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Near-Earth Object

2025 RQ2

NASA ID: 54545007

Safe

2025 RQ2 will pass Earth on 11 September 2026 at a distance of 17.41 lunar distances (LD) - about 6,690,812 km - travelling at 43,722 km/h. Its estimated diameter is between 13 and 28 metres, roughly the size of a double-decker bus (around 11 m long). NASA does not classify it as potentially hazardous.

Close Approach Date

11 September 2026

In 83 days

Miss Distance

17.41 LD

6,690,812 km

Moon PHA limit

17 times the Moon's distance from Earth

Velocity

43,722 km/h

ISS

1.6 times the orbital speed of the International Space Station

Est. Diameter

13–28 m

Absolute Magnitude

H = 26.62

The brightness measure astronomers use to estimate size

Hazard Classification

Not Hazardous

The real orbit in 3D

The actual path of 2025 RQ2 around the Sun, computed from JPL orbital elements. Drag to rotate, scroll to zoom, and use the time controls to run the orbit forwards or back.

Every recorded pass

Each dot is one close approach of 2025 RQ2 to Earth between 1903 and 2042, from JPL's records. Lower means closer: a dot under the dashed line passed nearer than the Moon. The orange dot is the approach on this page.

1900 1920 1940 1960 1980 2000 2020 2040 1 LDMoon's orbit 10 LD today 13 Sept 1903 - 4.33 LD15 Sept 2022 - 35.8 LD14 Sept 2023 - 18.22 LD12 Sept 2024 - 3.07 LD12 Sept 2025 - 1.49 LD11 Sept 2026 - 17.41 LD (this approach)11 Sept 2027 - 35.89 LD7 Mar 2041 - 36.32 LD4 Mar 2042 - 32.94 LD Close approach date Miss distance (LD, log scale)

Size Comparison

Asteroid 13–28 m Double-decker bus 11 m long

Reading the Numbers

  • A lunar distance (LD) is the average gap between Earth and the Moon, about 384,400 km. It is the standard yardstick for close approaches. Read more →
  • Diameter estimates come from brightness. A dark surface reflects less light than a bright one, so the true size can sit anywhere in the quoted range. Read more →
  • Potentially hazardous is a watch-list label based on size and orbital proximity. It does not mean an impact is expected. Read more →

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