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6 meteor showers will likely offer better views than the Perseids

Summertime sees the greatest number of “shooting stars,” with July being the peak. And every summer, skywatchers all over the world look forward to observing the Perseid meteors — the “Old Faithful” of the annual meteor displays. In the process, however, most viewers will overlook six relatively minor meteor showers that peak between July 26 and Aug. 21 (three in July and three in August). 

This year, sadly, a nearly full moon will seriously hamper Perseid watching. So why not take this opportunity to see the other six, all of which will enjoy dark, moonless skies?

The radiants for most of these meteor showers will be concentrated in the southern part of the sky between roughly 1 a.m. and 4 a.m. local time. A radiant is the place in the sky where the paths of meteors, if extended backward, would intersect from a particular constellation. Many people are misled into thinking that this is the best place to look for these meteors, but in reality, the radiant is an optical illusion: The meteors are traveling on parallel paths, but due to our perspective, the meteors appear to be darting from this particular spot in the sky. 

Related: Meteor shower guide 2022: Dates and viewing advice

So, in essence, if you concentrate your viewing here, you’ll be looking basically at the vanishing point or a void in the sky. Only the very occasional stationary meteor — one that is coming nearly straight at you — can be seen here. In contrast, the greatest number of meteors will be seen perhaps 30 degrees away from the radiant, in the general direction of the zenith, the point in the sky directly overhead. (Your fist held at arm’s length corresponds to roughly 10 degrees of the sky.)

But the majority of southern showers do make it more likely that any “shooting star” seen in late July or early August will appear to be coming from the south.

In addition to the shower meteors, there are always sporadic ones. Before midnight, these average two or three per hour, and just before dawn, there are perhaps as many as six or seven. The duration in days of the meteor showers provided here is somewhat arbitrary, since the beginning and end are gradual and indefinite. 

Our information was compiled from several sources — most notably, the book “Meteor Showers — A Descriptive Catalog” (opens in new tab) (Enslow, 1988), by Gary Kronk, and the International Meteor Organization’s 2022 Meteor Shower Calendar (opens in new tab).

Alpha Capricornids

This meteor shower peaks on July 26, though it extends from July 10 to Aug. 15. With the July new moon only two days away and the radiant reaching its highest point — about 30 degrees up — in the south at 1:40 a.m. local daylight time, conditions are nearly ideal to look for these bright meteors. The stars of Capricornus (the Sea Goat) form a roughly triangular figure, which may suggest an inverted cocked hat, or perhaps a stingray swimming directly toward you. Only a few Capricornids will appear per hour, so most of the visible meteors will be either sporadic or members of another shower. A good way to separate the two is to imagine the meteor’s path as being extended backward on the sky. Does it pass near Capricornus? If so, it is almost certainly a shower member.

Piscis Austrinids

This meteor shower extends from July 15 to Aug. 10, peaking on July 28. During the height of the Piscis Austrinids, the moon will be in new phase, so you won’t have to worry about moonlight ruining the view. The radiant is not far from the first-magnitude star Fomalhaut, which appears quite low — about 20 degrees, or two fists, above the southern horizon — at 3:15 a.m. Because of its low altitude, this meteor stream is best viewed from the Southern Hemisphere, where the radiant climbs high into the sky and produces up to eight members per hour. 

Delta Aquarids

July 30 marks the peak of the Delta Aquarids, the most prolific of the six minor showers, which runs from July 12 to Aug. 23. Aquarius (the Water Carrier) is pictured as carelessly carrying a water jar so that water is spilling out. The water jar is marked by a little triangle of faint stars, with a fourth star at its center. Interestingly, this shower has two radiants, suggesting that we’re seeing two distinct streams of celestial debris burning up in Earth’s atmosphere. One is located near the star Delta Aquarii, and the other is near the water jar configuration. As many as two dozen meteors per hour are provided by this shower. Expect chiefly faint, medium-speed meteors with occasional significantly brighter events. The moon is still well out of the picture, and both radiants reach their highest point in the south at around 3:40 a.m. at an altitude of roughly 40 degrees, meaning viewing circumstances will be favorable throughout the morning. 

The Perseid meteor shower is seen over the Zhongtiao Mountain range in Yuncheng city, North China’s Shanxi Province, August 14, 2021.  (Image credit: Costfoto/Future Publishing via Getty Images)

Alpha Capricornids

Another weak shower from Capricornus, which began about July 3, peaks the same night as the Delta Aquarids (July 30) and ends on Aug. 15. The radiant is 40 degrees above the horizon at 1 a.m. Though few in number, the Alpha Capricornids frequently produce slow and bright (sometimes fireball-class) yellow meteors that can be quite spectacular. 

