This is it! Meet the Supermassive Black Hole at the Heart of the Milky Way

This is the first image of Sgr A*, the supermassive black hole at the centre of our galaxy. Credit: EHT

On April 10th, 2019, the international consortium known as the Event Horizon Telescope (EHT) announced the first-ever image of a supermassive black hole (SMBH). The image showed the bright disk surrounding the black hole at the center of the M87 galaxy (aka. Virgo A). 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. Earlier this month, the European Southern Observatory (ESO) announced that the EHT would be sharing the results from its latest campaign – observations of Sagittarius A*!

This supermassive black hole resides at the center of the Milky Way Galaxy, roughly 27,000 light-years from Earth, 44 million km (27.34 million mi) in diameter, and has a mass of 4.31 million Suns. The campaign’s results were shared in an ESO press release and a series of live-streamed press conferences worldwide, including the ESO Headquarters in Munich, Germany. The team’s results (which were shared in six papers) were also published today in a special issue of The Astrophysical Journal Letters.

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Artemis 1 Probably won't Launch Until August

The Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida, the right-hand center aft booster segment for Artemis I is stacked on the mobile launcher for the Space Launch System (SLS) on Jan. 7, 2021. Photo credit: NASA/Kim Shiflett

On March 17th, the Artemis I mission rolled out of the Vehicle Assembly Building (VLB) and was transferred to Launch Complex 39B at the NASA Kennedy Space Center in Florida. This was the first time that a fully-stacked Space Launch System (SLS) and Orion spacecraft were brought to the launchpad in preparation for a “wet dress rehearsal.” To mark the occasion, NASA released a video of the event that featured a new song by Pearl Jam’s Eddie Vedder (“Invincible”).

Unfortunately, technical issues forced ground controllers to scrub the dress rehearsal repeatedly and return the Artemis I to the VLB on April 26th. This was followed by reports that these issues were addressed and that Artemis I rocket would return to LC 39B by early- to mid-June. Meanwhile, an official NASA statement (issued on Thursday, May 8th) says that the official launch of the mission is not likely to take place until August at the earliest.

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Mars' Carbon Dioxide Glaciers are on the Move

Mars’ south polar ice cap. Credit: ESA / DLR / FU Berlin /

In 1666, famed Italian astronomer and mathematician Giovanni Cassini (the man who discovered four of Saturn’s largest moons) observed the Martian polar ice caps for the first time. However, it was not until the late-18th century, when Sir William Herschel recorded his own observations, that the connection to Earth’s own ice caps was established. In his subsequent treatise, “On the remarkable appearances at the polar regions on the planet Mars” (1784), noted how the southern cap grew and shrunk due to seasonal changes.

With the development of modern telescopes and robotic explorers, scientists have learned a great deal more about these polar deposits. In 2011, they learned that unlike the northermost ice sheet, the southern cap is largely composed of frozen carbon dioxide (aka. “dry ice”). According to new research led by the Planetary Science Institute (PSI), glaciers of carbon dioxide ice have been moving and carving features in the southern polar region for more than 600,000 years – and are on the move right now!

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What’s the Best Way to Build Landing Pads on the Moon?

An illustration of a Moon base that could be built using 3D printing and ISRU, In-Situ Resource Utilization. Credit: RegoLight, visualisation: Liquifer Systems Group, 2018
An illustration of a Moon base that could be built using 3D printing and ISRU, In-Situ Resource Utilization. Credit: RegoLight, visualisation: Liquifer Systems Group, 2018

In the near future, NASA, the European Space Agency (ESA), China, and Roscosmos all mount crewed missions to the Moon. This will constitute the first time astronauts have walked on the lunar surface since the Apollo Era. But unlike the “Race to the Moon,” the goal of these programs is not to get their first and leave only a few experiments and landers behind (i.e., “footprints and flags” missions) but to establish a sustained human presence on the lunar surface. This means creating habitats on the surface and in orbit that can be used by rotating crews.

While NASA and other space agencies intend to leverage local resources as much as possible – a process known as In-Situ Resource Utilization (ISRU) – creating lunar bases will still require lots of materials and machinery to be shipped from Earth. In a recent study, Philip Metzger and Greg Autry reviewed the cost and energy consumption of building landing pads on the lunar surface. After considering various construction methods, they determined that a combination of additive manufacturing and polymer infusion was the most efficient and cost-effective means.

