Is This How You Get Hot Jupiters?

This artist’s impression shows a Jupiter-like exoplanet that is on its way to becoming a hot Jupiter — a large, Jupiter-like exoplanet that orbits very close to its star. Courtesy: NOIRLab/NSF/AURA/J. da Silva
This artist’s impression shows a Jupiter-like exoplanet that is on its way to becoming a hot Jupiter — a large, Jupiter-like exoplanet that orbits very close to its star. Courtesy: NOIRLab/NSF/AURA/J. da Silva

When we think of Jupiter-type planets, we usually picture massive cloud-covered worlds orbiting far from their stars. That distance keeps their volatile gases from vaporizing from stellar heat, similar to what we’re familiar with in our Solar System. So, why are so many exoplanets known as “hot Jupiters” orbiting very close to their stars? That’s the question astronomers ask as they study more of these extreme worlds.

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Curiosity Drives Over a Rock, Cracking it Open and Revealing an Amazing Yellow Crystal

The Mars Curiosity rover rolled over this rock containing pure sulfur crystals in May. Planetary scientists are still trying to figure out how the sulfur got there. NASA/JPL-Caltech/MSSS
The Mars Curiosity rover rolled over this rock containing pure sulfur crystals in May. Planetary scientists are still trying to figure out how the sulfur got there. NASA/JPL-Caltech/MSSS

On May 30th, the Mars Curiosity rover was just minding its own business exploring Gediz Vallis when it ran over a rock. Its wheel cracked the rock and voila! Pure elemental sulfur spilled out. The rover took a picture of the broken rock about a week later, marking the first time sulfur has been found in a pure form on Mars.

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Why is Jupiter’s Great Red Spot Shrinking? It’s Starving.

Hubble’s 2021 image of Jupiter shows the Great Red Spot, along with smaller storms that may be affecting its size over time. Courtesy NASA/ESA/STScI.
Hubble’s 2021 image of Jupiter shows the Great Red Spot, along with smaller storms that may be affecting its size over time. Courtesy NASA/ESA/STScI.

The largest storm in the Solar System is shrinking and planetary scientists think they have an explanation. It could be related to a reduction in the number of smaller storms that feed it and may be starving Jupiter’s centuries-old Great Red Spot (GRS).

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Stars Can Survive Their Partner Detonating as a Supernova

A binary star system consisting of two stars: a dense neutron star (lower right) and a normal Sun-like star (upper left). The neutron star formed in a supernova explosion and the Sun-like star survived it. Credit: Caltech/R. Hurt (IPAC)
A binary star system consisting of two stars: a dense neutron star (lower right) and a normal Sun-like star (upper left). The neutron star formed in a supernova explosion and the Sun-like star survived it. Credit: Caltech/R. Hurt (IPAC)

When a massive star dies in a supernova explosion, it’s not great news for any planets or stars that happen to be nearby. Generally, the catastrophic event crisps nearby worlds and sends companion stars careening through space. So, astronomers were pretty surprised to find 21 neutron stars—the crushed stellar cores left over after supernova explosions—orbiting in binary systems with Sun-like stars.

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Neutron Star is Spraying Jets Like a Garden Sprinkler

Radio image from the MeerKAT telescope showing Circinus X-1 in the center, within the spherical remnant of the supernova it was born in. The shock waves caaued by the jets are seen above and below Cir X-1, and the S-shape structure in the jets is somewhat obscured by a bright source in the background. Courtesy Fraser Cowie, Attribution CC BY 4.0.
Radio image from the MeerKAT telescope showing Circinus X-1 in the center, within the spherical remnant of the supernova it was born in. The shock waves caused by the jets are seen above and below Cir X-1, and the S-shape structure in the jets is somewhat obscured by a bright source in the background. Courtesy Fraser Cowie, Attribution CC BY 4.0.

X-ray binaries are some of the oddest ducks in the cosmic zoo and they attract attention across thousands of light-years. Now, astronomers have captured new high-resolution radio images of the first one ever discovered. It’s called Circinus X-1. Their views show a weird kind of jet emanating from the neutron star member of the binary. The jet rotates like an off-axis sprinkler as it spews material out through surrounding space, sending shockwaves through the interstellar medium.

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More Than Half of Near Earth Objects Could Be “Dark Comets”

An artist's concept of a dark comet floating in space. Courtesy Nicole Smith.
An artist's concept of a dark comet floating in space. Courtesy Nicole Smith.

Next time you’re visiting the seaside or a large lake, or even sipping a frosty glass of water, think about where it all originated. There are many pathways that water could have taken to the infant Earth: via comets, “wet asteroids”, and outgassing from early volcanism. Aster Taylor, a University of Michigan graduate student has another idea: dark comets. They’re something of a cross between asteroids and comets and could have played a role in water delivery to our planet.