Iota Aquarids 

This is the last minor shower before the Perseids and is another two-radiant shower having detectable members from July 15 to Aug. 25. At peak activity on Aug. 6, a bright waxing gibbous moon will set shortly after midnight, leaving the rest of the night dark for meteor watching. At best, perhaps six members per hour are seen under good conditions. The radiants are at their highest — 40 degrees high in the south — at 2:15 a.m.

The Perseids

A waning gibbous moon, one and a half days past full, will dominate the overnight skies of Aug. 12 to 13 to spoil this year’s annual performance of the Perseid meteor shower. The radiant, which is not far from the famous Double Star Cluster in northern Perseus, rises in the evening and is nearly 70 degrees above the northern horizon at the break of dawn. If not for the hampering effect of moonlight, observers would notice a crescendo in hourly rates averaging more than 60 meteors per hour, though double this rate has been seen on occasion. Many flaring meteors with trains are seen under dark skies, but unfortunately, only the brightest of them will be visible in 2022. This shower normally extends from July 25 through Aug. 18. 

Related: Perseid meteor shower 2022: When, where & how to see it

Kappa Cygnids

This is the last of the summer meteor showers, with the next significant display (the Orionids) not coming until the latter half of October. The host constellation Cygnus (the Swan) is formed by a large figure of six stars popularly called the Northern Cross, the long axis of which lies lengthwise along the Milky Way. The limits for this shower run from Aug. 3 to 25, with the peak occurring Aug. 17. But although the maximum rate is only three or four meteors per hour, this stream does provide slow-moving, sometimes brilliant flaring fireballs, and a careful skywatcher may be nicely rewarded for the time spent. On peak night, the moon is a waning gibbous and does not rise until around 10:30 p.m., but the hours before midnight are still the best time to view this shower. At its highest, the star Kappa Cygni — from where these meteors appear to radiate — stands more than 75 degrees above the northern horizon at 10:15 p.m. 

Joe Rao serves as an instructor and guest lecturer at New York’s Hayden Planetarium (opens in new tab). He writes about astronomy for Natural History magazine (opens in new tab), the Farmers’ Almanac (opens in new tab) and other publications. Follow us on Twitter @Spacedotcom (opens in new tab) and on Facebook (opens in new tab)



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Perseid meteor shower begins: When, where to see it

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The Perseids – one of the biggest meteor showers of the year – have returned this summer.

According to NASA, the evenings of Aug. 12 and Aug. 13 will be a great opportunity for skywatchers to catch the show. 

However, a full moon could negatively impact the view this year.

The agency notes that the Perseids are generally active from July 14 through Aug. 24.

NASA MARS ROVER DISCOVERS WEIRD STRING-LIKE OBJECT THAT GOES VIRAL

INNER MONGOLIA, CHINA – AUGUST 17, 2021 – The Perseid meteor shower is seen over the Tengger Desert in North China’s Inner Mongolia Autonomous Region, Aug. 17, 2020. 
(Photo credit should read Costfoto/Future Publishing via Getty Images)

According to FOX Weather, storms could also be a negative factor, and the channel said that July 28 – when there is a new moon – will also be an excellent time to stargaze.

The channel noted that, depending on where the viewer is in the Northern Hemisphere, there could be up to 40 meteors seen per hour during the shower’s peak.

The Perseids occur when Earth crosses through the stream of debris of the comet 109P/Swift-Tuttle and its meteors – most of which are pea-sized – create bright “shooting stars” as they burn up in the planet’s atmosphere.

Photomontage taken on Aug. 13, 2021 shows the night sky during the Perseid Meteor Shower above an ecological demonstration zone of Engebei in Kubuqi Desert, north China’s Inner Mongolia Autonomous Region. 
(Photo by Lian Zhen/Xinhua via Getty Images)

NASA’S PERSEVERANCE ROVER SPOTS PIECE OF ITS OWN LANDING GEAR ON MARS

The meteors appear to radiate from the constellation Perseus, or the shower’s “radiant,” but can be seen streaking across the sky anywhere at a speed of 37 miles per second.

The shower is also known for its fireballs, which can last longer than an average meteor streak.

The Perseid meteor shower is seen over the Zhongtiao Mountain range in Yuncheng city, North China’s Shanxi Province, Aug. 14, 2021. 
(Photo credit should read Costfoto/Future Publishing via Getty Images)

Swift-Tuttle orbits between the sun and beyond the orbit of Pluto once every 133 years. 

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Every year, the Earth passes near the path of the comet.

NASA says there is no chance the planet will soon run into the comet. 

