SHAFAQNA – Asteroid 2015 TB145 that was discovered on October 10 2015 flew slightly outside our moon’s orbit.
In celestial terms, this is rather close, especially considering the asteroid’s size; at an estimated 400 meters wide, this is the closest known flyby by a large asteroid until 2027.
TB145 will fly by at 480,000 kilometers from Earth, but poses no threat to our planet.
And that provides a special kind of Halloween treat for astronomers: the chance to view the surface in radar down to a resolution of as little as 2 meters.
“What’s particularly interesting is the number of boulders on the surface,” Paul Chodas, the Jet Propulsion Laboratory’s manager of the center of near-Earth object studies, told Space.com.
Among NASA’s proposed long-term plans is an asteroid-redirect mission that would move a space rock (or perhaps a large piece of a space rock) closer to Earth for astronauts to explore.
TB145 is not being considered for that mission because its orbit is highly tilted to the ecliptic, the plane in which the Earth and other planets in orbit.
It would take a lot of energy to get there, and there are better asteroid candidates to consider, Chodas said.
What TB145 can do, however, is provide an example of what sorts of boulders are on an asteroid’s surface, Chodas added. “They want to know in general how the asteroids are built, what is their structure, what is their strength, what is the surface distribution of boulders, how many are there, and how well they’re held to the surface.”
TB145 was detected by the University of Hawaii’s Pan-STARRS-1 telescope (the name’s short for Panoramic Survey Telescope and Rapid Response System), which participates in NASA’s near-Earth object observation program.
TB145’s weird, elliptical path through space brings it close to the Earth’s orbit once every three years. But its brush with us is brief, usually a quick dip in and out before flying farther out in the solar system again.
Astronomers think that perhaps past gravitational interactions with Jupiter threw it on the bizarre path.
The asteroid, however, hasn’t come this close to Earth in about 40 years, according to the calculations astronomers ran on its orbit.
“In 1975, there wasn’t really a dedicated search for asteroids and the technology was not as advanced to find asteroids of this size,” Chodas said.
Little is known right now about its composition — optical telescopes will continue observing its spectral signature in a few days — or where its orbit will take it past the next 100 years.
Chodas said the radar telescopes at the Goldstone Deep Space Communications Complex in California and the Arecibo Observatory in Puerto Rico look at the asteroid, among other observatories, very detailed information about its orbit will be available soon.
Astronomers also aim to get more information about TB145’s shape, and how it spins when the sun’s heat hits its surface.
Asteroids tend to spin at inconstant rates, and sometimes regolith (asteroid surface material) can migrate to the equator and fly off, Chodas said.