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Asteroid Near-Earth

2016 RG17

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(2016 RG17)

Where is it now

Distance from Sun
0.597 AU
True anomaly
98.24°
Distance from Earth
1.108 AU
As of
16 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 — 0.997 AU from the Sun Earth 2016 RG17 — 0.597 AU from the Sun 2016 RG17
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2016 RG17 is 1.108 AU from Earth today (9.2 light-minutes).

In the sky

Right ascension
15h 43m 17s
Declination
-10° 16′ 44″
Constellation
Libra
Distance from Earth
1.1 AU
Elongation from the Sun
33.03° — 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
0.812 AU
Eccentricity
0.5693
Inclination
21.98°
Orbital period
267 days
Perihelion
0.349 AU
Aphelion
1.274 AU
Longitude of ascending node
170.09°
Argument of periapsis
29.15°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 16.9 LD
0.0435 AU
Tisserand (Jupiter)
7.014

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
60
Data arc
32 days
First observed
4 September 2016
Last observed
6 October 2016
Residual RMS
0.39 ″
Solution · Otto Matic
15 April 2021

Visual & observation

Absolute magnitude (H)
23

Discovery & classification

Aten Near-Earth Object

Close approaches 213 on record

Flyby geometry
Ecliptic flyby of 2016 RG17 at 2027-09-16 22:38 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-09-16 22:38 UTC close approach of 2016 RG17. Catalogue miss distance 90.7 LD · 3.48 × 10⁷ km. The curve is the geocentric path from 2027-09-13 to 2027-09-19, 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 90.7 LD · 3.48 × 10⁷ km 2027-09-16 22:38 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-09-16 22:38 UTC close approach of 2016 RG17. Catalogue miss distance 90.7 LD · 3.48 × 10⁷ km. The curve is the geocentric path from 2027-09-13 to 2027-09-19, 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
2027-09-16 22:38:00 Earth 0.2329 AU 90.7 LD 14.8 km/s
2030-10-19 17:46:00 Earth 0.3663 AU 142.6 LD 14.6 km/s
2031-01-11 19:31:00 Earth 0.4957 AU 192.9 LD 16.6 km/s
2032-09-17 12:20:00 Earth 0.3594 AU 139.9 LD 29.1 km/s
2033-11-15 16:14:00 Earth 0.364 AU 141.7 LD 19.5 km/s
2035-09-08 02:14:00 Earth 0.0666 AU 25.9 LD 17.3 km/s
2038-10-01 05:22:00 Earth 0.326 AU 126.9 LD 14.8 km/s
2041-11-08 04:07:00 Earth 0.3548 AU 138.1 LD 14.5 km/s
2043-07-10 15:09:00 Mercury 0.0533 AU 20.7 LD 37.1 km/s
2043-07-10 15:09:00 Merc 0.0533 AU 20.7 LD 37.1 km/s

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

Sources