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Asteroid Near-Earth

Zeus

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5731 Zeus (1988 VP4)

Where is it now

Distance from Sun
1.118 AU
True anomaly
75.51°
Distance from Earth
2.086 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 Zeus — 1.118 AU from the Sun Zeus
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. Zeus is 2.086 AU from Earth today (17.4 light-minutes).

In the sky

Right ascension
13h 34m 59s
Declination
-15° 45′ 15″
Constellation
Virgo
Distance from Earth
2.09 AU
Elongation from the Sun
10.23° — too close to the Sun to observe

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
2.265 AU
Eccentricity
0.6525
Inclination
11.2°
Orbital period
3.41 years
Perihelion
0.787 AU
Aphelion
3.743 AU
Longitude of ascending node
280.59°
Argument of periapsis
218.45°
Epoch · J2000
2461200.5
Orbit class · APO
Apollo
Earth MOID · 25.2 LD
0.0649 AU
Tisserand (Jupiter)
3.278

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
1,607
Data arc
37.11 years
First observed
13 September 1988
Last observed
23 October 2025
Residual RMS
0.48 ″
Solution · Otto Matic
4 August 2026

Physical properties

Mean radius
2.62 km

Visual & observation

Geometric albedo
0.031
Absolute magnitude (H)
15.47

Discovery & classification

Discovered by
Shoemaker, C. S., Shoemaker, E. M.
Discovery date
4 November 1988
Discovery site
Palomar

Also known as 5731 · 1988 VP4

Apollo Near-Earth Object Named

Close approaches 18 on record

Flyby geometry
Ecliptic flyby of Zeus at 2029-12-08 14:39 UTC Top-down view of the ecliptic, Earth at the centre, for the 2029-12-08 14:39 UTC close approach of Zeus. Catalogue miss distance 38.5 LD · 1.48 × 10⁷ km. The curve is the geocentric path from 2029-12-05 to 2029-12-11, 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 38.5 LD · 1.48 × 10⁷ km 2029-12-08 14:39 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2029-12-08 14:39 UTC close approach of Zeus. Catalogue miss distance 38.5 LD · 1.48 × 10⁷ km. The curve is the geocentric path from 2029-12-05 to 2029-12-11, 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
2029-12-08 14:39:00 Earth 0.0988 AU 38.5 LD 18.2 km/s
2036-10-25 18:30:00 Venus 0.1499 AU 58.3 LD 11.1 km/s
2045-04-10 08:15:00 Juptr 1.5474 AU 602.2 LD 5.6 km/s
2047-01-14 11:13:00 Earth 0.1703 AU 66.3 LD 13.5 km/s
2064-04-13 21:44:00 Earth 0.1887 AU 73.4 LD 15.9 km/s
2069-02-21 03:52:00 Juptr 1.7696 AU 688.7 LD 6.6 km/s
2151-07-30 03:04:00 Juptr 1.7165 AU 668.0 LD 5.2 km/s
2159-12-12 18:12:00 Earth 0.0643 AU 25.0 LD 17.4 km/s
2175-06-07 14:44:00 Juptr 1.5528 AU 604.3 LD 4.8 km/s
2177-01-28 12:31:00 Venus 0.1304 AU 50.7 LD 11.2 km/s

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

Sources