:46 UTC close approach of 2022 CG1. Catalogue miss distance 97.8 LD · 3.76 × 10⁷ km. The curve is the geocentric path from 2027-04-12 to 2027-04-18, 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 south 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
2026-10-04 17:41:00 Earth 0.2997 AU 116.6 LD 8.9 km/s
2027-04-15 02:46:00 Earth 0.2514 AU 97.8 LD 12.1 km/s
2029-02-07 16:45:00 Venus 0.0842 AU 32.8 LD 10.5 km/s
2031-01-26 00:21:00 Earth 0.142 AU 55.3 LD 9.8 km/s
2031-07-22 21:44:00 Earth 0.2717 AU 105.7 LD 8.2 km/s
2031-07-25 23:16:00 Venus 0.0966 AU 37.6 LD 11 km/s
2034-01-08 23:20:00 Venus 0.1129 AU 44.0 LD 11.7 km/s
2035-10-21 16:15:00 Earth 0.2833 AU 110.3 LD 7.8 km/s
2036-04-16 05:38:00 Earth 0.1734 AU 67.5 LD 9.2 km/s
2036-06-24 12:43:00 Venus 0.1391 AU 54.1 LD 12.9 km/s

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

Sources