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Asteroid Near-Earth

Tukmit

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12711 Tukmit (1991 BB)

Where is it now

Distance from Sun
1.413 AU
True anomaly
144.9°
Distance from Earth
1.001 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.

Sun Earth — 0.998 AU from the Sun Earth Tukmit — 1.413 AU from the Sun Tukmit
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. Tukmit is 1.001 AU from Earth today (8.3 light-minutes).

In the sky

Right ascension
09h 23m 42s
Declination
+76° 57′ 22″
Constellation
Camelopardalis
Distance from Earth
1 AU
Elongation from the Sun
90.17° — 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
1.186 AU
Eccentricity
0.2721
Inclination
38.49°
Orbital period
471.9 days
Perihelion
0.864 AU
Aphelion
1.509 AU
Longitude of ascending node
294.96°
Argument of periapsis
322.9°
Epoch · J2000
2461200.5
Orbit class · APO
Apollo
Earth MOID · 43.4 LD
0.1114 AU
Tisserand (Jupiter)
5.106

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
3,788
Data arc
35.73 years
First observed
12 January 1991
Last observed
7 October 2026
Residual RMS
0.42 ″
Solution · Otto Matic
8 October 2026

Physical properties

Rotation period
3.48 hours

Visual & observation

Absolute magnitude (H)
16.02
Spectral type (SMASS)
Sr

Discovery & classification

Discovered by
Mueller, J. E.
Discovery date
19 January 1991
Discovery site
Palomar

Tukmit is Father Sky in the Luiseno creation story. He was made from nothingness and together with Tomaiyavit bore the First People. The First People became all the people, animals, plants and inanimate objects of the earth, the basis of Luiseno existence.

Also known as 12711 · 1991 BB

Apollo Near-Earth Object Named

Close approaches 15 on record

Flyby geometry
Ecliptic flyby of Tukmit at 2053-07-19 13:16 UTC Top-down view of the ecliptic, Earth at the centre, for the 2053-07-19 13:16 UTC close approach of Tukmit. Catalogue miss distance 43.2 LD · 1.66 × 10⁷ km. The curve is the geocentric path from 2053-07-16 to 2053-07-22, 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 43.2 LD · 1.66 × 10⁷ km 2053-07-19 13:16 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2053-07-19 13:16 UTC close approach of Tukmit. Catalogue miss distance 43.2 LD · 1.66 × 10⁷ km. The curve is the geocentric path from 2053-07-16 to 2053-07-22, 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
2053-07-19 13:16:00 Earth 0.111 AU 43.2 LD 22.1 km/s
2084-07-24 02:32:00 Earth 0.1317 AU 51.2 LD 22.6 km/s
2106-07-14 02:31:00 Earth 0.1522 AU 59.3 LD 21.7 km/s
2115-07-31 15:58:00 Earth 0.1957 AU 76.2 LD 23.6 km/s
2137-07-19 23:36:00 Earth 0.1114 AU 43.4 LD 22 km/s
2168-07-25 10:25:00 Earth 0.1318 AU 51.3 LD 22.6 km/s
2190-07-14 07:38:00 Earth 0.1525 AU 59.4 LD 21.7 km/s
2199-07-31 15:39:00 Earth 0.192 AU 74.7 LD 23.5 km/s

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

Sources