Thanks to two aggressive search programs, the count of near-Earth asteroids has soared past the 15,000-object milestone.

On August 13, 1898, Carl Gustav Witt discovered a medium-size asteroid that circled the Sun much closer than its siblings did. In fact, what came to be called 433 Eros actually crosses the orbit of Mars during its 1.8-year solar circuit, and it can come as close to the Sun as 1.13 astronomical units (170 million kilometers).

Near-Earth asteroids as of November 2016
A plot of all known near-Earth asteroids (NEAs, shown in red) looks scary, but the risk of collision is actually quite low. Main-belt asteroids are shown in green.
Minor Planet Center

From that modest beginning, the hunt for near-Earth asteroids (NEAs) — those that venture within 1.3 a.u. of the Sun — has evolved from sporadic, inadvertent pickups to dedicated searches that net hundreds of new objects every month.

A week ago, the International Astronomical Union's Minor Planet Center (just a few blocks from Sky & Telescope's offices) announced the discovery of asteroid 2016 TB57. With that find, the MPC's catalog of all known NEAs reached a new threshold: 15,000.

Orbit of near-Earth asteroid 2016 TB<sub>57</sub>
The 15,000th cataloged near-Earth asteroid is a small space rock designated 2016 TB57. It skirted near Earth on October 31, 2016, 18 days after its discovery.

Much like the steady climb of the stock market with time, there's no particular significance to a count of 15,000 (it's already zoomed to 15,197 as I write this) or to 2016 TB57. Observers participating in the NASA-funded Catalina Sky Survey discovered it on October 13th as it neared Earth. Rather small, roughly 15 to 35 m across, it passed by at a very safe distance of 2,010,000 km (more than five times the Moon's distance) on October 31st.

Most NEAs are found, as their name implies, someplace near Earth. Generally they're too small to be spotted far away, and it's only within the week or so when they skim near our planet that they make their existence know. These days almost all NEAs are swept up by the Catalina survey or by Pan-STARRS 1, a wide-field telescope on Haleakala in Hawai'i. (That name is a contraction of Panoramic Survey Telescope & Rapid Response System.)

Dynamicists break down NEAs into four types, each named for an archetype asteroid in that class. Amors (like Eros) cross the orbit of Mars but come no closer than 1.017 a.u. to the Sun (Earth's aphelion distance). Apollos have semimajor axes (their mean heliocentric distance) greater than 1.0 a.u. but still cross Earth's orbit at their closest. Atens have semimajor axes of less than 1 a.u. but likewise cross Earth's orbit (our planet's perihelion distance is 0.983 a.u.). At its most recent count, the MPC had tallied 6,537 Amors, 7,449 Apollos, and 1,120 Atens.

Rate of NEA discoveries
The pace of discovery for near-Earth asteroids has increased rapidly in recent year. Most of the recent ones are small.

Apohele asteroids (sometimes called Atiras) are the newest and smallest group — only a dozen or so have been confirmed — and their entire orbits lie entirely inside of Earth's.

Even with all those space rocks flying around, there’s very little risk that a known, sizable asteroid will strike Earth for the foreseeable future. According to NASA's Near-Earth Object Program and its European Space Agency counterpart, the object with the highest cumulative probability of impact (that is, the risk over dozens of close approaches) is 2010 RF12, which has a 1-in-15 chance of hitting in 2095 — but it’s only about 7 m (23 feet) across, almost certainly too small to make it to the ground.

Eros seen close-up
NASA's NEAR-Shoemaker spacecraft recorded this view of its final destination, asteroid 433 Eros, on February 12, 2000.

Meanwhile, 433 Eros has hardly been relegated to the back shelf of asteroid discoveries. A highly elongated body about 34 km long, Eros played host to NASA's NEAR-Shoemaker spacecraft, which orbited it for a year in 2000–01. Then, on February 12, 2001,  the spacecraft made a dramatic — but mission-ending — landing on Eros' surface


Image of Edward Schaefer

Edward Schaefer

November 4, 2016 at 10:30 am

The paragraph about collision danger seems a little garbled to me. No object has a probability of collision *lower* that 1 in 1000? I would think that "higher" would be the right word. Also, what is the "dubious honor" that 2011 AM37 has? I would assume the highest probability of collision, but even in that case what is the probability?

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Image of J. Kelly Beatty

J. Kelly Beatty

November 4, 2016 at 1:05 pm

hi, Edward, and thanks for that head's up. (That's what I get for writing at 6 a.m.!) I think you'll find that section clearer now.

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Image of George Sonnier

George Sonnier

November 5, 2016 at 12:57 pm

Looks like Earth may not have cleared its neighborhood of most other orbiting objects.

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