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Asteroid Near-Earth

2024 VC3

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(2024 VC3)

Where is it now

Distance from Sun
0.616 AU
True anomaly
44.45°
Distance from Earth
1.222 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 2024 VC3 — 0.616 AU from the Sun 2024 VC3
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2024 VC3 is 1.222 AU from Earth today (10.2 light-minutes).

In the sky

Right ascension
15h 09m 32s
Declination
-28° 42′ 10″
Constellation
Libra
Distance from Earth
1.22 AU
Elongation from the Sun
30.48° — near the Sun — look low at dusk or dawn

Favours the southern hemisphere; low or below the horizon from far north.

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
0.81 AU
Eccentricity
0.2885
Inclination
24.28°
Orbital period
266.3 days
Perihelion
0.576 AU
Aphelion
1.044 AU
Longitude of ascending node
49.82°
Argument of periapsis
195.44°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 14.3 LD
0.0368 AU
Tisserand (Jupiter)
7.112

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
91
Data arc
9 days
First observed
10 November 2024
Last observed
19 November 2024
Residual RMS
0.43 ″
Solution · Otto Matic
20 November 2024

Visual & observation

Absolute magnitude (H)
24.51

Discovery & classification

Aten Near-Earth Object

Close approaches 31 on record

Flyby geometry
Ecliptic flyby of 2024 VC3 at 2032-11-08 12:57 UTC Top-down view of the ecliptic, Earth at the centre, for the 2032-11-08 12:57 UTC close approach of 2024 VC3. Catalogue miss distance 37.0 LD · 1.42 × 10⁷ km. The curve is the geocentric path from 2032-11-05 to 2032-11-11, 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 37.0 LD · 1.42 × 10⁷ km 2032-11-08 12:57 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2032-11-08 12:57 UTC close approach of 2024 VC3. Catalogue miss distance 37.0 LD · 1.42 × 10⁷ km. The curve is the geocentric path from 2032-11-05 to 2032-11-11, 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
2032-11-08 12:57:00 Earth 0.0952 AU 37.0 LD 14.1 km/s
2033-04-05 09:51:00 Venus 0.1452 AU 56.5 LD 17.5 km/s
2051-11-16 02:54:00 Earth 0.1103 AU 42.9 LD 12.7 km/s
2052-12-15 06:17:00 Venus 0.1381 AU 53.8 LD 17.3 km/s
2059-11-11 13:43:00 Earth 0.0372 AU 14.5 LD 13 km/s
2067-11-09 04:51:00 Earth 0.1081 AU 42.1 LD 14.4 km/s
2078-11-21 15:51:00 Earth 0.1998 AU 77.8 LD 13.2 km/s
2086-11-15 10:18:00 Earth 0.1015 AU 39.5 LD 12.7 km/s
2094-11-11 03:42:00 Earth 0.0371 AU 14.4 LD 13.1 km/s
2102-11-09 22:21:00 Earth 0.1182 AU 46.0 LD 14.6 km/s

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

Sources