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Asteroid Near-Earth

2005 VL1

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(2005 VL1)

Where is it now

Distance from Sun
0.901 AU
True anomaly
105.61°
Distance from Earth
0.281 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 2005 VL1 — 0.901 AU from the Sun 2005 VL1
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2005 VL1 is 0.281 AU from Earth today (2.3 light-minutes).

In the sky

Right ascension
18h 03m 15s
Declination
-23° 46′ 14″
Constellation
Sagittarius
Distance from Earth
0.28 AU
Elongation from the Sun
62.86° — well clear of the Sun

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
0.891 AU
Eccentricity
0.2246
Inclination
0.24°
Orbital period
307.3 days
Perihelion
0.691 AU
Aphelion
1.091 AU
Longitude of ascending node
37.88°
Argument of periapsis
227.8°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 0.0 LD
0 AU
Tisserand (Jupiter)
6.645

Orbit quality

Orbit reasonably well determined (uncertainty code 4).

Observations used
79
Data arc
16.08 years
First observed
4 November 2005
Last observed
4 December 2021
Residual RMS
0.43 ″
Solution · Davide Farnocchia
20 December 2022

Visual & observation

Absolute magnitude (H)
26.45

Discovery & classification

Aten Near-Earth Object

Close approaches 85 on record

Flyby geometry
Ecliptic flyby of 2005 VL1 at 2026-11-03 07:03 UTC Top-down view of the ecliptic, Earth at the centre, for the 2026-11-03 07:03 UTC close approach of 2005 VL1. Catalogue miss distance 94.7 LD · 3.64 × 10⁷ km. The curve is the geocentric path from 2026-10-31 to 2026-11-06, 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 94.7 LD · 3.64 × 10⁷ km 2026-11-03 07:03 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2026-11-03 07:03 UTC close approach of 2005 VL1. Catalogue miss distance 94.7 LD · 3.64 × 10⁷ km. The curve is the geocentric path from 2026-10-31 to 2026-11-06, 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
2026-11-03 07:03:00 Earth 0.2432 AU 94.7 LD 14.1 km/s
2027-06-14 23:58:00 Earth 0.3243 AU 126.2 LD 10.3 km/s
2028-01-31 05:14:00 Earth 0.308 AU 119.9 LD 16.1 km/s
2032-08-01 14:41:00 Earth 0.2892 AU 112.6 LD 8.4 km/s
2033-02-04 10:27:00 Earth 0.019 AU 7.4 LD 5.9 km/s
2033-04-16 20:27:00 Venus 0.0288 AU 11.2 LD 6.7 km/s
2037-11-01 07:18:00 Earth 0.0289 AU 11.2 LD 5.6 km/s
2038-05-02 15:34:00 Earth 0.2836 AU 110.4 LD 8.2 km/s
2042-09-10 02:11:00 Venus 0.1065 AU 41.5 LD 10.7 km/s
2042-11-03 07:16:00 Earth 0.2614 AU 101.7 LD 14.6 km/s

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

Sources