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The observation of Chern mosaic and Berry-curvature magnetism in magic angle graphene

a, Schematic layout showing backgate voltage V_bg^dc+V_bg^ac applied to the MATBG sample and the corresponding change in the local magnetic field B_z^ac (x,y) is imaged using the scanning SOT. The Chern mosaic is shown schematically in the MATBG. b, m_z (x,y,ν_↑) measured at B_a=50 mT and ν= 0.966. The red (blue) colors indicate paramagnetic-like (diamagnetic-like) local differential magnetization. c, Chern mosaic map derived from the evolution of m_z (x,y,ν_↑) showing the C=1 (KB polarization, blue), C=-1 (KA, red), and C=0 or semimetallic intermediate regions (green). Credit: Grover et al.

Researchers at the Weizmann Institute of Science, the Barcelona Institute of Science and Technology and the National Institute for Material Science in Tsukuba (Japan) have recently probed a Chern mosaic topology and Berry-curvature magnetism in magic-angle graphene. Their paper, published in Nature Physics, offers new insight about topological disorder that can occur in condensed matter physical systems.

“Magic angle twisted bilayer graphene (MATBG) has drawn a huge amount of interest over the past few years due to its experimentally accessible flat bands, creating a playground of highly correlated physics,” Matan Bocarsly, one of the researchers who carried out the study, told Phys.org, “One such correlated phase observed in transport measurements is the quantum anomalous Hall effect, where topological edge currents are present even in the absence of an applied magnetic field.”

The quantum anomalous Hall effect is a charge transport-related phenomenon, in which a material’s Hall resistance is quantized to the so-called von Klitzing constant. It resembles the so-called integer quantum Hall effect, which Bocarsly and his colleagued had studied extensively in their previous works, particularly in graphene and MATBG.

Building on their past findings, the researchers set out to further investigate the quantum anomalous Hall effect using the measurement tools that they found to be most effective. To do this, they employed a scanning superconducting quantum interference device (SQUID), which was fabricated on the apex of a sharp pipette. This device is an extremely sensitive local magnetometer (i.e., sensor that measures magnetic fields), which can collect images in the 100nm scale.

“By varying the carrier density of our sample, we measured the response of the local magnetic field,” Bocarsly explained. “At low applied fields this magnetic response is exactly correlated with the internal orbital magnetization of the Bloch wave functions, which is induced by the Berry curvature. So, in essence we have a local probe that measures the local Berry curvature.”

Directly measuring the orbital magnetism induced by local Berry curvature in MATBG is a highly challenging task, which had never been attained before. This is because the signal is extremely weak, thus it eludes most existing magnetic measurement tools.

Bocarsly and his colleagues were the first to directly measure this elusive signal. During their experiments, they also observed a Chern mosaic topology in their sample, thus identifying a new topological disorder in MATBG.

“The Chern number, or the topology of an electronic system, is generally thought to be a global topological invariant,” Bocarsly said. “We observed that on a device scale (order of microns), the C number is not invariant, but alternates between +1 and -1. This introduces a new type of disorder, topological disorder, into condensed matter systems that needs to be accounted for in device fabrication and theoretical analysis.”

The recent study by this team of researchers greatly contributes to the understanding of MATBG, both in terms of its magnetism and topology. In the future, it could inform the development of more precise theoretical models of this material, while also potentially facilitating its implementation in various quantum computing devices.

“Our low field local orbital magnetization probe can also be used to investigate other fundamental properties such as local time reversal symmetry breaking,” Bocarsly added. “There are still many open questions about integer filling states of MATBG and the symmetries that they obey, which could be an interesting direction for future exploration.”


The direct detection of a topological phase transition through a sign change in the Berry curvature dipole


More information:
Sameer Grover et al, Chern mosaic and Berry-curvature magnetism in magic-angle graphene, Nature Physics (2022). DOI: 10.1038/s41567-022-01635-7

© 2022 Science X Network

Citation:
The observation of Chern mosaic and Berry-curvature magnetism in magic angle graphene (2022, July 22)
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Nasa’s James Webb telescope reveals millions of galaxies

SMACS 0723: Red arcs in the image trace light from galaxies in the very early Universe

There were 10 times more galaxies just like our own Milky Way in the early Universe than previously thought.

This cosmic insight comes form one of the first studies of images captured by Nasa’s new James Webb Space Telescope.

One of its authors, Prof Christopher Conselice from the University of Manchester, UK, said that Webb could “zoom in on the early Universe”.

This yielded insights about objects in space that “we knew existed but didn’t understand how and when they formed”.

Disc galaxies dominate the “galaxy population” today,” the researcher explained.

“Our own galaxy is a disc, Andromeda (our nearest neighbour, which is 2.5 million light-years from Earth) is a disc.

“Three-quarters of nearby galaxies are discs, but it was thought that they formed late in the evolution of the Universe,” he told BBC News.

