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Asteroid Near-Earth

2019 GK1

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(2019 GK1)

Where is it now

Distance from Sun
1.006 AU
True anomaly
215.05°
Distance from Earth
1.967 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 2019 GK1 — 1.006 AU from the Sun 2019 GK1
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2019 GK1 is 1.967 AU from Earth today (16.4 light-minutes).

In the sky

Right ascension
14h 19m 28s
Declination
-16° 26′ 30″
Constellation
Virgo
Distance from Earth
1.97 AU
Elongation from the Sun
10.67° — 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
0.88 AU
Eccentricity
0.1921
Inclination
8.74°
Orbital period
301.6 days
Perihelion
0.711 AU
Aphelion
1.049 AU
Longitude of ascending node
16.3°
Argument of periapsis
357.07°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 18.2 LD
0.0468 AU
Tisserand (Jupiter)
6.71

Orbit quality

Orbit poorly determined (uncertainty code 7).

Observations used
26
Data arc
11 days
First observed
3 April 2019
Last observed
14 April 2019
Residual RMS
0.31 ″
Solution · Otto Matic
15 April 2021

Visual & observation

Absolute magnitude (H)
26.4

Discovery & classification

Aten Near-Earth Object

Close approaches 30 on record

Flyby geometry
Ecliptic flyby of 2019 GK1 at 2028-03-02 05:48 UTC Top-down view of the ecliptic, Earth at the centre, for the 2028-03-02 05:48 UTC close approach of 2019 GK1. Catalogue miss distance 159.7 LD · 6.14 × 10⁷ km. The curve is the geocentric path from 2028-02-28 to 2028-03-05, 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 north of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate. Sun 159.7 LD · 6.14 × 10⁷ km 2028-03-02 05:48 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2028-03-02 05:48 UTC close approach of 2019 GK1. Catalogue miss distance 159.7 LD · 6.14 × 10⁷ km. The curve is the geocentric path from 2028-02-28 to 2028-03-05, 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 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
2028-03-02 05:48:00 Earth 0.4103 AU 159.7 LD 16.9 km/s
2028-09-25 08:15:00 Earth 0.2913 AU 113.4 LD 10.1 km/s
2029-04-27 07:02:00 Earth 0.4534 AU 176.4 LD 18.5 km/s
2033-02-27 08:08:00 Earth 0.1551 AU 60.4 LD 8.2 km/s
2033-08-11 03:32:00 Earth 0.2749 AU 107.0 LD 7.6 km/s
2037-10-09 19:38:00 Venus 0.1329 AU 51.7 LD 11.2 km/s
2038-04-16 18:52:00 Earth 0.0484 AU 18.8 LD 5.8 km/s
2040-04-05 05:13:00 Venus 0.0375 AU 14.6 LD 7.2 km/s
2042-10-03 08:08:00 Venus 0.0224 AU 8.7 LD 6 km/s
2042-10-19 02:04:00 Earth 0.2841 AU 110.6 LD 10 km/s

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

Sources