Asteroid 2012 TC4 To Zip Past Earth This Week

Asteroid 2012 TC4 To Zip Past Earth This Week


The close pass of near-Earth asteroid 2012 TC4 this week will give NASA a chance to test planetary defense coordination.

2012 TC4

A simulation of asteroid 2012 TC4 passing by Earth.

A small space rock designated 2012 TC4 will pass 31,180 miles (50,180 kilometers from the Earth over the southern Pacific Ocean on Thursday, October 12, 2017 at 1:42 a.m. EDT / 5:42 Universal Time (UT). Moving at 7.6 kilometers per second relative to the Earth at closest approach, this house-sized rock is about 13 meters in diameter, a little smaller than the 20-meter meteor which exploded over Chelyabinsk, Russia on February 15, 2013.

This asteroid has a unique history. Discovered by the PanSTARRS 1 telescope on Maui's Haleakala, 2012 TC4 on to pass 58,900 miles (94,800 km) from Earth on October 12, 2012, eight days after its discovery. There was increased interest in the Earth-crossing asteroid when it was realized that it could pass as close as 11,200 miles (18,000 km) from us — just under three Earth radii — this week.

2012 TC4 observed

Near-Earth asteroid 2012 TC4 appears as a dot (center) in this composite of 37 individual 50-second exposures obtained with the FORS2 instrument on ESO’s Very Large Telescope.

More observations often make for a better refinement for an asteroid's orbit, and 2012 TC4 was recovered by the European Southern Observatory's Very Large Telescope earlier this year on July 27th, at the extraordinarily faint magnitude 27. The asteroid was 0.4 astronomical unit (37 million miles or 60 million km) at the time of recovery, and this week's close pass marks the first documented return of an asteroid passing us closer than the Earth-Moon distance twice.

For perspective, the 31,180-mile pass on Thursday is roughly 13% of the Earth-Moon distance and not quite 50% farther than the ring of geosynchronous satellites around the Earth.

The pass is close enough that Earth's gravity will modify the orbit of 2012 TC4, which goes around the Sun once every 609 days. It's also a fairly fast tumbler, and observers know from analyzing its light curve that it spins once every 12.2 minutes. This is typical for small space rocks, but the rapidity record goes to 2014 RC, which spins at a dizzying once every 16 seconds.

Usually, we only see smaller asteroids such as 2012 TC4 shortly before closest approach. Some, like the Chelyabinsk meteor, approach Earth from our blind spot sunward (remember, we were all watching the Valentine's Day passage of asteroid 2012 DA14 just the night before) and strike with no warning at all.

2012 TC4 flyby

An animation showing the passage of 2012 TC4 past Earth (blue), versus the ring of geostationary satellites (purple) and the Moon (white).
Tony873004/Wikimedia Commons

2012 TC4 will also pass 172,000 miles (277,000 km) from the Moon just under 14 hours after its closest approach to Earth. A NASA bulletin from the ongoing 2012 TC4 Observing Campaign out last month states that a “new orbit solution precludes a possible impact in 2050.” The next future close pass for 2012 TC4 is on December 1, 2079, at about 1 million km distant. Of course, expect refinements in the orbit of 2012 TC4 made from observations during this week's pass to narrow down these future parameters a bit more.

“Scientists have always appreciated knowing when an asteroid will make a close approach to and safely pass the Earth because they can make preparations to collect data to characterize and learn as much as possible about it,” says Michael Kelley (NASA Headquarters) in a recent press release. “This time we are adding another layer of effort, using this asteroid flyby to test the worldwide asteroid detection and tracking network.”

NASA researchers will ping 2012 TC4 with radar from the Goldstone tracking station this week. Arecibo Observatory, recently battered by Hurricane Maria, will also ping asteroid 2012 TC4 on October 12th.

Observing Prospects

Even at its closest approach, 2012 TC4 will shine at only magnitude 12 to 13, meaning you'll need a telescope with at least an 8-inch aperture and dark skies to see it. The Moon also reaches last quarter phase on October 12th, and the best viewing prospects for North America come the evening prior on October 11th, as 2012 TC4 glides southward through the constellations Capricornus, Microscopium and Sagittarius. But at 10:00 PM EDT (2:00 UT on the 12) 2012 TC4 will still be 137,000 km distant, shining at around 15th magnitude. South American observers get the very best view, as 2012 TC4 heads sunward in the predawn hours of October 12th.

At its closest approach, 2012 TC4 will move across the sky at a whopping 1° every 4 minutes, fast enough to see it move in real time at the eyepiece. Such a close pass will also show a large amount of parallax shift, about 15° from pole-to-pole. Although planetarium programs take this into account, they usually don't incorporate the deflection of such a close pass due to Earth's gravity. Your best bet for nabbing 2012 TC4 is to use the JPL Horizons web-interface to generate an ephemeris for your specific location.

Telecopic view of 2012 TC<sub>4</sub>

Asteroid 2012 TC4 imaged during its 2012 pass near Earth. This view combines ten 15-second exposures made as the telescope tracked the asteroid (dot in center).
Gianluca Masi / Virtual Telescope Project

And though it's a frequent visitor to Earth's neighborhood, 2012 TC4 isn't a great candidate for some future asteroid-retrieval mission (ARM), due to its relatively high velocity compared to Earth. For example, Osiris-REX, which made a gravity assist past Earth on September 22nd headed for asteroid 101955 Bennu, requires a "delta V" of only 1.4 km/s for rendezvous and Earth return.

Clouded out? The good folks over at the Virtual Telescope Project have got you covered, with a webcast from Italy tracking 2012 TC4 starting October 11th at 19:00 UT (3:00 p.m EDT) and then the Tenagra observatory in Arizona starts at 2:00 UT on October 12th (10:00 p.m EDT on the 11th).

We can breathe easy as 2012 TC4 gives us a miss . . . for now.