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Asteroid Near-Earth

2024 RT5

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(2024 RT5)

Where is it now

Distance from Sun
0.952 AU
True anomaly
133.71°
Distance from Earth
1.233 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 2024 RT5 — 0.952 AU from the Sun 2024 RT5
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2024 RT5 is 1.233 AU from Earth today (10.3 light-minutes).

In the sky

Right ascension
16h 55m 30s
Declination
-26° 35′ 41″
Constellation
Ophiuchus
Distance from Earth
1.23 AU
Elongation from the Sun
49.18° — near the Sun — look low at dusk or dawn

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
0.832 AU
Eccentricity
0.5086
Inclination
14.84°
Orbital period
277.4 days
Perihelion
0.409 AU
Aphelion
1.256 AU
Longitude of ascending node
327.82°
Argument of periapsis
205.72°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 22.3 LD
0.0572 AU
Tisserand (Jupiter)
6.916

Orbit quality

Orbit poorly determined (uncertainty code 7).

Observations used
13
Data arc
2 days
First observed
5 September 2024
Last observed
7 September 2024
Residual RMS
0.76 ″
Solution · Otto Matic
7 September 2024

Visual & observation

Absolute magnitude (H)
23.92

Discovery & classification

Aten Near-Earth Object

Close approaches 28 on record

Flyby geometry
Ecliptic flyby of 2024 RT5 at 2027-08-11 18:40 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-08-11 18:40 UTC close approach of 2024 RT5. Catalogue miss distance 38.7 LD · 1.49 × 10⁷ km. The curve is the geocentric path from 2027-08-08 to 2027-08-14, 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 south of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate. Sun 38.7 LD · 1.49 × 10⁷ km 2027-08-11 18:40 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-08-11 18:40 UTC close approach of 2024 RT5. Catalogue miss distance 38.7 LD · 1.49 × 10⁷ km. The curve is the geocentric path from 2027-08-08 to 2027-08-14, 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 south 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
2027-05-20 14:33:00 Merc 0.0876 AU 34.1 LD 17.2 km/s
2027-05-20 14:33:00 Mercury 0.0876 AU 34.1 LD 17.2 km/s
2027-08-11 18:40:00 Earth 0.0993 AU 38.7 LD 13.4 km/s
2030-08-11 01:32:00 Earth 0.1313 AU 51.1 LD 18.5 km/s
2031-10-18 17:16:00 Earth 0.3978 AU 154.8 LD 24.2 km/s
2033-08-17 18:40:00 Earth 0.3355 AU 130.6 LD 25.2 km/s
2034-10-25 22:55:00 Earth 0.257 AU 100.0 LD 17.1 km/s
2035-11-10 22:44:00 Venus 0.1175 AU 45.7 LD 18.4 km/s
2037-04-04 06:31:00 Merc 0.0866 AU 33.7 LD 17.5 km/s
2037-04-04 06:31:00 Mercury 0.0866 AU 33.7 LD 17.5 km/s

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

Sources