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Asteroid Near-Earth

20826

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20826 (2000 UV13)

Where is it now

Distance from Sun
2.966 AU
True anomaly
215.96°
Distance from Earth
2.177 AU
As of
11 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.

Orbit of Mercury Orbit of Venus Orbit of Mars Sun Earth — 0.998 AU from the Sun Earth 20826 — 2.966 AU from the Sun 20826
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 20826 is 2.177 AU from Earth today (18.1 light-minutes).

In the sky

Right ascension
02h 00m 43s
Declination
+51° 10′ 13″
Constellation
Perseus
Distance from Earth
2.17 AU
Elongation from the Sun
135.06° — 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
2.417 AU
Eccentricity
0.6367
Inclination
31.93°
Orbital period
3.76 years
Perihelion
0.878 AU
Aphelion
3.956 AU
Longitude of ascending node
347.29°
Argument of periapsis
198.69°
Epoch · J2000
2461200.5
Orbit class · APO
Apollo
Earth MOID · 35.9 LD
0.0923 AU
Tisserand (Jupiter)
3.045

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
3,822
Data arc
73.02 years
First observed
1 October 1953
Last observed
7 October 2026
Residual RMS
0.39 ″
Solution · Otto Matic
8 October 2026

Physical properties

Mean radius
1.84 km
Rotation period
5.31 hours

Visual & observation

Geometric albedo
0.123
Absolute magnitude (H)
13.85
Spectral type (SMASS)
Sq

Discovery & classification

Discovered by
BATTeRS
Discovery date
21 October 2000
Discovery site
Bisei SG Center

Also known as 2000 UV13

Apollo Near-Earth Object

Close approaches 14 on record

Flyby geometry
Ecliptic flyby of 20826 at 2099-03-13 14:55 UTC Top-down view of the ecliptic, Earth at the centre, for the 2099-03-13 14:55 UTC close approach of 20826. Catalogue miss distance 53.5 LD · 2.06 × 10⁷ km. The curve is the geocentric path from 2099-03-10 to 2099-03-16, 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 53.5 LD · 2.06 × 10⁷ km 2099-03-13 14:55 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2099-03-13 14:55 UTC close approach of 20826. Catalogue miss distance 53.5 LD · 2.06 × 10⁷ km. The curve is the geocentric path from 2099-03-10 to 2099-03-16, 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
2070-04-09 00:08:00 Juptr 1.7063 AU 664.0 LD 10.6 km/s
2081-11-01 17:51:00 Juptr 1.1844 AU 460.9 LD 8.1 km/s
2093-06-28 13:10:00 Juptr 1.6072 AU 625.5 LD 7.8 km/s
2099-03-13 14:55:00 Earth 0.1375 AU 53.5 LD 21.3 km/s
2153-04-04 00:08:00 Juptr 1.5798 AU 614.8 LD 10.1 km/s
2164-11-06 01:28:00 Juptr 1.2051 AU 469.0 LD 7.8 km/s
2176-07-13 20:51:00 Juptr 1.7335 AU 674.6 LD 7.9 km/s
2182-03-07 17:48:00 Earth 0.1221 AU 47.5 LD 21.6 km/s

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

Sources