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Rosetta performs fly-by of asteroid Steins

On the 5th September 2008, the ESA Rosetta spacecraft performed a close fly-by of an asteroid known as (2867) Steins. The first images from the craft's wide angle camera show that Steins is roughly diamond shaped and measures around 5.9 x 4 kilometres. Analysis suggests it has an albedo of between 30-40% - that is to say that it reflects around 35% of the sunlight that falls on it.

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Six Rosetta images of asteroid (2867) Steins, taken from between 800 and 1340 km.
Credit: ESA/Rosetta

The above images show that the asteroid is dominated by a large crater with a diameter of around 2 kilometres, but appears to have 23 craters that are more than 200 metres across. Asteroids will have formed in the early Solar System when tiny particles of dust and metal underwent sticky collisions with each other and gradually formed larger objects. Most of these asteroids will have eventually collided with, and helped to form, one of the planets, but millions still wander the Solar System - most beyond the orbit of Neptune.

The recent fly-by saw the spacecraft pass within 800 kilometres (500 miles) of the asteroid's surface at a speed of 31,000 kilometres per hour (19,200 miles per hour). The main purpose of the Rosetta mission is to rendevous with Comet 67 P/Churyumov-Gerasimenko in 2015. On arrival at 67P, Rosetta will enter orbit around the comet and stay with it as it journeys in towards the Sun. However, en route, Rosetta will pass 2 asteroids: 2867 Steins (in 2008) and 21 Lutetia (in 2010).

For more information about the ESA Rosetts Mission, click here.


Please note that over the weekend of the 26-28th May 2017 we will be switching over to our brand new website - during this time there may be periods where the site is difficult to access, and users will be unable to request observations from the telescope. Please bear with us during this time. All should be back up and running by the 29th May 2017.