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Asteroids

Asteroids are the rocky and metallic leftovers from the building of the planets, and almost every meteorite is a piece of one. Here are 40 of the most interesting, the ones passing Earth this year, and how astronomers keep track of them all.

Where meteorites come from

Most asteroids orbit the Sun in the main belt, between Mars and Jupiter. More than a million larger than a kilometre are thought to exist there, yet together they would make a body far smaller than our Moon. When asteroids collide, fragments are knocked off. Over millions of years, the gentle push of sunlight and the pull of Jupiter steer some of those fragments onto orbits that cross Earth's, and a few eventually fall as meteorites. Comparing meteorites with the colours of asteroids, and with samples brought back by spacecraft, links the rocks in our collections to their sources: the howardites to Vesta, the LL chondrites to bodies like Itokawa, and the most primitive carbon-rich meteorites to asteroids like Ryugu and Bennu.

Notable asteroids

Giants of the main belt

The largest bodies between Mars and Jupiter, from the dwarf planet Ceres to the metal-rich Psyche.

About 940 km across

Ceres

Dwarf planet in the main belt

Dawn (in orbit 2015–2018)
About 510 km across

Pallas

Large main-belt asteroid

Not yet visited
About 250 km across

Juno

Large main-belt asteroid

Not yet visited
About 525 km across

Vesta

Large main-belt asteroid

Dawn (in orbit 2011–2012)
About 430 km across

Hygiea

Large main-belt asteroid

Not yet visited
About 220 km across (on average)

Psyche

Metal-rich main-belt asteroid

Psyche spacecraft, due to arrive in 2029
About 270 km long

Kleopatra

Main-belt asteroid with two moons

Not yet visited

Visited on the way

Main-belt asteroids photographed by spacecraft flying past on their way to other targets.

About 18 km long

Gaspra

Main-belt asteroid

Galileo fly-by, 1991
About 60 km long

Ida

Main-belt asteroid with a moon

Galileo fly-by, 1993
About 53 km across (on average)

Mathilde

Dark main-belt asteroid

NEAR Shoemaker fly-by, 1997
About 6 km long

Annefrank

Main-belt asteroid

Stardust fly-by, 2002
About 5 km across

Šteins

Rare E-type main-belt asteroid

Rosetta fly-by, 2008
About 100 km across

Lutetia

Large main-belt asteroid

Rosetta fly-by, 2010
About 790 m across

Dinkinesh

Small main-belt asteroid with a moon

Lucy fly-by, 2023
About 8 km long

Donaldjohanson

Main-belt asteroid

Lucy fly-by, 2025

Jupiter's Trojans

Ancient bodies that share Jupiter's orbit, leading and trailing the giant planet.

About 64 km across

Eurybates

Jupiter Trojan with a moon

Lucy fly-by planned for 2027
About 110 km across (each of the two)

Patroclus

Double Jupiter Trojan

Lucy fly-by planned for 2033

Near-Earth pioneers

The first near-Earth asteroids found, the ones that named the orbit groups, and others that taught us how these bodies behave.

About 34 km long

Eros

Near-Earth asteroid (Amor group)

NEAR Shoemaker (in orbit 2000–2001, landed 2001)
About 35 km across

Ganymed

Largest near-Earth asteroid (Amor group)

Not yet visited
About 1 km across

Amor

Near-Earth asteroid (namesake of the Amor group)

Not yet visited
About 1.5 km across

Apollo

Near-Earth asteroid (namesake of the Apollo group)

Not yet visited
About 1 km across

Aten

Near-Earth asteroid (namesake of the Aten group)

Not yet visited
About 1.3 km across

Icarus

Near-Earth asteroid (Apollo group)

Not yet visited
About 4.5 km across

Florence

Near-Earth asteroid with two moons (Amor group)

Not yet visited
About 4.5 km long

Toutatis

Near-Earth asteroid (Apollo group)

Chang'e 2 fly-by, 2012
About 530 m across

Golevka

Near-Earth asteroid (Apollo group)

Not yet visited
About 5–6 km across

Phaethon

Near-Earth asteroid (Apollo group), parent of the Geminids

DESTINY+ fly-by planned

Sample return and mission targets

Small asteroids that spacecraft have touched, sampled or struck, and the next ones in line.

