Skip to content
Public Universe
Asteroid Near-Earth

2016 CE

Add to an observing list or journal →

(2016 CE)

Where is it now

Distance from Sun
1.02 AU
True anomaly
145.14°
Distance from Earth
0.547 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 2016 CE — 1.02 AU from the Sun 2016 CE
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2016 CE is 0.547 AU from Earth today (4.5 light-minutes).

In the sky

Right ascension
09h 03m 27s
Declination
+27° 52′ 17″
Constellation
Cancer
Distance from Earth
0.55 AU
Elongation from the Sun
76.97° — well clear of the Sun

Favours the northern hemisphere; low or below the horizon from far south.

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
0.2855
Inclination
5.77°
Orbital period
286.4 days
Perihelion
0.608 AU
Aphelion
1.093 AU
Longitude of ascending node
315.65°
Argument of periapsis
316.5°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 0.1 LD
0.0003 AU
Tisserand (Jupiter)
6.89

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
57
Data arc
2 days
First observed
3 February 2016
Last observed
5 February 2016
Residual RMS
0.52 ″
Solution · Otto Matic
28 July 2026

Visual & observation

Absolute magnitude (H)
28.5

Discovery & classification

Aten Near-Earth Object

Close approaches 44 on record

Flyby geometry
Ecliptic flyby of 2016 CE at 2027-02-04 21:29 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-02-04 21:29 UTC close approach of 2016 CE. Catalogue miss distance 49.3 LD · 1.9 × 10⁷ km. The curve is the geocentric path from 2027-02-01 to 2027-02-07, 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 inset is a heliocentric view and is approximate. Sun 49.3 LD · 1.9 × 10⁷ km 2027-02-04 21:29 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-02-04 21:29 UTC close approach of 2016 CE. Catalogue miss distance 49.3 LD · 1.9 × 10⁷ km. The curve is the geocentric path from 2027-02-01 to 2027-02-07, 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 inset is a heliocentric view and is approximate.

JPL Horizons

When (UTC) Body Distance Lunar distances Relative speed
2027-02-04 21:29:00 Earth 0.1267 AU 49.3 LD 12.1 km/s
2029-08-13 09:54:00 Venus 0.1206 AU 46.9 LD 8.4 km/s
2032-11-23 03:49:00 Venus 0.12 AU 46.7 LD 14.1 km/s
2033-12-29 00:07:00 Earth 0.1292 AU 50.3 LD 6.5 km/s
2038-04-14 08:00:00 Venus 0.1269 AU 49.4 LD 9.8 km/s
2040-11-11 11:42:00 Earth 0.1655 AU 64.4 LD 12 km/s
2045-01-26 04:49:00 Earth 0.0739 AU 28.7 LD 6.6 km/s
2046-12-14 11:43:00 Venus 0.1091 AU 42.5 LD 9.6 km/s
2051-11-11 04:11:00 Earth 0.1043 AU 40.6 LD 8.8 km/s
2052-04-25 00:47:00 Venus 0.1067 AU 41.5 LD 11.2 km/s

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

Sources