2018 WV1

 is a very small asteroid and near-Earth object of the Apollo group that passed within 27000 km of the Earth's surface on 2 December 2018. It was first observed on 29 November 2018 by Hannes Gröller with the Catalina Sky Survey at Catalina Station on Mount Bigelow, Arizona, in the United States.

Orbit
orbits the Sun at a distance of 0.97–1.11 AU once every 389 days (semi-major axis of 1.04 AU). Its orbit has an eccentricity of 0.07 and an inclination of 2° with respect to the ecliptic.

As an Apollo asteroid with an orbital period slightly larger than that of the Earth, its orbit is very similar to that of the Earth, indicating that the object could potentially be a piece of lunar ejecta, a fragment of the Moon that was ejected into space when a larger asteroid hit the Moon a long time ago.

2018 flyby
On 2 December 2018, the asteroid passed about 33000 km from Earth, traveling 5.2 km/s relative to Earth and briefly reaching apparent magnitude 17. This was the third-closest approach by an asteroid in 2018, and the 70th asteroid of the year that passed within 1 lunar distance of Earth. Its absolute magnitude of 30.1 indicates a diameter between 2.5 and 5.6 metres.

remained inside the Earth's sphere of influence from 27 November till 7 December 2018. During the flyby, its orbital period changed from 1.13 to 1.06 years.

At the time of its discovery, had a 2% chance to hit Earth in early December 2018. The possibility of impact was ruled out soon after, as more data became available.

Other flybys
passed within 0.38 AU of Earth in December 2019.

The asteroid, when first discovered, was placed on the Sentry risk table. Further observations refined its orbit enough to remove it from the table on December 3, 2018