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Asteroid Near-Earth

2014 QZ295

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(2014 QZ295)

Where is it now

Distance from Sun
1.023 AU
True anomaly
239.05°
Distance from Earth
0.7 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 2014 QZ295 — 1.023 AU from the Sun 2014 QZ295
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2014 QZ295 is 0.7 AU from Earth today (5.8 light-minutes).

In the sky

Right ascension
18h 50m 27s
Declination
-23° 46′ 06″
Constellation
Sagittarius
Distance from Earth
0.7 AU
Elongation from the Sun
71.65° — well clear of the Sun

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
0.954 AU
Eccentricity
0.3363
Inclination
1.34°
Orbital period
340.4 days
Perihelion
0.633 AU
Aphelion
1.275 AU
Longitude of ascending node
144.17°
Argument of periapsis
325.6°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 4.2 LD
0.0108 AU
Tisserand (Jupiter)
6.26

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
25
Data arc
17 days
First observed
20 August 2014
Last observed
6 September 2014
Residual RMS
0.44 ″
Solution · Otto Matic
15 April 2021

Visual & observation

Absolute magnitude (H)
24.8

Discovery & classification

Aten Near-Earth Object

Close approaches 114 on record

Flyby geometry
Ecliptic flyby of 2014 QZ295 at 2027-01-07 05:02 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-01-07 05:02 UTC close approach of 2014 QZ295. Catalogue miss distance 136.2 LD · 5.24 × 10⁷ km. The curve is the geocentric path from 2027-01-04 to 2027-01-10, 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 136.2 LD · 5.24 × 10⁷ km 2027-01-07 05:02 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-01-07 05:02 UTC close approach of 2014 QZ295. Catalogue miss distance 136.2 LD · 5.24 × 10⁷ km. The curve is the geocentric path from 2027-01-04 to 2027-01-10, 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
2027-01-07 05:02:00 Earth 0.35 AU 136.2 LD 13 km/s
2027-08-15 09:08:00 Earth 0.2088 AU 81.2 LD 7 km/s
2027-11-04 20:58:00 Earth 0.2556 AU 99.5 LD 7.1 km/s
2028-09-09 11:19:00 Earth 0.154 AU 59.9 LD 14.1 km/s
2038-05-24 01:05:00 Earth 0.3833 AU 149.2 LD 21 km/s
2039-05-09 11:03:00 Earth 0.0351 AU 13.7 LD 8.7 km/s
2040-02-15 09:25:00 Earth 0.323 AU 125.7 LD 11.2 km/s
2040-07-05 11:30:00 Earth 0.2561 AU 99.7 LD 7.8 km/s
2040-12-21 00:15:00 Earth 0.341 AU 132.7 LD 12.4 km/s
2041-09-07 18:25:00 Earth 0.1234 AU 48.0 LD 6.5 km/s

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

Sources