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Asteroid Near-Earth

Anteros

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1943 Anteros (1973 EC)

Where is it now

Distance from Sun
1.503 AU
True anomaly
115.54°
Distance from Earth
0.959 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 Anteros — 1.503 AU from the Sun Anteros
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. Anteros is 0.959 AU from Earth today (8.0 light-minutes).

In the sky

Right ascension
19h 54m 40s
Declination
-06° 57′ 04″
Constellation
Aquila
Distance from Earth
0.97 AU
Elongation from the Sun
100.08° — 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
1.431 AU
Eccentricity
0.2562
Inclination
8.71°
Orbital period
625.3 days
Perihelion
1.064 AU
Aphelion
1.798 AU
Longitude of ascending node
246.27°
Argument of periapsis
338.49°
Epoch · J2000
2461200.5
Orbit class · AMO
Amor
Earth MOID · 24.3 LD
0.0626 AU
Tisserand (Jupiter)
4.638

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
7,640
Data arc
53.58 years
First observed
10 March 1973
Last observed
9 October 2026
Residual RMS
0.38 ″
Solution · Otto Matic
10 October 2026

Physical properties

Mean radius
1.15 km
Rotation period
2.87 hours

Visual & observation

Geometric albedo
0.17
Absolute magnitude (H)
15.66
Colour index (B–V)
0.84
Spectral type (SMASS)
L
Spectral type (Tholen)
S
Colour index (U–B)
0.44

Discovery & classification

Discovered by
Gibson, J.
Discovery date
13 March 1973
Discovery site
El Leoncito

Also known as 1943 · 1973 EC

Amor Near-Earth Object Named

Close approaches 12 on record

Flyby geometry
Ecliptic flyby of Anteros at 2038-05-23 09:26 UTC Top-down view of the ecliptic, Earth at the centre, for the 2038-05-23 09:26 UTC close approach of Anteros. Catalogue miss distance 25.8 LD · 9.93 × 10⁶ km. The curve is the geocentric path from 2038-05-20 to 2038-05-26, 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 Moon’s position is approximate. The inset is a heliocentric view and is approximate. Sun 25.8 LD · 9.93 × 10⁶ km 2038-05-23 09:26 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2038-05-23 09:26 UTC close approach of Anteros. Catalogue miss distance 25.8 LD · 9.93 × 10⁶ km. The curve is the geocentric path from 2038-05-20 to 2038-05-26, 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 Moon’s position is approximate. The inset is a heliocentric view and is approximate.

JPL Horizons

When (UTC) Body Distance Lunar distances Relative speed
2038-05-23 09:26:00 Earth 0.0664 AU 25.8 LD 5.8 km/s
2050-05-20 09:34:00 Earth 0.0636 AU 24.8 LD 5.5 km/s
2062-05-14 21:01:00 Earth 0.096 AU 37.4 LD 5.5 km/s
2115-06-01 17:52:00 Earth 0.1396 AU 54.3 LD 7.5 km/s
2127-05-24 21:51:00 Earth 0.0651 AU 25.3 LD 5.8 km/s
2139-05-20 15:23:00 Earth 0.0684 AU 26.6 LD 5.4 km/s
2151-05-10 11:54:00 Earth 0.1482 AU 57.7 LD 6.3 km/s

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

Sources