That was before the James Webb Space Telescope gave astronomers a view so far back in time.

The study, which has been published on a preprint server, meaning it has yet to be peer reviewed by other scientists in the field, used the first image released from the telescope.

This image shows a foreground cluster of galaxies called SMACS 0723. The gravity of this great mass of objects has magnified the light of galaxies in the background, in distant Universe, making them visible for the first time. Some of these galaxies existed a mere 600 million years after the Big Bang.

Webb is taking some incredible pictures: “This might be the most important telescope ever”

Webb, with its 6.5m-wide golden mirror and super-sensitive infrared instruments, is able to resolve their shapes and count them.

“We knew we would see things Hubble didn’t see. But in this case we’re seeing things differently,” said Prof Conselice, who will be presenting some of his discoveries on Saturday 23 July at the Bluedot Festival at Jodrell Bank in Cheshire.

The Universe is about 13.8 billion years old, so the images that the JWST is capturing are glimpses of the processes that formed stars and planets long before our own came into existence.

“These are the processes we need to understand if we want to understand our origins,” said Prof Conselice.

“This might be the most important telescope ever,” he added. “At least since Galileo’s.”

James Webb is a joint effort between the American, European and Canadian space agencies, with Nasa in the lead.

James Webb

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Customer Finds 100 Million-Year-Old Footprints Belonging to World’s Largest Dinosaur Species At a Restaurant in China!

Picture of a dinosaur track found at the restaurant.

(Lida Xing (facebook.com/xinglida))

Imagine walking into a restaurant in search of something delicious, only to find dinosaur footprints dating back to the Cretaceous! Believe it or not, that’s precisely what happened with a palaeontology-enthusiast in China earlier this month.

On July 10, Ou Hongtao visited a restaurant in Leshan (based in China’s Sichuan province) as per usual, when his eyes caught something quite unusual. In the yard of the restaurant, he spotted “special dents” on the ground that looked very much like dinosaur footprints to him.

His assumptions were soon confirmed by a team headed by Dr Lida Xing, a palaeontologist and associate professor at the China University of Geosciences.

Using a 3D scanner, the team was able to deduce that the prints were left behind by two brontosauruses, a genus of gigantic quadruped sauropod dinosaurs. They roamed the Earth during the Cretaceous period that lasted from about 145 to 66 million years ago, at a time when dinosaurs flourished around the globe.

These dinos, which had four thick legs and an extremely long neck, are believed to be among the largest land animals to have ever existed! They were 122 feet long and an estimated 70 tons heavy, extending the length of three buses and weighing as much as 10 African elephants.

This discovery was made just 5 kilometres from the Giant Buddha of Leshan — the world’s largest stone Buddha statue that’s carved out of a cliff of red sandstone. In fact, the 8-metre-long footprints were found preserved in sediment similar to what was used to create the statue.

What makes this find even more incredible is its rarity — in China, the field of palaeontology is being hampered by the country’s rapid development, with construction projects increasingly destroying countless fossils.

It was sheer luck that kept these footprints intact. Prior to the restaurant, the site was home to a chicken farm where sand and dirt possibly helped protect the prints.

And once the restaurant owner took over, his preference for a natural stone look was the sole reason why he decided not to cover the ground with cement and unknowingly bury the prints with it. Quite fascinating, isn’t it?

**

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Rocket Report: A heavy-lift rocket funded by crypto; Falcon 9 damaged in transport

Enlarge / An Electron rocket launches the NROL-162 mission on July 13.

Rocket Lab

Welcome to Edition 5.04 of the Rocket Report! Be sure and read to the end, as most of the news this week concerns heavy-lift rockets, or at least proposed heavy-lift rockets. Also, there will be no newsletter next week as I’ll be taking some vacation time with the family. But after that I’ll be back in the saddle for the remainder of the summer and fall, which promises to be full of big-ticket rocket launches.

As always, we welcome reader submissions, and if you don’t want to miss an issue, please subscribe using the box below (the form will not appear on AMP-enabled versions of the site). Each report will include information on small-, medium-, and heavy-lift rockets as well as a quick look ahead at the next three launches on the calendar.

Isar Aerospace to launch from French Guiana. The Germany-based launch startup announced Thursday that it will conduct commercial and institutional launches from the European spaceport in French Guiana beginning as early as 2024. In what appears to be a nice coup, Isar was selected by French space agency CNES for the opportunity to launch at the Diamant launch complex near the equator. Isar is also developing a spaceport in Andøya, Norway, for its Spectrum small launch vehicle.

