Skip to content
Public Universe
Asteroid Near-Earth

2019 ED

Add to an observing list or journal →

(2019 ED)

Where is it now

Distance from Sun
1 AU
True anomaly
189.01°
Distance from Earth
1.942 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 ED — 1 AU from the Sun 2019 ED
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2019 ED is 1.942 AU from Earth today (16.2 light-minutes).

In the sky

Right ascension
12h 54m 19s
Declination
-05° 21′ 27″
Constellation
Virgo
Distance from Earth
1.94 AU
Elongation from the Sun
13.32° — 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
0.891 AU
Eccentricity
0.1241
Inclination
1.15°
Orbital period
307.3 days
Perihelion
0.781 AU
Aphelion
1.002 AU
Longitude of ascending node
136.1°
Argument of periapsis
215.72°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 1.2 LD
0.0031 AU
Tisserand (Jupiter)
6.66

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
74
Data arc
33 days
First observed
1 March 2019
Last observed
3 April 2019
Residual RMS
0.4 ″
Solution · Otto Matic
15 April 2021

Visual & observation

Absolute magnitude (H)
26.9

Discovery & classification

Listed by JPL impact monitoring; see the Sentry table for current probabilities.

Aten Near-Earth Object

Close approaches 27 on record

Flyby geometry
Ecliptic flyby of 2019 ED at 2029-10-02 19:45 UTC Top-down view of the ecliptic, Earth at the centre, for the 2029-10-02 19:45 UTC close approach of 2019 ED. Catalogue miss distance 84.6 LD · 3.25 × 10⁷ km. The curve is the geocentric path from 2029-09-29 to 2029-10-05, 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. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate. Sun 84.6 LD · 3.25 × 10⁷ km 2029-10-02 19:45 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2029-10-02 19:45 UTC close approach of 2019 ED. Catalogue miss distance 84.6 LD · 3.25 × 10⁷ km. The curve is the geocentric path from 2029-09-29 to 2029-10-05, 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. 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
2029-10-02 19:45:00 Earth 0.2173 AU 84.6 LD 5.8 km/s
2030-04-05 04:00:00 Earth 0.307 AU 119.5 LD 12.2 km/s
2034-08-13 19:08:00 Venus 0.1445 AU 56.2 LD 2.7 km/s
2035-04-04 15:04:00 Earth 0.0274 AU 10.7 LD 3.2 km/s
2040-02-05 00:45:00 Earth 0.0388 AU 15.1 LD 3.7 km/s
2045-02-08 03:09:00 Earth 0.2933 AU 114.1 LD 11.8 km/s
2051-04-05 11:23:00 Earth 0.3381 AU 131.6 LD 13.2 km/s
2056-04-10 06:06:00 Earth 0.0848 AU 33.0 LD 5.2 km/s
2061-02-04 02:59:00 Earth 0.0522 AU 20.3 LD 4.2 km/s

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

Sources