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Asteroid Near-Earth

Sekhmet

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5381 Sekhmet (1991 JY)

Where is it now

Distance from Sun
1.049 AU
True anomaly
233.53°
Distance from Earth
1.18 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 Sekhmet — 1.049 AU from the Sun Sekhmet
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. Sekhmet is 1.18 AU from Earth today (9.8 light-minutes).

In the sky

Right ascension
15h 57m 24s
Declination
-63° 41′ 30″
Constellation
Triangulum Australe
Distance from Earth
1.18 AU
Elongation from the Sun
56.91° — near the Sun — look low at dusk or dawn

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
0.947 AU
Eccentricity
0.2964
Inclination
48.97°
Orbital period
336.9 days
Perihelion
0.667 AU
Aphelion
1.228 AU
Longitude of ascending node
58.53°
Argument of periapsis
37.44°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 43.8 LD
0.1127 AU
Tisserand (Jupiter)
6.027

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
1,473
Data arc
35.25 years
First observed
14 May 1991
Last observed
13 August 2026
Residual RMS
0.53 ″
Solution · Otto Matic
14 August 2026

Physical properties

Mean radius
0.47 km
Rotation period
2.82 hours

Visual & observation

Geometric albedo
0.507
Absolute magnitude (H)
16.75

Discovery & classification

Discovered by
Shoemaker, C. S.
Discovery date
14 May 1991
Discovery site
Palomar

Also known as 5381 · 1991 JY

Aten Near-Earth Object Named

Close approaches 23 on record

Flyby geometry
Ecliptic flyby of Sekhmet at 2038-05-20 20:40 UTC Top-down view of the ecliptic, Earth at the centre, for the 2038-05-20 20:40 UTC close approach of Sekhmet. Catalogue miss distance 77.3 LD · 2.97 × 10⁷ km. The curve is the geocentric path from 2038-05-17 to 2038-05-23, 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. At closest approach the object is north of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate. Sun 77.3 LD · 2.97 × 10⁷ km 2038-05-20 20:40 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2038-05-20 20:40 UTC close approach of Sekhmet. Catalogue miss distance 77.3 LD · 2.97 × 10⁷ km. The curve is the geocentric path from 2038-05-17 to 2038-05-23, 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. At closest approach the object is north of the ecliptic. 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
2038-05-20 20:40:00 Earth 0.1986 AU 77.3 LD 25.3 km/s
2050-05-19 23:14:00 Earth 0.1599 AU 62.2 LD 24.7 km/s
2062-05-19 07:35:00 Earth 0.1334 AU 51.9 LD 24.2 km/s
2074-05-18 20:58:00 Earth 0.1188 AU 46.2 LD 23.9 km/s
2086-05-18 13:31:00 Earth 0.1135 AU 44.2 LD 23.7 km/s
2098-05-18 09:13:00 Earth 0.1136 AU 44.2 LD 23.5 km/s
2110-05-19 06:36:00 Earth 0.1157 AU 45.0 LD 23.4 km/s
2122-05-19 05:18:00 Earth 0.1183 AU 46.0 LD 23.3 km/s
2134-05-19 05:07:00 Earth 0.1202 AU 46.8 LD 23.3 km/s
2146-05-19 05:14:00 Earth 0.1216 AU 47.3 LD 23.3 km/s

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

Sources