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Asteroid Near-Earth

2014 CE13

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(2014 CE13)

Where is it now

Distance from Sun
0.642 AU
True anomaly
259.19°
Distance from Earth
1.614 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 2014 CE13 — 0.642 AU from the Sun 2014 CE13
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2014 CE13 is 1.614 AU from Earth today (13.4 light-minutes).

In the sky

Right ascension
13h 10m 01s
Declination
-08° 42′ 02″
Constellation
Virgo
Distance from Earth
1.61 AU
Elongation from the Sun
7.57° — 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
0.851 AU
Eccentricity
0.5716
Inclination
5.47°
Orbital period
286.9 days
Perihelion
0.365 AU
Aphelion
1.338 AU
Longitude of ascending node
334.75°
Argument of periapsis
312.75°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 2.9 LD
0.0074 AU
Tisserand (Jupiter)
6.773

Orbit quality

Orbit very well determined (uncertainty code 1).

Observations used
76
Data arc
11.03 years
First observed
10 February 2014
Last observed
19 February 2025
Residual RMS
0.62 ″
Solution · Otto Matic
20 February 2025

Visual & observation

Absolute magnitude (H)
24.09

Discovery & classification

Aten Near-Earth Object

Close approaches 274 on record

Flyby geometry
Ecliptic flyby of 2014 CE13 at 2034-11-26 13:36 UTC Top-down view of the ecliptic, Earth at the centre, for the 2034-11-26 13:36 UTC close approach of 2014 CE13. Catalogue miss distance 48.4 LD · 1.86 × 10⁷ km. The curve is the geocentric path from 2034-11-23 to 2034-11-29, 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 48.4 LD · 1.86 × 10⁷ km 2034-11-26 13:36 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2034-11-26 13:36 UTC close approach of 2014 CE13. Catalogue miss distance 48.4 LD · 1.86 × 10⁷ km. The curve is the geocentric path from 2034-11-23 to 2034-11-29, 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
2028-06-06 21:03:00 Mercury 0.0903 AU 35.1 LD 22.7 km/s
2028-06-06 21:03:00 Merc 0.0903 AU 35.1 LD 22.7 km/s
2031-08-05 00:22:00 Mercury 0.0816 AU 31.8 LD 22.6 km/s
2031-08-05 00:22:00 Merc 0.0816 AU 31.8 LD 22.6 km/s
2034-09-30 19:44:00 Merc 0.0428 AU 16.7 LD 26.8 km/s
2034-09-30 19:44:00 Mercury 0.0428 AU 16.7 LD 26.8 km/s
2034-10-27 20:52:00 Venus 0.0891 AU 34.7 LD 21 km/s
2034-11-26 13:36:00 Earth 0.1242 AU 48.4 LD 14.9 km/s
2036-02-19 18:26:00 Moon 0.0073 AU 2.8 LD 16.6 km/s
2036-02-19 20:17:00 Earth 0.0073 AU 2.8 LD 17.5 km/s

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

Sources