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Near-Earth Object

2026 FX1

NASA ID: 54606517

Safe

2026 FX1 will pass Earth on 15 March 2027 at a distance of 62.12 lunar distances (LD) - about 23,879,098 km - travelling at 55,735 km/h. Its estimated diameter is between 12 and 27 metres, roughly the size of a double-decker bus (around 11 m long). NASA does not classify it as potentially hazardous.

Close Approach Date

15 March 2027

In 268 days

Miss Distance

62.12 LD

23,879,098 km

Moon PHA limit

62 times the Moon's distance from Earth

Velocity

55,735 km/h

ISS

2.0 times the orbital speed of the International Space Station

Est. Diameter

12–27 m

Absolute Magnitude

H = 26.73

The brightness measure astronomers use to estimate size

Hazard Classification

Not Hazardous

The real orbit in 3D

The actual path of 2026 FX1 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 2026 FX1 to Earth between 1961 and 2095, 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.

1960 1980 2000 2020 2040 2060 2080 2100 1 LDMoon's orbit 10 LD today 18 Mar 1961 - 4.89 LD16 Sept 1992 - 38.67 LD19 Mar 1993 - 19.41 LD23 Sept 2024 - 28.84 LD18 Mar 2026 - 5.89 LD18 Sept 2059 - 28.7 LD19 Mar 2060 - 34.74 LD16 Mar 2061 - 31.01 LD20 Sept 2093 - 21.11 LD17 Mar 2095 - 16.55 LD Close approach date Miss distance (LD, log scale)

Size Comparison

Asteroid 12–27 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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