Skip to content
Public Universe
Asteroid Near-Earth

2020 FV4

Add to an observing list or journal →

(2020 FV4)

Where is it now

Distance from Sun
1.019 AU
True anomaly
170.92°
Distance from Earth
1.912 AU
As of
15 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 2020 FV4 — 1.019 AU from the Sun 2020 FV4
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2020 FV4 is 1.912 AU from Earth today (15.9 light-minutes).

In the sky

Right ascension
12h 18m 09s
Declination
-00° 48′ 57″
Constellation
Virgo
Distance from Earth
1.91 AU
Elongation from the Sun
18.83° — 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
0.714 AU
Eccentricity
0.4417
Inclination
3.65°
Orbital period
220.2 days
Perihelion
0.398 AU
Aphelion
1.029 AU
Longitude of ascending node
18.84°
Argument of periapsis
335.64°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 3.5 LD
0.009 AU
Tisserand (Jupiter)
7.954

Orbit quality

Orbit poorly determined (uncertainty code 7).

Observations used
64
Data arc
7 days
First observed
24 March 2020
Last observed
31 March 2020
Residual RMS
0.45 ″
Solution · Otto Matic
15 April 2021

Visual & observation

Absolute magnitude (H)
25.39

Discovery & classification

Aten Near-Earth Object

Close approaches 148 on record

Flyby geometry
Ecliptic flyby of 2020 FV4 at 2029-02-20 21:08 UTC Top-down view of the ecliptic, Earth at the centre, for the 2029-02-20 21:08 UTC close approach of 2020 FV4. Catalogue miss distance 27.6 LD · 1.06 × 10⁷ km. The curve is the geocentric path from 2029-02-17 to 2029-02-23, 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 27.6 LD · 1.06 × 10⁷ km 2029-02-20 21:08 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2029-02-20 21:08 UTC close approach of 2020 FV4. Catalogue miss distance 27.6 LD · 1.06 × 10⁷ km. The curve is the geocentric path from 2029-02-17 to 2029-02-23, 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
2029-02-20 21:08:00 Earth 0.071 AU 27.6 LD 10.6 km/s
2032-02-20 18:48:00 Earth 0.1455 AU 56.6 LD 13.5 km/s
2035-02-22 12:01:00 Earth 0.2334 AU 90.8 LD 16.7 km/s
2038-02-25 07:11:00 Earth 0.324 AU 126.1 LD 19.9 km/s
2040-03-25 01:08:00 Earth 0.4948 AU 192.5 LD 26.4 km/s
2040-06-30 08:52:00 Venus 0.1414 AU 55.0 LD 23 km/s
2041-02-07 08:34:00 Venus 0.0589 AU 22.9 LD 18.8 km/s
2041-02-28 15:09:00 Earth 0.4153 AU 161.6 LD 23.2 km/s
2041-09-18 01:05:00 Venus 0.0359 AU 14.0 LD 14.7 km/s
2043-03-29 10:14:00 Earth 0.4037 AU 157.1 LD 23.1 km/s

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

Sources