Pulsars Could Explain the Excess of Gamma Radiation Coming from the Center of the Milky Way

A gamma-ray view of the sky centered on the core of the Milky Way Galaxy. Could strange spinning neutron stars explain an excess of gamma-radiation emanating from the Milky Way's core region? That's one possibility astronomers are discussing. Courtesy NASA/DOE/Fermi LAT Collaboration
A gamma-ray view of the sky centered on the core of the Milky Way Galaxy. Could strange spinning neutron stars explain a mysterious excess of gamma radiation emanating from the core region? That’s one possibility astronomers are discussing. Courtesy NASA/DOE/Fermi LAT Collaboration

Ever hear of the Galactic Center GeV Excess? No, it’s not a cosmic rock band, although that’s a great name for one. Actually, it’s what astronomers call a super-high rate of gamma-ray radiation coming from the heart of our Milky Way Galaxy. Since this Galactic Center Excess was first detected in 2009, people thought it might be a signature of dark matter annihilating itself in mass quantities. But, as with any unexplained phenomenon in space, others disagreed. It could also have something to do with Sagittarius A*, the galaxy core’s own supermassive black hole. Or, it might be some other kind of strange burst event. Now, an astronomer at the Australian National University suggests that rapidly spinning neutron stars may be the culprits behind this high-energy galactic mystery.

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Astronomers Discover Eight Echoes from Black Holes

A black hole in an x-ray binary system pulls material away from its neigbor star and into its accretion disk. Credit: Aurore Simonnet and NASA’s Goddard Space Flight Center
A black hole in an x-ray binary system pulls material away from its neighbor star and into its accretion disk. Credit: Aurore Simonnet and NASA’s Goddard Space Flight Center

Black holes are the ultimate space-time sinks in the universe. Anything that wanders too close to one of these monsters gets sucked in, never to be seen again. That includes clouds of gas and dust from nearby stars. It all just disappears down the black hole’s insatiable maw. However, not all is lost. As the black hole feeds on the feast supplied by its neighbors, it gives off bright flashes of X-ray light. In a few places, the light bounces off the train of material spiraling into the black hole. That creates what astronomers call a black hole echo. Now, researchers have found eight of these systems relatively close to us in the Milky Way Galaxy.

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They Did It! Rocket Lab Uses Copter to Catch (and Release) a Rocket

Rocket Lab Electron launch
Rocket Lab's Electron rocket rises from its New Zealand launch pad. Credit: Rocket Lab via Twitter

Rocket Lab has just joined SpaceX in the club of space companies that can launch an orbital-class rocket booster and bring it back alive.

In a sense, the California-based company one-upped SpaceX by having a helicopter snag the first-stage booster of its Electron rocket with a cable and a hook as it floated past on the end of a parachute, 6,500 feet above the Pacific Ocean.

So what if the pilots of the customized Sikorsky S-92 helicopter had to release the booster moments later, due to concerns about the way their load was behaving as it swung from the hook?

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This is it! On May 12th we’ll see the Event Horizon Telescope’s Image of the Milky Way’s Supermassive Black Hole

This image contains a collage of ESO’s telescopes at various sites in Chile.

In April of 2019, the international astronomical consortium known as the Event Horizon Telescope (EHT) made headlines worldwide when it announced the first-ever image of a black hole. Specifically, the image showed the glowing disk surrounding the supermassive black hole (SMBH) at the center of the M87 galaxy. In 2021, they followed up on this by acquiring an image of the core region of the Centaurus A galaxy and the radio jet emanating from it.

But in what is sure to be the most exciting announcement yet, the European Southern Observatory (ESO) and researchers from the EHT will announce the results of their survey that examined the SMBH at the center of our very own Milky Way Galaxy – Sagittarius A*! The results will be shared as part of a press conference on Thursday, May 12th, starting at 03:00 PM CEST (08:00 EDT; 05:00 PDT). The event will take place at the ESO Headquarters in Munich, Germany, and live-streamed via an ESO webcast.

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Now, We can Finally Compare Webb to Other Infrared Observatories

The evolution of infrared astronomy, from Spitzer to WISE to JWST. Image credit: Andras Gaspar.

The images released by the James Webb Space Telescope team last week aren’t officially ‘first light’ images from the new telescope, but in a way, it feels like they are. These stunning views provide the initial indications of just how powerful JWST will be, and just how much infrared astronomy is about to improve.

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Humanity Will Need to Survive About 400,000 Years if We Want any Chance of Hearing From an Alien Civilization

Standing beside the Milky Way. Drowming out the night sky blocks us off from nature, and that's not good for humans. Credit: P. Horálek/ESO

If there are so many galaxies, stars, and planets, where are all the aliens, and why haven’t we heard from them? Those are the simple questions at the heart of the Fermi Paradox. In a new paper, a pair of researchers ask the next obvious question: how long will we have to survive to hear from another alien civilization?

Their answer? 400,000 years.

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Watch What Happens to Astronauts When the International Space Station Gets an Orbital Reboost

Astronauts on the International Space Station experience an orbital reboost. Credit: NASA/ESA

This is reminiscent of going down slide on the playground – and then immediately getting back in line to go down again. Except in space.

Here’s what it looks like on board the International Space Station when thrusters fire for an orbital reboost. While it seems like the astronauts are moving inside the station, in in reality it is the Space Station that is moving around them. And in actuality, the acceleration doesn’t happen this fast – the video is sped up eight times. But it still looks like fun!

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Which Parts of Mars are the Safest From Cosmic Radiation?

Artist's impression of a Mars habitat in conjunction with other surface elements on Mars. Credit: NASA

In the coming decade, NASA and China plan to send the first crewed missions to Mars. This will consist of both agencies sending spacecraft in 2033, 2035, 2037, and every 26 months after that to coincide with Mars being in “Opposition” (i.e., when Earth and Mars are closest in their orbits). The long-term aim of these programs is to establish a base on Mars that will serve as a hub that accommodates future missions, though the Chinese have stated that they intend for their base to be a permanent one.

The prospect of sending astronauts on the six-to-nine-month journey to Mars presents several challenges, to say nothing of the hazards they’ll face while conducting scientific operations on the surface. In a recent study, an international team of scientists conducted a survey of the Martian environment – from the peaks of Mount Olympus to its underground recesses – to find where radiation is the lowest. Their findings could inform future missions to Mars and the creation of Martian habitats.

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Space Lettuce Could Reduce Astronaut Bone Loss

All kinds of challenges will face the first humans to travel to Mars. One that has been much discussed, with no potential solution yet, is the potential for a significant amount of bone density loss on the three-year mission.  Astronauts lose about 1% of their bone density per month in the microgravity of the ISS. That’s not too big of a deal if they are only on the station for six months, but the two 10-month space trips of a mission to the red planet could be a concern.  Now a team of researchers think they have a solution – have the astronauts eat more salad.

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China is Building an Asteroid Deflection Mission of its own, due for Launch in 2025

Illustration of the DART spacecraft with the Roll Out Solar Arrays (ROSA) extended. Credit: NASA

There’s an old joke that the dinosaurs are only extinct because they didn’t develop a space agency. The implication, of course, is that unlike our reptilian ancestors, we humans might be able to save ourselves from an impending asteroid strike on Earth, given our six-and-a-half decades of spaceflight experience. But the fact is that while we have achieved amazing things since Sputnik kicked off the space age in 1957, very little effort thus far has gone into developing asteroid deflection technologies. We are woefully inexperienced in this arena, and aside from our Hollywood dramatizations of it, we’ve never yet put our capabilities to the test. But that’s about to change.

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