About 535 m long

Itokawa

Near-Earth asteroid (Apollo group)

Hayabusa (2005); samples returned 2010
About 900 m across

Ryugu

Near-Earth asteroid (Apollo group)

Hayabusa2 (2018–2019); samples returned 2020
About 490 m across

Bennu

Near-Earth asteroid (Apollo group)

OSIRIS-REx (2018–2021); samples returned 2023
About 780 m (Didymos) and 150 m (Dimorphos)

Didymos and Dimorphos

Double near-Earth asteroid (Apollo group)

DART impact, 2022; Hera due late 2026
Roughly 40–100 m across

Kamoʻoalewa

Near-Earth asteroid and quasi-satellite of Earth

Tianwen-2 (arrived 2026)
About 11 m across

1998 KY26

Small near-Earth asteroid (Apollo group)

Hayabusa2 arrival planned for 2031

Close passes and careful tracking

Asteroids whose paths have been followed closely, and what that tracking showed.

About 340 m across

Apophis

Near-Earth asteroid (Aten group)

OSIRIS-APEX due to arrive in 2029
About 1.3 km across

1950 DA

Near-Earth asteroid (Apollo group)

Not yet visited
About 30–40 m across

Duende (2012 DA14)

Small near-Earth asteroid (now in the Aten group)

Not yet visited
About 60 m across

2024 YR4

Small near-Earth asteroid (Apollo group)

Not yet visited

Found before they fell

Small asteroids spotted in space hours before they reached the ground as meteorites.

About 4 m across

2008 TC3

Small asteroid that struck Earth on 7 October 2008

Fell over Sudan; meteorites recovered
Under 2 m across

2018 LA

Small asteroid that struck Earth on 2 June 2018

Fell over Botswana; meteorites recovered
About 1 m across

2023 CX1

Small asteroid that struck Earth on 13 February 2023

Fell over Normandy, France; meteorites recovered

Passing Earth soon

The next known asteroids to pass within 19 Moon distances. All are predicted misses.

All close approaches

Keeping watch

Survey telescopes scan the sky every clear night, and their measurements are combined to work out each new asteroid's orbit, years and centuries ahead. More than 90 per cent of near-Earth asteroids larger than a kilometre have been found, and none of them is on course to hit Earth in the foreseeable future. The search now concentrates on smaller ones.

When an asteroid has just been discovered, its orbit is uncertain, so a computer works out a whole range of possible future paths. If Earth falls anywhere inside that range, the asteroid goes on a watch list with a calculated chance of impact. These chances are almost always tiny, and as more observations come in, the range narrows and the asteroid is usually removed from the list altogether. 2024 YR4 and Apophis both followed exactly that path.

The watch list currently holds 2,227 objects. About 95 per cent of them are smaller than 50 metres, the size that would break up high in the atmosphere. None is rated above zero on the Torino scale, which runs from 0 (no hazard) to 10.

The largest objects on the list, with the chance that they miss Earth on every listed date:

AsteroidSizeYears studiedChance of missing
29075 (1950 DA)about 1.3 km2880-288099.97%
2010 ER12about 1 km2026-2094more than 99.99%
2026 GN18about 730 m2054-2118more than 99.99%
1979 XBabout 660 m2056-2113more than 99.99%
101955 Bennu (1999 RQ36)about 490 m2178-229099.94%
2010 MY112about 370 m2027-2122more than 99.99%
2014 HN197about 350 m2069-2118more than 99.99%
2007 FT3about 340 m2030-2119more than 99.99%

From open tracking data. Most entries have been seen only briefly, and further observations normally rule out every impact. Figures last updated 1 Nov 2026.

If a sizeable asteroid were ever found on a collision course, it would most likely be spotted years or decades ahead. In 2022 the DART mission showed that a spacecraft can change an asteroid's path, so a warning like that would give time to act.

Words to know