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Asteroid Near-Earth

2004 FG29

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(2004 FG29)

Where is it now

Distance from Sun
0.863 AU
True anomaly
117.77°
Distance from Earth
0.879 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 2004 FG29 — 0.863 AU from the Sun 2004 FG29
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2004 FG29 is 0.879 AU from Earth today (7.3 light-minutes).

In the sky

Right ascension
10h 15m 26s
Declination
+07° 14′ 58″
Constellation
Leo
Distance from Earth
0.88 AU
Elongation from the Sun
54.54° — near the Sun — look low at dusk or dawn

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
0.878 AU
Eccentricity
0.4929
Inclination
3.43°
Orbital period
300.7 days
Perihelion
0.445 AU
Aphelion
1.311 AU
Longitude of ascending node
182.89°
Argument of periapsis
142.56°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 3.9 LD
0.0101 AU
Tisserand (Jupiter)
6.637

Orbit quality

Orbit poorly determined (uncertainty code 7).

Observations used
45
Data arc
2 days
First observed
29 March 2004
Last observed
31 March 2004
Residual RMS
0.5 ″
Solution · Otto Matic
14 April 2021

Visual & observation

Absolute magnitude (H)
26

Discovery & classification

Aten Near-Earth Object

Close approaches 76 on record

Flyby geometry
Ecliptic flyby of 2004 FG29 at 2027-03-14 11:16 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-03-14 11:16 UTC close approach of 2004 FG29. Catalogue miss distance 99.8 LD · 3.84 × 10⁷ km. The curve is the geocentric path from 2027-03-11 to 2027-03-17, 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 99.8 LD · 3.84 × 10⁷ km 2027-03-14 11:16 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-03-14 11:16 UTC close approach of 2004 FG29. Catalogue miss distance 99.8 LD · 3.84 × 10⁷ km. The curve is the geocentric path from 2027-03-11 to 2027-03-17, 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
2027-03-14 11:16:00 Earth 0.2565 AU 99.8 LD 11 km/s
2032-04-01 13:51:00 Earth 0.0351 AU 13.7 LD 15.9 km/s
2035-01-14 10:18:00 Earth 0.4711 AU 183.3 LD 30 km/s
2036-02-12 17:36:00 Earth 0.3257 AU 126.8 LD 11.7 km/s
2037-03-19 13:30:00 Earth 0.4058 AU 157.9 LD 27.8 km/s
2039-12-30 23:33:00 Earth 0.1079 AU 42.0 LD 17.6 km/s
2041-03-20 11:28:00 Earth 0.2226 AU 86.6 LD 10.8 km/s
2045-01-13 23:44:00 Earth 0.2449 AU 95.3 LD 10.8 km/s
2046-03-31 03:21:00 Earth 0.1117 AU 43.5 LD 18.3 km/s
2049-01-10 14:51:00 Earth 0.3943 AU 153.4 LD 27.4 km/s

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

Sources