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762 Pulcova

Adapted from Wikipedia · Discoverer experience

An image of the main-belt asteroid 762 Pulcova and its satellite taken by the Hubble Space Telescope, showing the wonder of space and celestial bodies.

762 Pulcova is a main-belt asteroid that was discovered by Grigoriy N. Neujmin in 1913. It is named after Pulkovo Observatory, near Saint Petersburg. Pulcova has a diameter of 137 km and is a C-type asteroid, meaning it is dark in colour and made of carbonate material.

Photometric observations of this asteroid from Leura, Australia in 2006 produced a light curve with a period of 5.8403 ± 0.0005 hours and a brightness variation of 0.20 ± 0.02 in magnitude. This result matches earlier studies.

Satellite

Astronomers found a small moon orbiting 762 Pulcova in the year 2000. This moon is about 15 kilometers across and orbits Pulcova at a distance of 800 kilometers. It takes 4 days to go around Pulcova and is much dimmer than the asteroid itself. This was one of the first times scientists found a moon orbiting an asteroid.

Pulcova and its satellite imaged by the Hubble Space Telescope in January 2005

Density

In the year 2000, someone thought Pulcova had a density of 1.8 g/cm3, making it denser than two other space rocks. However, in 2008, another person suggested the density might be only 0.90 g/cm3, meaning it could be a loosely packed pile of pieces instead of one solid object.

Images

Diagram showing the orbit of asteroid 762 Pulkova around the Sun.

Related articles

This article is a child-friendly adaptation of the Wikipedia article on 762 Pulcova, available under CC BY-SA 4.0.

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