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Canada's Criminal Laws now Extend to Earth Orbit and the Moon

Moon base
Illustration of NASA astronauts on the lunar South Pole. Mission ideas we see today have at least some heritage from the early days of the Space Age. Credit: NASA

In this decade and the next, astronauts will be going to space like never before. This will include missions beyond Low Earth Orbit (LEO) for the first time in over fifty years, renewed missions to the Moon, and crewed missions to Mars. Beyond that, new space stations will be deployed to replace the aging International Space Station (ISS), and there are even plans to establish permanent human outposts on the Lunar and Martian surfaces.

In anticipation of humanity’s growing presence in space, and all that it will entail, legal scholars and authorities worldwide are looking to extend Earth’s laws into space. In a recent decision, the Canadian government introduced legislation extending Canada’s criminal code to the Moon. The amendment was part of the Budget Implementation Act (a 443-page document) tabled and passed late last month in Canada’s House of Commons.

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InSight Senses its two Biggest Marsquakes so far, Coming From the Opposite Side of the Planet

Artist's concept of InSight "taking the pulse of Mars". Credit: NASA/JPL-Caltech

On Nov. 26th, 2018, NASA’s Interior Exploration using Seismic Investigations, Geodesy, and Heat Transport (InSight) lander arrived on Mars. Since then, this robotic mission has been using its advanced suite of instruments to study Mars’ interior and geological activity to learn more about its formation and evolution. One of these is the Seismic Experiment for Interior Structure (SEIS), the lander’s primary instrument, which was deployed on the Martian surface less than a month after it arrived.

On August 25th, 2021, the mission detected a magnitude 4.2 and a magnitude 4.1 marsquake, the two largest seismic events recorded to date. These events (labeled S0976a and S1000a, respectively) were five times stronger than the previous largest event (a 3.7 marsquake in 2019) and the first that originated on the other side of the planet. The seismic wave data from these events could help scientists learn more about the interior of Mars, particularly its core-mantle boundary.

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NASA is Looking for Ideas on How to Simulate Missions to Mars!

In the coming decade, NASA plans to conduct the first crewed missions to Mars. Whereas robotic missions have provided images of the Martian surface for decades, this will be the first time human beings experience the Red Planet directly. In anticipation of these missions, NASA and its commercial partners (Epic Games and Buendea) have come together with HeroX – the leading platform for crowdsourced solutions – to launch the NASA MarsXR Challenge.

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NASA Announces the Winners of its Second Payload Challenge!

Lunar exploration has advanced considerably in the last two decades, with more countries sending robotic orbiters, landers, and rovers to the surface than ever before. These missions have taught us much about the Moon’s geological evolution, composition, environment, and resources. In a few years, this information will prove vital as NASA sends the first astronauts to the Moon since the Apollo Era (as part of the Artemis Program). They will be followed by many more crewed missions, which will eventually lead to the creation of lunar bases.

Alas, there is still a lot that we still need to know before regular, long-duration missions to the Moon can be conducted. To help fill in the gaps in our knowledge, HeroX launched the “Honey, I Shrunk the NASA Payload, the Sequel” Challenge in September 2020. With up to $800,000 in prizes, this competition sought innovative miniature payload designs that could collect information about the lunar environment and its potential resources. The competition’s winners were announced today during the Lunar Surface Innovation Consortium Spring meeting.

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A Space Telescope Could Reveal a Black Hole's Photon Ring

M87 black hole
This view of the M87 supermassive black hole in polarized light highlights the signature of magnetic fields. (Credit: EHT Collaboration)

Despite decades of study, black holes remain one of the most powerful and mysterious celestial objects ever studied. Because of the extreme gravitational forces involved, nothing can escape the surface of a black hole (including light). As a result, the study of these objects has traditionally been confined to observing their influence on objects and spacetime in their vicinity. It was not until 2019 that the first image of a black hole was captured by the Event Horizon Telescope (EHT).

This feat was made possible thanks to a technique known as Very-Long Baseline Interferometry (VLBI), which allowed scientists to see the bright ring surrounding the supermassive black hole (SMBH) at the center of the M87 galaxy. A new study by an international team of astronomers has shown how a space-based interferometry mission could provide reveal even more secrets hiding within the veil of a black hole’s event horizon!

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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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