|Artist's conception of the NEAR Shoenmaker spacecraft|
Eros was throughout history often object of scientific research, due to its larger size. The asteroid was discovered on August 13, 1898 by Gustav Witt in Berlin and Auguste Chalois in Nice independently. In 1900, a worldwide program was even launched in order to determine Eros' distance to the sun, which resulted in a famous publication by Arthur Hinks at Cambridge. Harold Spencer Jones accomplished even more exact measurements in the 1930s. A few decades later, it was then decided that Eros would be the first c-type asteroid ever visited by a spacecraft.
|A composite image of the north polar region|
The famous rendevous manuever started on February 3, which slowed the spacecraft down and perfectly in time for valentine's day, NEAR went into an elliptical orbit around Eros. In February 2001, NEAR finally accomplished the touchdown on Eros completely operable and undamaged, to the huge surprise to the scientists. They immediately began collecting data and by the end of the month, the last dataset was received by the craft before all connection attempts failed, which is probably due to the extreme temperature changes.
Still, a great amount of data was collected. Eros is with about 13x13x33km the second largest near Earth-asteroids and was studied by the NEAR scientists from orbit for about one year. Also, many scientists claim that another goal of the mission was to link the asteroid to meteorites recovered on Earth in concerns of its chemical composition. Unfortunately, NEAR-Shoemaker did not prove or disprove this link to the satisfaction of the respinsible scientists. However, it was managed to gather highly advanced data in this field of study, wherefore it was still seen as a success. It was also found that due to Eros' peanut-like shape, its surface gravity varies highly. The mission's scientists have found out, that about 1 billlion years ago, an impact occurred on Eros, wherefore a large crater established and that most of the larger rocks found on the asteroid may origin from this incident. Also, it is theorized that seismic shockwaves propagated through the asteroid, shaking smaller craters into rubble.
At yovisto, you may be interested in a lecture by Andrew Cheng, who talks about the NEAR-mission to Eros, its history, accomplishments, problems, and lessons learned.
References and Further Reading:
- The NEAR Rendezvous Burn Anomaly of December 1998
- NEAR image of the day archive
- Eros Project Website