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Asteroid Near-Earth

Selqet

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136818 Selqet (1997 MW1)

Where is it now

Distance from Sun
1.027 AU
True anomaly
235.42°
Distance from Earth
0.88 AU
As of
22 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 — 0.995 AU from the Sun Earth Selqet — 1.027 AU from the Sun Selqet
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. Selqet is 0.88 AU from Earth today (7.3 light-minutes).

In the sky

Right ascension
18h 18m 09s
Declination
-08° 40′ 32″
Constellation
Serpens
Distance from Earth
0.88 AU
Elongation from the Sun
66.04° — well clear of the Sun

Visible from both hemispheres.

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
0.937 AU
Eccentricity
0.3463
Inclination
12.78°
Orbital period
331.5 days
Perihelion
0.613 AU
Aphelion
1.262 AU
Longitude of ascending node
259.91°
Argument of periapsis
203.84°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 44.0 LD
0.1131 AU
Tisserand (Jupiter)
6.327

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
781
Data arc
29.1 years
First observed
29 June 1997
Last observed
3 August 2026
Residual RMS
0.36 ″
Solution · Otto Matic
5 August 2026

Visual & observation

Absolute magnitude (H)
18.96

Discovery & classification

Discovered by
Tucker, R. A.
Discovery date
29 June 1997
Discovery site
Goodricke-Pigott

Selqet was the ancient Egyptian goddess of magic and protector of the other gods from the destroyer, Apep. She was one of the four guardians of the deceased. Her aid was beseeched by those afflicted by scorpion or other stings. The scorpion was her sacred creature.

Also known as 136818 · 1997 MW1

Aten Near-Earth Object Named

Close approaches 48 on record

Flyby geometry
Ecliptic flyby of Selqet at 2036-05-29 00:35 UTC Top-down view of the ecliptic, Earth at the centre, for the 2036-05-29 00:35 UTC close approach of Selqet. Catalogue miss distance 66.7 LD · 2.57 × 10⁷ km. The curve is the geocentric path from 2036-05-26 to 2036-06-01, 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 66.7 LD · 2.57 × 10⁷ km 2036-05-29 00:35 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2036-05-29 00:35 UTC close approach of Selqet. Catalogue miss distance 66.7 LD · 2.57 × 10⁷ km. The curve is the geocentric path from 2036-05-26 to 2036-06-01, 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
2032-06-15 00:27:00 Venus 0.1172 AU 45.6 LD 13.8 km/s
2034-03-25 09:28:00 Venus 0.1153 AU 44.9 LD 15.9 km/s
2036-05-29 00:35:00 Earth 0.1715 AU 66.7 LD 9.2 km/s
2051-07-02 23:01:00 Venus 0.0935 AU 36.4 LD 13.9 km/s
2065-05-14 22:59:00 Earth 0.1489 AU 57.9 LD 13.2 km/s
2070-07-21 14:15:00 Venus 0.085 AU 33.1 LD 14.2 km/s
2075-05-15 19:54:00 Earth 0.1149 AU 44.7 LD 11.3 km/s
2085-05-19 00:40:00 Earth 0.1226 AU 47.7 LD 9.8 km/s
2087-11-04 05:01:00 Venus 0.1391 AU 54.1 LD 13.8 km/s
2089-08-11 11:59:00 Venus 0.0918 AU 35.7 LD 14.8 km/s

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

Sources