First Asteroid Mission, Triumphant Despite Many Troubles

Ten years ago today — May 9, 2003 — Japan launched a daring asteroid sample-return mission from the Uchinoura Space Center, atop an M-5 rocket.

(Hayabusa. Image from the National Space Science Data Center.)

Originally called Muses-C, Hayabusa (“Falcon”) was a difficult mission to begin with, but experienced a series of setbacks that made its ultimate success all the more impressive.

  • In late 2003, a large solar flare degraded the spacecraft’s solar panels, reducing the power available to its ion engines. The original rendezvous date in early summer 2005 was pushed back to September.
  • On July 31, 2004, Hayabusa’s X-axis reaction wheel failed.
  • The spacecraft successfully rendezvoused with 25143 Itokawa (1998 SF36) — an asteroid  about as big as three football stadiums at 550 x 180 meters (1800 x 590 feet) — on September 12, 2005. Hayabusa established itself in a heliocentric orbit for station-keeping about 20 km (12.4 mi) from the asteroid.
  • On October 3, 2005 Hayabusa’s Y-axis reaction wheel failed, leaving its attitude control subsystem operating only on “one reaction wheel and two chemical thrusters.”
  • Hayabusa mapped the asteroid’s surface in two phases, then began descent operations. During the second touchdown rehearsal on November 12th, the spacecraft released a “lander/hopper” called Minerva; unfortunately, “the release was at a higher altitude than planned…. and it is believed Minerva moved off into space without landing.”
  • A week later, on November 19, Hayabusa again descended toward the asteroid, and released a “target marker” before contact was lost as it fell to the surface.

Later telemetry indicated that Hayabusa hit the surface at 20:40 UT 19 November (5:40 a.m. JST 20 November) at roughly 10 cm/sec and bounced. It bounced again at 21:10 and then landed at 21:30 within about 30 meters of the target marker. At 21:58 (6:58 a.m. JST 20 November) it was commanded to make an emergency ascent. The craft remained on the surface for about half an hour but did not collect a sample. This was the first ever controlled landing on an asteroid and first ascent from any other solar system body except the Moon.

  • On November 25, Hayabusa touched down again, and fired two “sampling bullets” at the surface. Telemetry could not verify that they actually fired; nevertheless, Hayabusa lifted off.
  • On December 9, ground controllers lost contact with the spacecraft, “presumably because of torques caused by a thruster leak which altered the pointing of the antenna.”
  • Controllers restored communication in March 2006, and learned over the next several months that the spacecraft’s status was somewhat grim: low on fuel, two out of three reaction wheels inoperative, plus 4 out of 11 batteries had also stopped working. The spacecraft’s degraded solar cells and batteries were still sufficient to maintain thrust and attitude control with its xenon ion engine, and in April 2007 it started its journey Earth-ward.

When Hayabusa was a little outside the Moon’s orbit, it released its sample return capsule, which de-orbited on June 13, 2010 and landed near Woomera, Australia.

Subsequent examination of the sample return capsule showed that there were roughly 1500 dust particles, presumably from asteroid Itokawa.

Well done, Hayabusa!

You can learn more about this remarkable mission at this Japan Aerospace Exploration Agency (JAXA) page.

Facebooktwittergoogle_pluspinterestlinkedinmailby feather

Dawn Begins Its Trek to the Asteroid Belt

Five years ago today — September 27, 2007 — a Delta-II launch vehicle carried the Dawn spacecraft to space from Cape Canaveral, sending it on a roundabout journey to the asteroid belt.

(Artist’s conception of the Dawn spacecraft. The glow represents one of the xenon-ion thrusters operating. NASA image.)

After a gravity-boost flyby of Mars in February 2009, Dawn reached its first asteroid target, 4 Vesta, and entered orbit around it in August 2011. There it began its mission to “characterize the asteroids’ internal structure, density, shape, size, composition and mass and to return data on surface morphology, cratering, and magnetism.” Dawn’s measurements and subsequent analysis should help scientists understand better the conditions in the early solar system.

On the main mission page, you can read about one of Dawn’s most exciting discoveries: hydrated minerals on the surface of 4 Vesta. While not as potentially useful as discovering actual water, it did provide evidence that Vesta once held water, but it long since boiled away.

Dawn left Vesta’s orbit this past September 5th, and is scheduled to rendezvous with 1 Ceres in February 2015. It will study that asteroid until the end of its mission, currently set for July 2015.

Facebooktwittergoogle_pluspinterestlinkedinmailby feather

A New Target for Asteroid Exploration?

NASA reported yesterday that Canadian astronomer Martin Connors of Athabasca University identified a 1000-foot-wide asteroid orbiting in a very convoluted path around the Earth’s leading LaGrange point.

Connors made the discovery using data from NASA’s Wide-field Infrared Survey Explorer (WISE) spacecraft.

(Image from the WISE spacecraft, with the newly discovered asteroid 2010 TK7 circled in green. NASA image.)

Surprisingly, the New Scientist article in which I first learned about the find pitches it inaccurately as an asteroid stalking the Earth. It is more accurate to say the asteroid is leading the Earth in its orbit around the sun.

The asteroid is roughly 1,000 feet (300 meters) in diameter. It has an unusual orbit that traces a complex motion near a stable point in the plane of Earth’s orbit, although the asteroid also moves above and below the plane. The object is about 50 million miles (80 million kilometers) from Earth. The asteroid’s orbit is well-defined and for at least the next 100 years, it will not come closer to Earth than 15 million miles (24 million kilometers).

NASA has an interesting video of the asteroid’s orbit: Earth’s First Trojan Asteroid (NASA video)

Alas, 2010 TK7’s odd orbital path probably excludes it from being explored and exploited any time soon. But there are plenty of other possibilities still waiting to be found for future explorers … and even for fictional ones like the “Asteroid Consortium” in my novel.

Facebooktwittergoogle_pluspinterestlinkedinmailby feather

NEAR-Shoemaker Launched

Fifteen years ago today — February 17, 1996 — the Near Earth Asteroid Rendezvous (NEAR) spacecraft launched on a Delta-II rocket out of Cape Canaveral.

(NEAR-Shoemaker spacecraft. NASA image.)

The spacecraft was renamed NEAR-Shoemaker in honor of astronomer Gene Shoemaker, and was sent on its way to the asteroid Eros.

NEAR-Shoemaker flew by the asteroid 253 Mathilde on June 27, 1997, made a gravity-assist maneuver around Earth on January 23, 1998, flew by Eros on 23 December 1998, and finally entered into a tight orbit around Eros on (appropriately enough) Valentine’s Day 2000. As we noted a few days ago, after a year of observations NEAR-Shoemaker landed on Eros on February 12, 2001.

Facebooktwittergoogle_pluspinterestlinkedinmailby feather