Competing with other small launchers … “With adding Kourou, we will further extend our global network of critical infrastructure and gain even more flexibility for our customers,” said Josef Fleischmann, chief operating officer and co-founder of Isar Aerospace. “Creating more launch and deployment capabilities is an essential block to take on the global market for satellite launches.” Isar will be competing with companies like Relativity Space, ABL Space Systems, and Firefly for commercial payloads in the 1-ton class. (submitted by Ken the Bin)

Firefly works toward second Alpha launch. Firefly Aerospace is preparing for the second launch of its Alpha rocket in late August or early September, Space News reports. “Our target is in the next 45 to 60 days of being able to launch,” Peter Schumacher, interim chief executive of Firefly, told the publication. “It’s really pending, at this point, range availability.” The rocket itself is ready for flight, he said, other than performing a wet dress rehearsal and a static fire test, which he said would be done within two weeks of launch.

Modeling a rocket’s debris … The company is waiting on a launch license from the Federal Aviation Administration, which in turn depends on approval of a new debris model for the rocket. The revised debris model came after the first Alpha rocket exploded in flight when the range activated its flight termination system. Debris from the rocket, made primarily of carbon composite materials, fell outside of the range, including in nearby communities, although no damage was reported. (submitted by EllPeaTea and Ken the Bin)

The easiest way to keep up with Eric Berger’s space reporting is to sign up for his newsletter, we’ll collect his stories in your inbox.

Electron launch postponed due to payload issue. Rocket Lab’s next mission for the National Reconnaissance Office—the second of two back-to-back launches for the US spy satellite agency—has been postponed to complete a software update on the classified payload, Spaceflight Now reports. Named NROL-199, the mission was scheduled to launch Friday from Rocket Lab’s spaceport in New Zealand and would have meant that the company launched two Electrons in a nine-day period.

Where will NRO go? … Previously, Rocket Lab launched the NROL-162 mission on July 13. As soon as the software updates are implemented, NRO and Rocket Lab will provide a new launch date for NROL-199. The payloads are classified, as with most NRO satellites. They will operate in low Earth orbit, but the target orbital altitude and inclination have not been released. (submitted by Ken the Bin)

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How can astronauts explore Mars’ Grand Canyon, Valles Marineris

There are many in Mars exploration circles that see Valles Marineris as a “tell all” place, ripe for human exploration that can uncover the planet’s history and its capacity to sustain microbial life. 

That said, how best to investigate the multifaceted geology in evidence at this site? Can future crews on the Red Planet dive safely into this huge canyon system? And what awaits those probing a vast region that’s been branded as the Grand Canyon of Mars?

Valles Marineris is a humongous feature; a system of canyons cutting across the Martian surface spanning 2,500 miles (4,000 kilometers), covering about one-fifth the circumference of Mars. At some points, this colossal chasm is 125 miles (200 km) wide. In certain places, the canyon floor reaches a depth of 5 miles (8 km). 

Bottom line: that’s far deeper than Earth’s Grand Canyon.

Related: Glaciers on Mars likely helped carve Red Planet’s ‘Grand Canyon’

To encourage on-the-spot human studies of Valles Marineris, some scientists have pinpointed and provisionally named an area known as the “Noctic Landing” site. Its strategic location allows the shortest possible surface excursions to the Martian volcanic plateau of Tharsis as well as Valles Marineris — that grand feature and region on the Red Planet that exposes the longest record of Mars’ geology and evolution through time.

Tharsis is the area of Mars that has experienced the longest and most extensive volcanic history, and might still be volcanically active. Some of the youngest lava flows on Mars have been identified on the western flanks of the Tharsis Bulge. 

Furthermore, those flows are within driving range of future pressurized rover traverses.

Top priority science

“I think that, when it comes to planning human missions to Mars, we might be past the point of thinking only about notional science objectives in location-agnostic ways,” said Pascal Lee, a planetary scientist at NASA Ames Research Center in California and the SETI Institute. 

Lee is chairman of the Mars Institute, an international, non-governmental, non-profit research organization dedicated to advancing the scientific study, exploration, and public understanding of Mars. He’s also director of the NASA Haughton-Mars Project, an international multidisciplinary field research project focused on Mars analog studies at the Haughton impact crater site on Devon Island in the High Arctic.

We can and should, right now, look for human landing sites where most if not all our top priority science objectives could be met, Lee told Space.com. That human touchdown zone would likely offer multiple ways of extracting water locally — something a robotic scouting mission could ascertain — and where it would make sense to establish a base for long term exploration, he said.

Noctis Landing on Mars is an ostensibly flat transitional region between Noctis Labyrinthus and Valles Marineris proper.  (Image credit: Pascal Lee)

At the crossroads

Lee is passionate that such a site that he dubs Noctis Landing is an ostensibly flat transitional region between Noctis Labyrinthus (Latin for ‘the labyrinth of night’) and Valles Marineris proper.

