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Asteroid Near-Earth

2007 VV83

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(2007 VV83)

Where is it now

Distance from Sun
1.05 AU
True anomaly
205.78°
Distance from Earth
0.076 AU
As of
24 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 — 0.994 AU from the Sun Earth 2007 VV83 — 1.05 AU from the Sun 2007 VV83
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2007 VV83 is 0.076 AU from Earth today (37.7 light-seconds).

In the sky

Right ascension
23h 26m 16s
Declination
+41° 14′ 53″
Constellation
Andromeda
Distance from Earth
0.08 AU
Elongation from the Sun
135.98° — 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
0.967 AU
Eccentricity
0.0979
Inclination
10.12°
Orbital period
347.3 days
Perihelion
0.872 AU
Aphelion
1.062 AU
Longitude of ascending node
225.49°
Argument of periapsis
318.8°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 15.6 LD
0.04 AU
Tisserand (Jupiter)
6.226

Orbit quality

Orbit reasonably well determined (uncertainty code 5).

Observations used
26
Data arc
9 days
First observed
7 November 2007
Last observed
16 November 2007
Residual RMS
0.56 ″
Solution · Otto Matic
15 April 2021

Physical properties

Rotation period
0.15 hours

Visual & observation

Absolute magnitude (H)
24.7

Discovery & classification

Aten Near-Earth Object

Close approaches 68 on record

Flyby geometry
Ecliptic flyby of 2007 VV83 at 2026-11-07 00:21 UTC Top-down view of the ecliptic, Earth at the centre, for the 2026-11-07 00:21 UTC close approach of 2007 VV83. Catalogue miss distance 21.7 LD · 8.34 × 10⁶ km. The curve is the geocentric path from 2026-11-04 to 2026-11-10, 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 21.7 LD · 8.34 × 10⁶ km 2026-11-07 00:21 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2026-11-07 00:21 UTC close approach of 2007 VV83. Catalogue miss distance 21.7 LD · 8.34 × 10⁶ km. The curve is the geocentric path from 2026-11-04 to 2026-11-10, 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
2026-11-07 00:21:00 Earth 0.0558 AU 21.7 LD 5.5 km/s
2027-11-22 12:04:00 Earth 0.245 AU 95.4 LD 10.8 km/s
2044-07-27 13:26:00 Earth 0.3073 AU 119.6 LD 10.7 km/s
2045-06-03 00:20:00 Earth 0.1219 AU 47.5 LD 6.4 km/s
2045-10-17 12:32:00 Earth 0.1318 AU 51.3 LD 5.7 km/s
2046-03-26 20:28:00 Earth 0.1689 AU 65.7 LD 6 km/s
2046-11-21 12:15:00 Earth 0.1369 AU 53.3 LD 7.9 km/s
2047-11-18 15:48:00 Earth 0.4283 AU 166.7 LD 16.1 km/s
2063-08-06 18:46:00 Earth 0.4082 AU 158.9 LD 13.9 km/s
2064-06-28 03:14:00 Earth 0.1739 AU 67.7 LD 7 km/s

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

Sources