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Webb Completes Its Second Year of Operations

This “penguin party” (called Arp 142) is loud! The distorted spiral galaxy at center, the Penguin, and the compact elliptical galaxy at left, the Egg, are locked in an active embrace. A new near- and mid-infrared image from the Webb Space Telescope, taken to mark its second year of science, shows that their interaction is marked by a faint upside-down U-shaped blue glow. The blue galaxy at upper right (near bright star) is a closer galaxie teeming with new stars. It's not part of the collision and lies closer to Earth than Arp 142.
This “penguin party” (called Arp 142) is loud! The distorted spiral galaxy at center, the Penguin, and the compact elliptical galaxy at left, the Egg, are locked in an active embrace. A new near- and mid-infrared image from the Webb Space Telescope, taken to mark its second year of science, shows that their interaction is marked by a faint upside-down U-shaped blue glow. The blue galaxy at upper right (near bright star) is a closer galaxie teeming with new stars. It's not part of the collision and lies closer to Earth than Arp 142.

What happens when a spiral and an elliptical galaxy collide? To celebrate the second anniversary of the “first light” for the Webb telescope, NASA released an amazing infrared view of two galaxies locked in a tight dance. They’re called the Penguin and the Egg and their dance will last hundreds of millions of years.

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Ancient People Saw a Kilonova Light up the Sky

A comparison between the observed XMM-Newton image of the kilonova 1181 with an IRAS-derived schematic of infrared contours (presumably of the dust ring) around the resulting white dwarf. This kilonova occurred when two white dwarfs collided and were observed in 1181. Courtesy Ko, et al, 2024.
A comparison between the observed XMM-Newton image of the kilonova 1181 with an IRAS-derived schematic of infrared contours (presumably of the dust ring) around the resulting white dwarf. This kilonova occurred when two white dwarfs collided and were observed in 1181. Courtesy Ko, et al, 2024.

What happens when aging white dwarf stars come together? Observers in feudal Japan in the year 1181 had a front-row view of the superpowerful kilonova created by such a merger. Their records show that a rare “guest star” flared up and then faded. It took until 2021 for astronomers to find the place in the sky where it occurred.

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Webb Looks at One of the Best Gravitationally Lensed Quasars Ever Discovered

A small image of a galaxy distorted by gravitational lensing into a dim ring. At the top of the ring are three very bright spots with diffraction spikes coming off them, right next to each other: these are copies of a single quasar in the lensed galaxy, duplicated by the gravitational lens. In the centre of the ring, the elliptical galaxy doing the lensing appears as a small blue dot. Courtesy: ESA/Webb, NASA & CSA, A. Nierenberg
A small image of a galaxy distorted by gravitational lensing into a dim ring. At the top of the ring are three very bright spots with diffraction spikes coming off them, right next to each other: these are copies of a single quasar in the lensed galaxy, duplicated by the gravitational lens. In the centre of the ring, the elliptical galaxy doing the lensing appears as a small blue dot. Courtesy: ESA/Webb, NASA & CSA, A. Nierenberg

It looks like a distant ring with three sparkly jewels, but the Webb telescope’s (JWST) most recent image is really the view of a distant quasar lensed by a nearby elliptical galaxy. The telescope’s Mid-Infrared Instrument (MIRI) looked at the faint apparition during a study of dark matter and its distribution in the Universe.

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More Evidence that the Kuiper Belt is Bigger Than We Thought

The Kuiper Belt was named in honor of Dutch-American astronomer Gerard Kuiper, who postulated a reservoir of icy bodies beyond Neptune. The first Kuiper Belt object was discovered in 1992. We now know of more than a thousand objects there, and it's estimated it's home to more than 100,000 asteroids and comets there over 62 miles (100 km) across. Credit: JHUAPL
The Kuiper Belt was named in honor of Dutch-American astronomer Gerard Kuiper, who postulated a reservoir of icy bodies beyond Neptune. The first Kuiper Belt object was discovered in 1992. We now know of more than a thousand objects there, and it's estimated it's home to more than 100,000 asteroids and comets there over 62 miles (100 km) across. Credit: JHUAPL

As the New Horizons spacecraft continues its epic journey to explore the Kuiper Belt, it has a study partner back here on Earth. The Subaru Telescope on the Big Island of Hawaii is deploying its Hyper Suprime-Cam imager to look at the Kuiper Belt along the spacecraft’s trajectory. Its observations show that the Kuiper Belt extends farther than scientists thought.

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