Phantom Galarxy Looks Like A Wormhole

The James Webb Space Telescope's imagery of NGC 628 (the "Phantom Galaxy") shows glowing 

dust in this citizen science image. (Image credit: NASA/ESA/CSA/Judy Schmidt)

A fresh image based on brand-new deep-space data appears to show a wormhole spinning before our very eyes.

The appropriately named "Phantom Galaxy" glows eerily in a new image by Judy Schmidt based on James Webb Space Telescope data collected nearly a million miles away from our planet using the observatory's mid-infrared instrument (MIRI).

"I've been doing this for 10 years now, and [Webb] data is new, different, and exciting," Schmidt told Space.com. "Of course I'm going to make something with it."

The image highlights the dust lanes in the galaxy, which is more properly known as NGC 628 or Messier 74. Dubbed the "perfect spiral" by some astronomers because the galaxy is so symmetrical, the Phantom Galaxy is scientifically interesting because of the intermediate-mass black hole scientists believe is embedded at its heart.

The galaxy has been imaged professionally many times before, including by space observatories such as the Hubble Space Telescope and the Wide-field Infrared Survey Explorer (WISE). 

What makes Webb imagery stand apart from these past efforts is the mid-infrared range that highlights cosmic dust, along with the power of its unique 18-segment hexagonal mirror and deep-space location.

Webb observed M74 earlier this week. The data was also shared on Twitter(opens in new tab) (with different filtration) by Gabriel Brammer, an astronomer at the Cosmic Dawn Center in the Niels Bohr Institute at the University of Denmark.  READ MORE...

A Spectacular Universe

Just 12 million light-years away, the galaxies Messier 81 and 82 offer a nearby preview of the Milky Way-Andromeda merger.

Right in our cosmic backyard, a preview of the Milky Way’s future unfolds.
The galaxy Messier 81, also known as Bode’s Galaxy, is one of the brightest and closest galaxies to Earth not found in our Local Group. By connectng the lower-left corner of the Big Dipper’s cup to the upper-right corner and then traveling that same distance in the same direction, you can find M81 and the other major galaxies of its group all clustered together. (Credit: E. Siegel/Stellarium)

Just outside the Big Dipper’s “cup,” Bode’s Galaxy, Messier 81, lingers.
This optical image of Bode’s Galaxy, M81, comes courtesy of the Hubble Space Telescope. The spiral arms are littered with hot, young, blue stars, while large extent of the arms indicates a gravitational interaction with one or more nearby neighbors. A wider-field and multiwavelength view supports that. (Credit: NASA, ESA and the Hubble Heritage Team (STScI/AURA))

12 million light-years away, it’s a naked eye object for those with acute vision and exceptionally dark skies.
The two largest, brightest galaxies in the M81 Group, M81 (right) and M82 (left), are shown in the same frame in these 2013 and 2014 photos. In 2014, M82 experienced a supernova, visible in the 2014 (blue) image just above the galactic center. (Credit: Simon in the Lakes)

The largest galaxy in the M81 group moves ever-so-slightly towards us.       READ MORE...

Universe Expanding Faster Than Expected

This image from the Hubble Space Telescope features the spiral galaxy Markarian 1337, which is roughly 120 million light-years away from Earth. In 2006, astronomers saw a certain kind of supernova explode in this galaxy, providing researchers with some of the data nee...IMAGE BY ESA/HUBBLE & NASA, A. RIESS ET AL.

The latest measurements with the Hubble Space Telescope suggest the universe is expanding faster than scientists' models predict—a hint that some unknown ingredient could be at work in the cosmos.

It’s one of the biggest puzzles in modern astronomy: Based on multiple observations of stars and galaxies, the universe seems to be flying apart faster than our best models of the cosmos predict it should. Evidence of this conundrum has been accumulating for years, causing some researchers to call it a looming crisis in cosmology.

Now a group of researchers using the Hubble Space Telescope has compiled a massive new dataset, and they’ve found a-million-to-one odds that the discrepancy is a statistical fluke. In other words, it’s looking even more likely that there’s some fundamental ingredient of the cosmos—or some unexpected effect of the known ingredients—that astronomers have yet to pin down.

“The universe seems to throw a lot of surprises at us, and that’s a good thing, because it helps us learn,” says Adam Riess, an astronomer at Johns Hopkins University who led the latest effort to test the anomaly.

The conundrum is known as the Hubble tension, after astronomer Edwin Hubble. In 1929 he observed that the farther a galaxy is from us, the faster it recedes—an observation that helped pave the way toward our current notion of the universe starting with the big bang and expanding ever since.

Researchers have tried to measure the universe’s current rate of expansion in two primary ways: by measuring distances to nearby stars, and by mapping a faint glow dating back to the infant universe. These dual approaches provide a way to test our understanding of the universe across more than 13 billion years of cosmic history. The research has also uncovered some key cosmic ingredients, such as “dark energy,” the mysterious force thought to be driving the universe’s accelerating expansion.

But these two methods disagree on the universe’s current expansion rate by about 8 percent. That difference might not sound like much, but if this discrepancy is real, it means the universe is now expanding faster than even dark energy can explain—implying some breakdown in our accounting of the cosmos.  READ MORE...

Exoplant Clouds

Using data from multiple telescopes, scientists have detected clouds on a gas giant exoplanet some 520 light-years from Earth. So detailed were the observations, they even discerned the altitude of the clouds and the structure of the upper atmosphere, with the greatest precision yet.

It's work that will help us better understand exoplanet atmospheres – and look for worlds that may have conditions hospitable to life, or biosignatures in their spectra. We're also getting closer to making weather reports for distant alien worlds.

The exoplanet in question is WASP-127b, discovered in 2016. It's a hot and therefore puffy beast, orbiting so close to its star that its year is just 4.2 days. The exoplanet clocks in at 1.3 times the size of Jupiter, but only 0.16 times Jupiter's mass.

This means that its atmosphere is somewhat thin and tenuous – perfect for trying to analyze its contents based on the light that streams through it from the exoplanet's host star.

To do this, a team of researchers led by astronomer Romain Allart of the Université de Montréal in Canada combined infrared data from the space-based Hubble Space Telescope, and optical data from the ESPRESSO instrument on the ground-based Very Large Telescope, to peer into different altitudes of WASP-127b's atmosphere.

"First, as found before in this type of planet, we detected the presence of sodium, but at a much lower altitude than we were expecting," Allart said.  TO READ MORE, CLICK HERE...