Asteroids

22 350 TRACKED

An asteroid is a rocky or metallic body left over from the formation of the Solar System, too small to be a planet and without the ice that gives a comet its tail. Most orbit in the main belt between Mars and Jupiter, but a substantial population crosses Earth's orbit and is tracked for that reason. They are the material planets were built from, much of it unaltered for 4.6 billion years, which is what makes them worth visiting.

[

THE FAMOUS ONES

] 12 ENTRIES
[

THE SCIENCE OF ASTEROIDS

] 4 CARDS
The main belt · 14 677 orbits · 1.25.6 AU
MARS3:15:27:32:1JUPITER1.5 AU2 AU2.5 AU3 AU3.5 AU4 AU4.5 AU5 AU5.5 AU
Beyond Neptune · 6053 orbits · 2860 AU
NEPTUNE2:31:230 AU35 AU40 AU45 AU50 AU55 AU60 AU
Looking down on it · 2122 bodies placed · 1 January 2000
JUPITERLEADING · 60°TRAILING · 60°
EVERY CATALOGUED ASTEROID WITH A CLOSED ORBIT, BINNED BY ITS OWN SEMI-MAJOR AXIS · BAR HEIGHTS ARE THE SQUARE ROOT OF THE COUNT, SO THE NEAR-EARTH POPULATION IS VISIBLE BESIDE A BELT HOLDING A HUNDRED TIMES AS MANY · THE DASHED LINES ARE WHERE AN ORBIT WOULD BEAT AGAINST THE PLANET MARKED BESIDE THEM, COMPUTED FROM THAT PLANET’S OWN STORED SEMI-MAJOR AXIS AND NOTHING ELSE · THE 2:1 GAP HOLDS 1 PER CENT OF WHAT THE BUSIEST BIN HOLDS, AND NOBODY PUT IT THERE · THE SPIKE ON JUPITER’S OWN ORBIT IS THE TROJANS, WHICH LEAD AND FOLLOW IT BY SIXTY DEGREES AND ARE NOT IN THE BELT AT ALL · THE STRETCH BETWEEN THE TWO PANELS IS LEFT OUT RATHER THAN COMPRESSED · THE MAP UNDER THEM IS ONE BODY IN 7 OF THE SAME POPULATION, EACH PLACED WHERE ITS OWN ELEMENTS PUT IT AT NOON ON 1 JANUARY 2000, AND IT IS THE FIGURE THAT SHOWS THE TROJANS ARE TWO CLOUDS RATHER THAN A RING · NEITHER FIGURE DOES THE OTHER’S WORK, BECAUSE WHERE A BODY IS AT AN INSTANT IS NOT HOW FAR OUT IT ORBITS

Where they live

The main belt runs from about 2.1 to 3.3 astronomical units, with gaps at the distances where Jupiter's gravity would resonate with the orbit and drive a body out. The Trojans share Jupiter's own orbit, sixty degrees ahead and behind it, where the combined pull of the Sun and Jupiter keeps a body circling in step with the planet. Near-Earth asteroids have been nudged inward and are the ones that get tracked closely. Beyond Neptune the scale is ten times larger and the resonances work the other way: instead of clearing gaps they collect bodies, and Pluto leads the thousands that share its 2:3 rhythm with Neptune.

Why no planet formed there

Jupiter got there first. Its gravity stirs the belt hard enough that collisions between bodies shatter them rather than sticking them together, so accretion stalled. Everything in the belt together would make a body about 3 per cent of the mass of the Moon, and Ceres alone accounts for roughly a third of it.

What the magnitude column is

For an asteroid it is H, the absolute magnitude: how bright the body would look one astronomical unit from both the Sun and the observer, with the Sun directly behind us. Nothing is ever in that position, which is the point — H describes the body rather than where it happens to be in its orbit, so it is comparable between one asteroid and another. It stands in for size, because a diameter has been measured for far fewer of them than a brightness.

What they are made of

Their reflectance spectra sort them into families. C-types are carbon-rich, dark as fresh asphalt and account for most of the belt. S-types are stony and brighter, dominating the inner belt. M-types appear metallic. This is not a chemical assay — it is the light returned from the surface, matched against laboratory samples — but it is why meteorites can be tied back to the classes of body they came from.

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COMMON QUESTIONS

] 8 ANSWERED
How much material is there altogether?
Not much. The whole main belt together comes to about 3 per cent of the mass of the Moon, which is why no planet formed there — and why the crowded asteroid field of films has no counterpart in reality, since the average gap between belt objects runs to millions of kilometres.
What is a near-Earth asteroid?
One whose orbit brings it within 1.3 astronomical units of the Sun, close enough to come near the Earth's own path. Those are the ones surveyed hardest, and the reason continuous asteroid surveys are funded at all.
Have any been visited?
Several. Spacecraft have orbited Eros, Vesta, Ceres and Bennu, brought samples of Itokawa, Ryugu and Bennu back to Earth, and in 2022 deliberately hit the small moon Dimorphos to measure how much its orbit changed.
Who names them?
The discoverer proposes and the IAU decides, but only after the orbit is secure enough for the object to be given a permanent number. Until then it carries a provisional designation recording the year and the half-month it was first seen. A body that turns out not to have come from here is renumbered again, with an I for interstellar — there are three so far, and the first of them was catalogued as an asteroid.
Will an asteroid hit the Earth?
Small ones do constantly and burn up harmlessly. For anything large enough to cause regional damage, surveys have catalogued the great majority of the kilometre-scale near-Earth population and none of them is on a collision course this century. The risk that remains sits with smaller, darker and less complete populations, which is why the surveys continue.
What is the difference between an asteroid, a meteor and a meteorite?
They are three stages of one thing. An asteroid or a smaller meteoroid is the body while it is in space. The meteor is the streak of light when it burns through the atmosphere. A meteorite is what reaches the ground. The great majority never survive the third stage.
How big is the largest asteroid?
Ceres, at about 940 km across, which is large enough to be round under its own gravity and is therefore also classified as a dwarf planet. It holds about a third of the mass of the entire belt on its own. Vesta and Pallas follow at around 500 km, and after that the sizes fall away quickly — most catalogued asteroids are a few kilometres or less.
Could an asteroid be deflected?
It has been done once, as a test. In 2022 a spacecraft was flown into the small moon of a near-Earth asteroid and measurably shortened its orbital period, which showed that a kinetic impact can change an orbit. Doing it for real would need years of warning, which is the reason the tracking effort exists.