Noctis Landing not only offers a large number and wide range of regions of interest for short-term exploration, it is also located strategically at the crossroads between Tharsis and Valles Marineris, which are key for long-term exploration. The area is distinguished for its maze-like system of deep, steep-walled valleys.

“If you head east or south from Noctis Landing, you go deeper into Valles Marineris and can look for signs of past life,” Lee said. “If you head west or north from Noctis, you climb onto Mars’ giant volcanoes with their many caves, and can look for extant life.”

No rock-climbing required

The upshot is that the Noctis Landing locale is unique, being at the literal junction of the search for signs of past and present life on Mars.

As for exploring Valles Marineris, the key advantage of Noctis Landing is that you can access all the rock layers of the canyon without having to resort to rock-climbing, Lee said.

“Thanks to the giant Oudemans impact crater nearby the Noctis Landing, giant slabs of Valles Marineris canyon walls have been laid flat there, ready for you to explore, one rock layer at a time, by just driving along the canyon floor,” Lee added.

Once down at Noctis Landing, astronaut explorers have a number of routes to investigate Mars. (Image credit: Pascal Lee, et al.)

Hidden water

Late last year, Igor Mitrofanov of the Space Research Institute of the Russian Academy of Sciences in Moscow, Russia reported that a significant quantity of hidden water has been spotted at the central part of Mars’ dramatic canyon system, Valles Marineris.

The observation came via the European Space Agency-Roscosmos ExoMars Trace Gas Orbiter (TGO). Mitrofanov is the principal investigator of the TGO-toted Fine Resolution Epithermal Neutron Detector (FREND) neutron telescope. That instrument is mapping the hydrogen — a measure of water content — in the uppermost meter of Mars’ soil.

Mitrofanov and colleagues found evidence for unusually high hydrogen abundances in the heart of Valles Marineris on Mars.

Unclear mix of conditions

“With TGO we can look down to one meter below this dusty layer and see what’s really going on below Mars’ surface — and, crucially, locate water-rich ‘oases’ that couldn’t be detected with previous instruments,” Mitrofanov stated (opens in new tab) in an ESA-issued statement.

“Assuming the hydrogen we see is bound into water molecules, as much as 40% of the near-surface material in this region appears to be water,” Mitrofanov said. 

As the ESA statement puts it, the detection suggests that “some special, as-yet-unclear mix of conditions must be present in Valles Marineris to preserve the water — or that it is somehow being replenished.”

Mitrofanov and his research associates published their work (opens in new tab) in the March 2022 issue of the journal Icarus, stating: “Such ice not only is an intriguing material for searching frozen proto-life fragments or complex organic molecules from the early epoch of Mars, but also is an indispensable natural resource for future Mars exploration that is easy to exploit.”

Fog banks

NASA’s Lee underscored the intriguing finding that there’s frequent occurrence of fog in Valles Marineris. “While the average Martian atmosphere is generally considered to hold too little water vapor for it to be worth compressing and exploiting, the presence of ice fog, the most likely explanation for the fog banks frequently filling Valles Marineris, indicates that the Martian atmosphere could be locally supersaturated in water, possibly up to amounts worth extracting,” he said.

The presence of fog in Valles Marineris, Lee said, also suggests that at least part of the hydrogen detected by Mitrofanov and his associates is likely to be in the form of H2O, not just water of hydration in minerals.

The European Space Agency’s Mars Express caught this image of fog at Valles Marineris. (Image credit: ESA/DLR/FU Berlin (G. Neukum))

Taking to the air

Purging Valles Marineris of its scientific holdings could be augmented by aerial vehicles, said Abigail Fraeman, a research scientist and Mars Science Laboratory Deputy project scientist at NASA’s Jet Propulsion Laboratory.

That view is clearly backed by the airborne success of NASA’s Ingenuity Mars helicopter at Jezero Crater.

“We can start to imagine all sorts of possibilities for future Mars exploration with aerial assets,” Fraeman told Space.com. “One of the benefits of exploring Mars from the air is the ability to travel much longer distances over terrains that would be too treacherous for rovers.”

Astronauts working on the surface of Mars could employ a helicopter (airborne at left) similar to the Ingenuity Mars Helicopter.  (Image credit: NASA)

Fraeman said that Valles Marineris is one example of a site that might really benefit from exploration by helicopters. “This platform could enable us to explore sections of really ancient crust exposed in the walls of the canyon, the steep layered sedimentary deposits in the canyon’s center, and even the mysterious recurring slope lineae which occur on steep slopes throughout Valles Marineris and might be formed by very salty liquid water.” 

