Astronomy Archives

September 18, 2020July 7, 2022 by Matt Williams

The Space Court Foundation is Now in Session!

Illustration of Artemis astronauts on the Moon. Credits: NASA

With the closing of the Apollo Era, the priorities of the world’s space agencies began to shift. Having spent the past two decades racing to send astronauts to orbit and to the Moon, the focus now changed towards developing the technologies needed to stay there. A new era of international cooperation, space stations, and partnerships between space agencies and the commercial industry is what followed.

In the near future, things are expected to become even more interesting, with plans for the commercialization of Low Earth Orbit (LEO), the mining of Near-Earth Asteroids (NEAs), and the establishment of a permanent human presence on the Moon. Beyond the logistical and technical challenges this poses, there’s been no shortage of concern about the legal issues and implications this will raise as well.

To this end, a group of legal scholars and space experts recently came together to form the Space Court Foundation (SCF), a non-profit educational organization created to foster a conversation about these and other related space issues. By beginning the conversation now, they hope, the public will be able to play an active role in the burgeoning and evolving domain known as “space law.”

September 17, 2020September 17, 2020 by Evan Gough

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.

September 17, 2020September 17, 2020 by Brian Koberlein

Colliding Neutron Stars Don’t Make Enough Gold to Explain What We See in the Universe

gamma-ray burst from neutron star merger — Artist rendering of colliding neutron stars. Credit: Robin Dienel/Carnegie Institution for Science

In the beginning, the universe created three elements: hydrogen, helium, and lithium. There isn’t much you can do with these simple elements, other than to let gravity collapse them into stars, galaxies, and black holes. But stars have the power of alchemy. Within their hearts, they can fuse these elements into new ones. Carbon, nitrogen, oxygen, and others, all up to the heavy element of iron. When these first stars exploded, they scattered the new elements across the cosmos, creating planets, new stars, and even us.

September 17, 2020September 17, 2020 by Evan Gough

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.

September 16, 2020September 21, 2020 by Evan Gough

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.

September 16, 2020September 16, 2020 by Evan Gough

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

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.

September 15, 2020September 15, 2020 by Evan Gough

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

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.

September 15, 2020September 15, 2020 by Evan Gough

The Milky Way is Already Starting to Digest the Magellanic Clouds, Starting With Their Protective Halos of Hot Gas

A view of the gas in the Magellanic System as it would appear in the night sky. The Magellanic Corona covers the entire sky while the Magellanic Stream is seen as gas flowing away from the two dwarf galaxies, the Large and the Small Magellanic Clouds. This image, taken directly from the numerical simulations, has been modified slightly for aesthetics. Image Credit: COLIN LEGG / SCOTT LUCCHINI

Massive galaxies like our Milky Way gain mass by absorbing smaller galaxies. The Large Magellanic Cloud and the Small Magellanic Cloud are irregular dwarf galaxies that are gravitationally bound to the Milky Way. Both the clouds are distorted by the Milky Way’s gravity, and astronomers think that the Milky Way is in the process of digesting both galaxies.

A new study says that process is already happening, and that the Milky Way is enjoying the Magellanic Clouds’ halos of gas as an appetizer, creating a feature called the Magellanic Stream as it eats. It also explains a 50 year old mystery: Why is the Magellanic Stream so massive?

September 15, 2020September 15, 2020 by Paul M. Sutter

Extreme galaxies depend on extreme conditions for their formation

The spiral pattern shown by the galaxy NGC 2275 in this image from the NASA/ESA Hubble Space Telescope is striking because of its delicate, feathery nature. Credit: ESA/Hubble & NASA, J. Lee and the PHANGS-HST Team; Acknowledgment: Judy Schmidt (Geckzilla)

Some galaxies are too small, and some galaxies are too big, while others are just right. A new survey of the nearby Virgo cluster has potentially revealed why extreme galaxies are the wrong size, and how they might be connected.

September 14, 2020September 14, 2020 by Paul M. Sutter

A beautiful picture of Saturn’s heavily-cratered moon Mimas, processed by @kevinmgill

Mimas, as imaged by NASA's Cassini spacecraft and processed by @kevinmgill

The Cassini mission to Saturn took many images of Mimas, one of the smallest moons in the solar system. And now you can view it in all its icy, cratered glory, thanks to the work of Kevin Gill.