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Asteroid Near-Earth

2017 GT5

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(2017 GT5)

Where is it now

Distance from Sun
1.18 AU
True anomaly
174.41°
Distance from Earth
2.15 AU
As of
22 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 — 0.995 AU from the Sun Earth 2017 GT5 — 1.18 AU from the Sun 2017 GT5
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2017 GT5 is 2.15 AU from Earth today (17.9 light-minutes).

In the sky

Right ascension
14h 30m 24s
Declination
-10° 15′ 19″
Constellation
Libra
Distance from Earth
2.15 AU
Elongation from the Sun
9.44° — too close to the Sun to observe

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
0.962 AU
Eccentricity
0.2289
Inclination
21.7°
Orbital period
344.6 days
Perihelion
0.742 AU
Aphelion
1.182 AU
Longitude of ascending node
205.29°
Argument of periapsis
206.86°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 51.8 LD
0.1331 AU
Tisserand (Jupiter)
6.187

Orbit quality

Orbit very well determined (uncertainty code 1).

Observations used
205
Data arc
468 days
First observed
4 April 2017
Last observed
16 July 2018
Residual RMS
0.45 ″
Solution · Otto Matic
15 April 2021

Visual & observation

Absolute magnitude (H)
21.3

Discovery & classification

Aten Near-Earth Object

Close approaches 148 on record

Flyby geometry
Ecliptic flyby of 2017 GT5 at 2032-04-02 08:00 UTC Top-down view of the ecliptic, Earth at the centre, for the 2032-04-02 08:00 UTC close approach of 2017 GT5. Catalogue miss distance 180.3 LD · 6.93 × 10⁷ km. The curve is the geocentric path from 2032-03-30 to 2032-04-05, 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 south of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate. Sun 180.3 LD · 6.93 × 10⁷ km 2032-04-02 08:00 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2032-04-02 08:00 UTC close approach of 2017 GT5. Catalogue miss distance 180.3 LD · 6.93 × 10⁷ km. The curve is the geocentric path from 2032-03-30 to 2032-04-05, 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 south 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
2032-04-02 08:00:00 Earth 0.4632 AU 180.3 LD 20.7 km/s
2033-04-01 16:39:00 Earth 0.1917 AU 74.6 LD 13.4 km/s
2033-12-04 00:41:00 Earth 0.341 AU 132.7 LD 13.6 km/s
2034-04-18 14:03:00 Earth 0.1775 AU 69.1 LD 11.4 km/s
2034-10-20 05:51:00 Earth 0.2405 AU 93.6 LD 14.8 km/s
2034-10-25 06:16:00 Venus 0.0372 AU 14.5 LD 15.4 km/s
2035-05-17 22:42:00 Earth 0.3402 AU 132.4 LD 11.5 km/s
2035-09-09 06:31:00 Earth 0.2927 AU 113.9 LD 14.6 km/s
2036-07-22 04:14:00 Earth 0.473 AU 184.1 LD 16.5 km/s
2048-12-20 23:28:00 Venus 0.0993 AU 38.6 LD 15.5 km/s

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

Sources