Exploring these features, Fraeman added, “would help us answer questions about the entirety of Mars’ history, from the first formation through the present day, and provide unprecedented insight into mechanisms that affect the climate and habitability of Mars, as well as rocky worlds beyond our solar system.”

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JWST’s stunning ‘Phantom Galaxy’ picture looks like a wormhole

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.”

Live updates: NASA’s James Webb Space Telescope mission
Gallery: James Webb Space Telescope’s 1st photos

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. 

A selected of raw Webb imagery is made publicly available at this portal (opens in new tab) a few hours or days after observations, and amateur imagers and scientists are free to use the data as long as they credit the source when publishing.

The Phantom Galaxy, also known as Messier 74 or NGC 628, as seen by the Hubble Space Telescope. (Image credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration)

The busy deep-space telescope released its first operational images on July 12 of deep-space objects, including a nebula and a view of very young galaxies. An infrared view of Jupiter, along with the gas giant’s moons and rings, joined the iconic new images on July 14. 

That week’s work alone showcases Webb’s flexibility in switching between faraway objects near the cosmic dawn — when stars began shining — and solar system objects much closer to its viewfinder.

As for the Phantom Galaxy, Schmidt used Photoshop and FITS Liberator for most of the work and said many of the concepts in her 2017 YouTube imaging tutorial (opens in new tab) will help with the more advanced software of today.

You can check out more spectacular imagery of Webb photos and other cosmic objects at Schmidt’s Flickr page (opens in new tab).

Follow Elizabeth Howell on Twitter @howellspace (opens in new tab). Follow us on Twitter @Spacedotcom (opens in new tab) and on Facebook (opens in new tab)



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Scientists Analyzed Penguin DNA And Found Something Quite Remarkable

Penguins are no strangers to climate change. Their life history has been shaped by rising and falling temperatures, and their bodies are highly specialized for some of Earth’s most extreme conditions.

 

And yet, scientists are concerned the evolutionary path of the penguin may be grinding to a halt, thanks to what appears to be the lowest evolutionary rates ever detected in birds.

A team of international researchers has just published one of the most comprehensive studies of penguin evolution to date, which is the first to integrate data from living and fossil penguin species.

The research unveils the tumultuous life history of penguins in general, with three-quarters of all known penguin species – now represented by fossils only – already extinct.

“Over 60 million years, these iconic birds have evolved to become highly specialized marine predators, and are now well adapted to some of the most extreme environments on Earth,” the authors write.

“Yet, as their evolutionary history reveals, they now stand as sentinels highlighting the vulnerability of cold-adapted fauna in a rapidly warming world.”

On land, penguins can appear a bit ridiculous, with their awkward waddle and seemingly useless wings. But underwater, their bodies are transformed into hydrodynamic torpedoes that would make any fleeing fish wish it could fly.

 

Penguins had already lost their ability to fly 60 million years ago, before the formation of the polar ice sheets, in favor of wing-propelled diving.

The fossils and genomic data suggest the unique features that enable penguins’ aquatic lifestyles emerged early in their existence as a group, with rates of evolutionary change generally trending downwards over time.

The scientists think penguins originated on a Gondwanan micro-continent called Zealandia, which is now mostly submerged under the ocean.

The paper suggests the ancestors of modern penguins – crown penguins – emerged approximately 14 million years ago, a whole 10 million years after genetic analyses have hinted at.

This particular period would coincide with a moment of global cooling named the middle Miocene climate transition. Living penguins, however, split into separate genetic groups within the last 3 million years.

Penguins spread out across Zealandia before dispersing to South America and Antarctica multiple times, with later groups likely hitching a ride on the Antarctic Circumpolar Current.

The scientists found that almost every penguin species experienced a period of physical isolation during the Last Glacial Period.

 

Their contact with other penguins was limited during this time, as groups were forced to live in more fragmented areas of habitat further north, where they could still find food and shelter.

As a result, the DNA pool of each group became narrower, pushing species further apart genetically.

In the period of warming that followed, they moved back towards the poles, and some groups, now much more genetically distinct, crossed paths once more.

The way certain groups of penguins experienced these significant climate events offers insight into how they might cope with human-caused climate change.

The groups that increased in number when warming occurred shared some features: They were migratory, and foraged offshore. The researchers think these features allowed them to respond to changing climates better, especially the ability to look further afar for prey and to move to lower latitudes.

Those that decreased in number, on the other hand, lived in one particular place, and foraged closer to shore for food: a lifestyle that doesn’t cope too well when the conditions ‘at home’ drastically change.

 

But penguins’ ability to change might be limited by more than just lifestyle – it seems to be embedded in their genes.

