Universe Today

October 7, 2021October 11, 2021 by Matt Williams

Nancy Grace Roman Just Passed a Critical Design Review

High-resolution illustration of the Roman spacecraft against a starry background. Credit: NASA's Goddard Space Flight Center

By 2027, the Nancy Grace Roman Space Telescope – or Roman Space Telescope (RST), for short – will take to space and build on the legacy of the venerable Hubble Space Telescope (HST). Combing a large primary mirror, a camera as sensitive as its predecessors, and next-generation surveying capabilities, Roman will have the power of “One-Hundred Hubbles.” It’s little wonder then why the telescope is named after Dr. Roman (1925 – 2018), NASA’s first Chief Astronomer and the “Mother of Hubble.”

As part of its journey towards realization, this next-generation space telescope recently passed a crucial milestone. This would be the all-important Mission Critical Design Review (CDR), signaling that all design and developmental engineering work is complete. With this milestone reached, the next-generation space telescope is now ready to move from the conceptual stage into the fabrication and assembly phase.

October 7, 2021October 7, 2021 by Evan Gough

An Exoplanet Reaches 2400 C in One Hemisphere. Does it Really Rain Iron?

This artist's illustration shows the fiery exoplanet WASP-76b. Previous study shows the planet rains iron it's so hot. Now astronomers have detected barium in its atmosphere. Image Credit: ESO/M. Kornmesser

WASP-76b is an ultra-hot Jupiter about 640 light-years away from Earth in the constellation Pisces. A few years ago it gained notoriety for being so hot that iron falls as rain. It’s tidally locked to its star, and the planet’s star-facing hemisphere can reach temperatures as high as 2400 Celsius, well above iron’s 1538 C melting point.

Scientists have been studying the planet since its discovery in 2013, and new evidence suggests that it’s even hotter than thought. But, almost disappointingly, there might be no iron rain after all.

October 7, 2021October 6, 2021 by Paul M. Sutter

Are the Burned-Out Remnants of the First Stars all Around us?

An artist's illustration of the Universe's first stars, called Population 3 stars. Pop 3 stars would have been much more massive than most stars today, and would have burned hot and blue. Their lifetimes would've been much shorter than stars like our Sun. Image Credit: Public Domain, https://commons.wikimedia.org/w/index.php?curid=1582286

The first stars to appear in the universe lived fast and died young. Today, none of them likely remain. But their remnants, the black holes and neutron stars, might still wander around the cosmos. Unfortunately, they’re extremely difficult to detect unless they merge, and according to new research the only way to see them would be to conduct an unprecedented survey of the local volume of the universe.

October 7, 2021October 7, 2021 by Nancy Atkinson

Russian Actor and Filmmaker are On the Space Station to Shoot Scenes for a Film

The Soyuz MS-19 rocket with three Russian crewmates aboard ascends into space shortly after launching under clear blues skies in Kazakhstan. Credit: NASA

Earlier this week, a Soyuz spacecraft launched to the International Space Station with three people on board. But only one of them was a cosmonaut. The other two crew members were Russian actress Yulia Peresild and film producer Klim Shipenko. They will be on the ISS for 12 days to film scenes for an upcoming movie, called “Challenge.”

NASA says the film crew is there under a commercial agreement between Roscosmos and Moscow-based media entities, adding that “the launch will mark the expansion of commercial space opportunities to include feature filmmaking.”

October 7, 2021October 7, 2021 by Paul M. Sutter

It’s Official, William Shatner Will be Flying to Space With Blue Origin

William Shatner, photo by Keith McDuffee, CC BY 2.0

Star Trek meets star reality as William Shatner, the iconic 90-year-old actor, will fly on the next Blue Origins suborbital launch on October 12th.

October 6, 2021October 6, 2021 by Evan Gough

One Star Could Answer Many Unsolved Questions About Black Holes

Detection of an unusually bright X-Ray flare from Sagittarius A*, a supermassive black hole in the center of the Milky Way galaxy. Credit: NASA/CXC/Stanford/I. Zhuravleva et al.

A supermassive black hole (SMBH) likely resides at the center of the Milky Way, and in the centers of other galaxies like it. It’s never been seen though. It was discovered by watching a cluster of stars near the galactic center, called S stars.

S stars’ motions indicated the presence of a massive object in the Milky Way’s center and the scientific community mostly agreed that it must be an SMBH. It’s named Sagittarius A*.

But some scientists wonder if it really is a black hole. And one of the S stars could answer that question and a few others about black holes.

October 6, 2021October 6, 2021 by Paul M. Sutter

Astronomers Have a new way to Measure the Mass of Supermassive Black Holes

Even the most supermassive of the supermassive black holes aren’t very large, making it extremely difficult to measure their sizes. However, astronomers have recently developed a new technique that can estimate the mass of a black hole based on the movement of hot gas around them – even when the black hole itself it smaller than a single pixel.

October 6, 2021October 6, 2021 by Paul M. Sutter

Astronomers Might use Pulsars to First Detect Merging Supermassive Black Holes

This artist’s impression shows the material ejected from the region around the supermassive black hole in the quasar SDSS J1106+1939. This object has the most energetic outflows ever seen, at least five times more powerful than any that have been observed to date. Quasars are extremely bright galactic centres powered by supermassive black holes. Many blast huge amounts of material out into their host galaxies, and these outflows play a key role in the evolution of galaxies. But, before this object was studied, the observed outflows weren’t as powerful as predicted by theorists. The very bright quasar appears at the centre of the picture and the outflow spreads about 1000 light-years out into the surrounding galaxy.

Astronomers have been using gravitational waves to detect merging black holes for years now, but may have to rely on pulsars – rapidly spinning neutron stars – to observe the mergers of supermassive black holes.

October 6, 2021October 6, 2021 by Andy Tomaswick

There are Many Metal-Rich Asteroids Nearby to Investigate

Usually, when the topic of asteroid mining comes up, thoughts turn to the riches of the asteroid belt between Mars and Jupiter. The sheer size and scale of the available resources in these asteroids are astounding and overshadow a much more accessible resource – Near-Earth Asteroids (NEAs) that are much closer to home. Now a team from the University of Arizona (UA) has spent some time looking at these near neighbors and realized some are very similar to one of the most famous asteroids in the belt – Psyche.

October 6, 2021October 6, 2021 by Andy Tomaswick

On its Next run, LIGO Will be Able to Probe 8 Times as Much Space

Materials science has once again come through for space exploration. Researchers at the Laser Interferometer Gravitational-Wave Observatory (LIGO) have developed a coating that could increase the sensitivity of LIGO by almost an order of magnitude. That would increase the detection rate of the gravitational waves the observatory is seeking from about once a week to once a day, mainly due to the increased volume of space that the observatory’s interferometers would be able to collect signals from.