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Asteroid Near-Earth

464798

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464798 (2004 JX20)

Where is it now

Distance from Sun
1.139 AU
True anomaly
185.9°
Distance from Earth
1.756 AU
As of
20 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 — 0.996 AU from the Sun Earth 464798 — 1.139 AU from the Sun 464798
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 464798 is 1.756 AU from Earth today (14.6 light-minutes).

In the sky

Right ascension
16h 14m 40s
Declination
-20° 42′ 35″
Constellation
Scorpius
Distance from Earth
1.76 AU
Elongation from the Sun
37.27° — 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
0.902 AU
Eccentricity
0.2657
Inclination
10.53°
Orbital period
312.7 days
Perihelion
0.662 AU
Aphelion
1.141 AU
Longitude of ascending node
101.74°
Argument of periapsis
349.13°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 37.1 LD
0.0954 AU
Tisserand (Jupiter)
6.56

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
995
Data arc
19.93 years
First observed
15 May 2004
Last observed
20 April 2024
Residual RMS
0.37 ″
Solution · Otto Matic
2 January 2026

Physical properties

Mean radius
0.55 km
Rotation period
10.76 hours

Visual & observation

Geometric albedo
0.028
Absolute magnitude (H)
19.37

Discovery & classification

Discovered by
CSS
Discovery date
15 May 2004
Discovery site
Catalina

Also known as 2004 JX20

Aten Near-Earth Object

Close approaches 84 on record

Flyby geometry
Ecliptic flyby of 464798 at 2028-06-10 09:52 UTC Top-down view of the ecliptic, Earth at the centre, for the 2028-06-10 09:52 UTC close approach of 464798. Catalogue miss distance 54.5 LD · 2.1 × 10⁷ km. The curve is the geocentric path from 2028-06-07 to 2028-06-13, 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 54.5 LD · 2.1 × 10⁷ km 2028-06-10 09:52 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2028-06-10 09:52 UTC close approach of 464798. Catalogue miss distance 54.5 LD · 2.1 × 10⁷ km. The curve is the geocentric path from 2028-06-07 to 2028-06-13, 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
2028-06-10 09:52:00 Earth 0.1401 AU 54.5 LD 7.2 km/s
2030-09-13 05:35:00 Venus 0.0883 AU 34.4 LD 11.5 km/s
2034-06-15 18:28:00 Earth 0.1379 AU 53.7 LD 7.2 km/s
2034-12-05 16:21:00 Venus 0.0609 AU 23.7 LD 7.6 km/s
2039-02-13 18:31:00 Venus 0.1089 AU 42.4 LD 9.9 km/s
2040-06-20 07:40:00 Earth 0.1337 AU 52.0 LD 7.2 km/s
2046-06-28 01:02:00 Earth 0.1272 AU 49.5 LD 7.2 km/s
2052-07-03 16:36:00 Earth 0.1205 AU 46.9 LD 7.2 km/s
2054-08-26 19:25:00 Venus 0.0388 AU 15.1 LD 7.9 km/s
2058-07-09 01:42:00 Earth 0.1142 AU 44.4 LD 7.2 km/s

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

Sources