There Could Be Carbon-Rich Exoplanets Made Of Diamonds

llustration of a carbon-rich planet with diamond and silica as main minerals. Water can convert a carbide planet into a diamond-rich planet. In the interior, the main minerals would be diamond and silica (a layer with crystals in the illustration). The core (dark blue) might be iron-carbon alloy. Credit: Shim/ASU/Vecteezy

Scientists are getting better at understanding exoplanets. We now know that they’re plentiful, and that they can even orbit dead white dwarf stars. Researchers are also getting better at understanding how they form, and what they’re made of.

A new study says that some carbon-rich exoplanets could be made of silica, and even diamonds, under the right circumstances.

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Chinese Asteroid Mining Robot Due to Launch in November

Mining asteroids might be necessary for humanity to expand into the Solar System. But what effect would asteroid mining have on the world's economy? Credit: ESA.

Does it seem like science is catching up with science fiction? Sometimes it does. Especially when there’s an announcement like this one.

A Chinese company says that they’ll be launching an asteroid-mining robot by November.

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Chitin Could be the Perfect Building Material on Mars

An artist's illustration of a Mars settlement. Image: Bryan Versteeg/MarsOne
An artist's illustration of an early Mars settlement. Credit: Bryan Versteeg/MarsOne

It’s hard to deny that we’re heading for a future with a human presence on Mars. But to develop sustained presence, there are an enormous number of technical problems to be worked out. One of those problems concerns manufacturing and building.

We can’t send everything people will need to Mars. We’ll need some way to build structures, and tools and other things.

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A History of the Magellanic Clouds and How They Got Their Names

Image of the night sky taken at the European Southern Observatory’s Very Large Telescope in Chile. The Large and Small Magellanic Clouds are visible in the night sky. Credit: ESO, Y. Beletsky

The Magellanic Clouds are a pair of dwarf galaxies that are bound to the Milky Way. The Milky Way is slowly consuming them in Borg-like fashion, starting with the gas halo that surrounds both Clouds. They’re visible in the southern sky, and for centuries people have gazed up at them. They’re named after the Portuguese explorer Ferdinand Magellan, in our current times.

But they weren’t always called that.

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Searching for Phosphorus in Other Stars

A Southwest Research Institute scientist has identified stellar phosphorus as a probable marker in narrowing the search for life in the cosmos. Stars with phosphorus levels similar to the Sun are considered more likely to host rocky planets with the potential to host life as we know it. Image Credit: NASA/JPL-Caltech

The Search for Life can be a lot messier than it sounds. The three words make a nice, tidy title, but what it entails is extraordinarily difficult. How, in this vast galaxy, can we find life and the planets or moons that might host it? We’re barely at the point of either discovering or ruling out other life in our own Solar System.

Finding it somewhere else in the galaxy, even in our own interstellar neighbourhood, is a task so daunting it can be hard to comprehend.

So any time scientists think they’ve found something that can give them an edge in their near-impossible task, it deserves to be talked about.

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James Webb Will Look for Signs of Life on Planets Orbiting Dead Stars

A planet orbiting a small star produces strong atmospheric signals when it passes in front, or “transits,” its host star, as pictured above. White dwarfs offer astronomers a rare opportunity to characterize rocky planets. Image Credit: Jack Madden/Carl Sagan Institute

Can the galaxy’s dead stars help us in our search for life? A group of researchers from Cornell University thinks so. They say that watching exoplanets transit in front of white dwarfs can tell us a lot about those planets.

It might even reveal signs of life.

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Check Out How Big the Planets and the Moon Will be in Our Sky Over the Next Two Years

This is a screenshot of a data visualization video. It shows the apparent sizes of Solar System objects from our Earthly vantage point. Image Credit: James O'Donoghue

Everything in space is moving. Galaxies collide and merge, massive clouds of gas migrate, and asteroids, comets, and rogue planets zip around and between it all. And in our own Solar System, the planets follow their ancient orbits.

Now a new data visualization shows us just how much our view from Earth changes in two years, as the orbits of the planets change the distance between us and our neighbours.

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Missions Are Already Being Planned to Figure Out What’s Creating the Biosignature on Venus

The planet Venus, as imaged by the Magellan mission. Credit: NASA/JPL

The discovery of phosphine in the upper clouds in Venus’ atmosphere has generated a lot of excitement. On Earth, phosphine is produced biologically, so it’s a sign of life. If it’s not produced by life, it takes an enormous amount of energy to be created abiologically.

On other planets like Jupiter, there’s enough energy to produce phosphine, so finding it there isn’t surprising. But on a small rocky world like Venus, where there’s no powerful source of energy, its existence is surprising.

This discovery clearly needs some more investigating.

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Uranus’ Moons are Surprisingly Similar to Dwarf Planets in the Kuiper Belt

Ö. H. Detre et al./MPIA

Astronomer William Herschel discovered Uranus—and two of its moons—230 years ago. Now a group of astronomers working with data from the telescope that bears his name, the Herschel Space Observatory, have made an unexpected discovery. It looks like Uranus’ moons bear a striking similarity to icy dwarf planets.

The Herschel Space Observatory has been retired since 2013. But all of its data is still of interest to researchers. This discovery was a happy accident, resulting from tests on data from the observatory’s camera detector. Uranus is a very bright infrared energy source, and the team was measuring the influence of very bright infrared objects on the camera.

The images of the moons were discovered by accident.

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Astronomers Have Discovered a 2-km Asteroid Orbiting Closer to the Sun than Venus

NEO asteroid
An artist's conception of an NEO asteroid orbiting the Sun. Credit: NASA/JPL.

Astronomers have painstakingly built models of the asteroid population, and those models predict that there will be ~1 km sized asteroids that orbit closer to the Sun than Venus does. The problem is, nobody’s been able to find one. Until now.

Astronomers working with the Zwicky Transient Facility say they’ve finally found one. But this one’s bigger, at about 2 km. If its existence can be confirmed, then asteroid population models may have to be updated.

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