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Asteroid Near-Earth

2013 GT66

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(2013 GT66)

Where is it now

Distance from Sun
0.633 AU
True anomaly
309.02°
Distance from Earth
1.216 AU
As of
19 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 2013 GT66 — 0.633 AU from the Sun 2013 GT66
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2013 GT66 is 1.216 AU from Earth today (10.1 light-minutes).

In the sky

Right ascension
15h 33m 03s
Declination
-26° 55′ 45″
Constellation
Libra
Distance from Earth
1.21 AU
Elongation from the Sun
31.35° — 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
0.85 AU
Eccentricity
0.3233
Inclination
14.6°
Orbital period
286.3 days
Perihelion
0.575 AU
Aphelion
1.125 AU
Longitude of ascending node
21.28°
Argument of periapsis
321.91°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 4.9 LD
0.0126 AU
Tisserand (Jupiter)
6.861

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
32
Data arc
2 days
First observed
10 April 2013
Last observed
12 April 2013
Residual RMS
0.28 ″
Solution · Otto Matic
15 April 2021

Visual & observation

Absolute magnitude (H)
25.2

Discovery & classification

Aten Near-Earth Object

Close approaches 177 on record

Flyby geometry
Ecliptic flyby of 2013 GT66 at 2027-01-18 07:15 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-01-18 07:15 UTC close approach of 2013 GT66. Catalogue miss distance 119.3 LD · 4.59 × 10⁷ km. The curve is the geocentric path from 2027-01-15 to 2027-01-21, 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 119.3 LD · 4.59 × 10⁷ km 2027-01-18 07:15 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-01-18 07:15 UTC close approach of 2013 GT66. Catalogue miss distance 119.3 LD · 4.59 × 10⁷ km. The curve is the geocentric path from 2027-01-15 to 2027-01-21, 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
2027-01-18 07:15:00 Earth 0.3065 AU 119.3 LD 14.8 km/s
2027-08-11 15:03:00 Earth 0.4589 AU 178.6 LD 15.7 km/s
2029-03-29 18:05:00 Venus 0.1345 AU 52.4 LD 12.9 km/s
2030-11-12 17:40:00 Earth 0.3308 AU 128.7 LD 12.6 km/s
2031-03-27 10:49:00 Earth 0.1707 AU 66.4 LD 9 km/s
2034-09-17 03:51:00 Earth 0.4369 AU 170.0 LD 17.3 km/s
2035-04-09 14:47:00 Earth 0.2593 AU 100.9 LD 18.2 km/s
2037-11-19 08:46:00 Venus 0.116 AU 45.1 LD 12.7 km/s
2038-01-12 06:50:00 Earth 0.2494 AU 97.1 LD 10 km/s
2038-07-23 14:03:00 Earth 0.4459 AU 173.5 LD 13.3 km/s

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

Sources