It turns out that penguins have the lowest evolutionary rates yet detected in bird species, along with their sister order, Procellariiformes, which includes birds like petrels and albatrosses.

The researchers compared 17 different orders of birds overall, using several genetic signatures closely related to rates of evolutionary change.

They noticed that aquatic birds generally had slower rates of evolution than their terrestrial kin, so they think the adoption of an aquatic lifestyle might go hand-in-hand with low evolutionary rates. They also think that evolutionary rates in birds are lower in cooler climates.

The order Pelecaniformes, which includes seafaring birds like pelicans and cormorants, were a near third for lowest evolutionary rate, and waterfowl (order Anseriformes) had much lower rates than earthbound fowls like turkeys, chickens, and quails (order Galliformes).

The researchers note that the ancestral crown penguins evolved at a faster rate than living penguins, but even then, this was slow compared to other birds.

Half of all living penguin species are endangered or vulnerable, and the scientists say their slow evolutionary rates and niche lifestyles could send penguins towards a dead end.

“The current pace of warming combined with limited refugia in the Southern Ocean will likely far exceed the adaptive capability of penguins,” they write.

“The risks of future collapses are ever-present as penguin populations across the Southern Hemisphere are faced with rapid anthropogenic climate change.”

This research was published in Nature Communications.

 

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Ancient Microbial “Dark Matter” – Thousands of Unknown Bacterial Species Discovered in Hawaiian Lava Caves

Steve Smith in a Hawaiian cave passage filled with roots of the Kaʻu district on the Island of Hawai`i. Credit: Kenneth Ingham

Centuries-Old Lava Caves of Hawaiʻi Island Contain Thousands of Unknown Bacterial Species

Higher bacterial diversity than scientists expected has been uncovered in the lava caves, lava tubes, and geothermal vents on the big island of Hawaiʻi. The findings have been reported in a new study published today (July 21, 2022) in the journal Frontiers in Microbiology.

This research investigates the variety and interactions within these microbial ecosystems, which illustrate how life may have existed on

“This study points to the possibility that more ancient lineages of bacteria, like the phylum Chloroflexi, may have important ecological ‘jobs,’ or roles,” said first author Dr. Rebecca D Prescott of

Thick microbial mats hang under a rock ledge in steam vents that run along the Eastern Rift Zone on Hawaiʻi Island. Credit: Jimmy Saw

The harshest conditions—the geothermal sites—were expected to have lower diversity than the more established and habitable lava tubes. While the diversity was indeed found to be lower, the team of researchers was surprised to discover that the interactions within these communities were more complex than in locations with higher diversity.

“This leads to the question, do extreme environments help create more interactive microbial communities, with microorganisms more dependent on each other?” said Prescott. “And if so, what is it about extreme environments that helps to create this?”

Since Chloroflexi, and another class called Acidobacteria, were present at nearly all of the locations, they may play essential roles in these communities. However, these were not the most abundant bacteria, and the individual communities from the different sites showed large variations in the diversity and complexity of the microbial interactions. Counterintuitively, the most abundant groups, Oxyphotobacteria and Actinobacteria, were not often ‘hub’ species, suggesting that their roles may be less important to the overall structure of the community.

More questions than answers

Since the current study was based on the partial sequencing of one gene, it cannot accurately determine the species of microbes or their ‘jobs’ in the community. Therefore, further research is needed to help reveal the individual species that are present, as well as to better understand these bacteria’s roles in the environment.

A stalactite formation in a Hawaiian cave system from this study with copper minerals and white microbial colonies. Despite the fact that copper is toxic to many organisms, this formation hosts a microbial community. Credit: Kenneth Ingham

“Overall, this study helps to illustrate how important it is to study microbes in co-culture, rather than growing them alone (as isolates),” said Prescott. “In the natural world, microbes do not grow in isolation. Instead, they grow, live, and interact with many other microorganisms in a sea of chemical signals from those other microbes. This then can alter their gene expression, affecting what their jobs are in the community.”

Beyond the insights about past, or even future, life on Mars, bacteria from volcanic environments can also be useful in understanding how microbes turn volcanic rock (basalt) into soils, as well as bioremediation, biotechnology, and sustainable resource management.

Reference: “Islands Within Islands: Bacterial Phylogenetic Structure and Consortia in Hawaiian Lava Caves and Fumaroles” by Rebecca D. Prescott, Tatyana Zamkovaya, Stuart P. Donachie, Diana E. Northup, Joseph J. Medley, Natalia Monsalve, Jimmy H. Saw, Alan W. Decho, Patrick S. G. Chain and Penelope J. Boston, 21 July 2022, Frontiers in Microbiology.
DOI: 10.3389/fmicb.2022.934708

Funding: NASA Headquarters, George Washington University



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