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Asteroid Near-Earth

2023 SM3

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(2023 SM3)

2023 SM3 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.71 AU to 1.36 AU from the Sun; one orbit takes 384.1 days. Orbit from the JPL solution of 21 September 2023.

Where is it now

Distance from Sun
1.024 AU
True anomaly
106.33°
Distance from Earth
0.943 AU
As of
3 November 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 — 0.992 AU from the Sun Earth 2023 SM3 — 1.024 AU from the Sun 2023 SM3
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2023 SM3 is 0.943 AU from Earth today (7.8 light-minutes).

In the sky

Right ascension
19h 11m 23s
Declination
-24° 04′ 23″
Constellation
Sagittarius
Distance from Earth
0.95 AU
Elongation from the Sun
64.03° — 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
1.034 AU
Eccentricity
0.3111
Inclination
13.28°
Orbital period
384.1 days
Perihelion
0.712 AU
Aphelion
1.356 AU
Longitude of ascending node
352.77°
Argument of periapsis
246.27°
Epoch · J2000
2460207.5
Orbit class · APO
Apollo
Earth MOID · 13.2 LD
0.0339 AU
Tisserand (Jupiter)
5.857

Orbit quality

Orbit very uncertain — the object may be effectively lost (uncertainty code 8).

Observations used
16
Data arc
2 days
First observed
19 September 2023
Last observed
21 September 2023
Residual RMS
0.25 ″
Solution · Otto Matic
21 September 2023

Visual & observation

Absolute magnitude (H)
26.71

Discovery & classification

Apollo Near-Earth Object

Close approaches 7 on record

Flyby geometry
Ecliptic flyby of 2023 SM3 at 2145-09-09 19:29 UTC Sun 7 Sep 13.6 LD · 5.21 × 10⁶ km 2145-09-09 19:29 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2145-09-09 19:29 UTC close approach of 2023 SM3. Catalogue miss distance 13.6 LD · 5.21 × 10⁶ km. The curve is the geocentric path from 2145-09-06 to 2145-09-12, 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 south 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
2145-09-09 19:29:00 Earth 0.0348 AU 13.6 LD 11.4 km/s

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

Sources