Astronomers have spotted one of the strangest-looking asteroids we have ever seen. The space rock, called 44 Nysa, was discovered in 1857, but it wasn’t until now that we had the observational capability to figure out its shape – and its shape is weird.

An E-type asteroid, which is a relatively rare type rich in a mineral called enstatite, 44 Nysa circles the sun in the main asteroid belt between the orbits of Mars and Jupiter. It is the brightest E-type asteroid we know of and one of the largest, with an average diameter of about 75 kilometres, which makes it a tempting observational target.

at the Lowell Observatory in Arizona and her colleagues used the Large Binocular Telescope, also in Arizona, and the Very Large Telescope in Chile to take a closer look at 44 Nysa. They used that data to build a three-dimensional model of the asteroid, and found that it seems to have three lobes, each separated from the others by a thin “neck” that holds the asteroid together.

While two-lobed asteroids are relatively common, trinary ones are much rarer. It isn’t yet clear how exactly it formed – it could have once been a more normal-shaped asteroid and then been battered beyond recognition by other space rocks, or the three lobes could have once been separate and then joined together in what’s called a contact trinary. Either way, its interior must be strong to have stuck together.

Another wrinkle in the story is that 44 Nysa seems to have a tiny moon, just about a kilometre across. In future observations, measuring the moon’s orbit could give us more information about 44 Nysa’s interior structure, and therefore its origins.

The Vera C. Rubin Observatory in Chile is finally beginning its mammoth survey of the universe. After a year of testing and calibration, it is starting the Legacy Survey of Space and Time, which is poised to become the most detailed record of the universe ever captured.

“Today, we begin filming the greatest cosmic movie ever made,” said Brian Stone at the US National Science Foundation in a .

For the next decade, Rubin will collect about 10 terabytes of data every night in the form of hundreds of high-resolution images of the southern sky. Each image will cover an area about 40 times the size of the full moon, and the completed survey will include nearly the entirety of the sky that is visible from the southern hemisphere.

This treasure trove of data will serve several purposes. The first, which has already begun, is to alert researchers to anything changing in the night sky, such as the appearance of supernovae or the motion of asteroids and comets.

“Millions of alerts in just the last couple of months show that Rubin is up and running as a discovery machine,” said at Stanford University in California, who is part of the Rubin team. “Now we’re putting it all together.”

These alerts have already led to the discovery of more than 11,000 new asteroids, and they are expected to result in the most complete inventory of solar system objects ever created.

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In addition to canvassing the solar system, Rubin will provide information about more distant objects, building a detailed map of the Milky Way galaxy and peering deeper into the universe.

An early-release image (above) shows a sea of stars, interstellar gas and even distant galaxies. Such deep, detailed images taken again and again over 10 years will enable researchers to study rare cosmic events and even gain insight into dark matter, dark energy and the expansion of the universe.