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Ultraviolet Aurora Spotted on Comet 67P/Churyumov-Gerasimenko (Astronomy)

Using data from several instruments aboard ESA’s Rosetta mission, researchers have found evidence of far-ultraviolet aurora on comet 67P/Churyumov-Gerasimenko.

This false-color four-image mosaic comprises images taken from a distance of 28.7 km from the center of Comet 67P/Churyumov-Gerasimenko on 3 February 2015. The mosaic measures 4.2 x 4.6 km. Image credit: ESA / Rosetta / NAVCAM / CC BY-SA IGO 3.0.

The Rosetta spacecraft escorted comet 67P/Churyumov-Gerasimenko for more than two years.

The data for the current study is on what the Rosetta scientists initially interpreted as ‘dayglow,’ a process caused by photons interacting with the coma that radiates from, and surrounds, the comet’s nucleus.

But the new analysis of the Rosetta data paints a very different picture. By linking data from numerous Rosetta instruments, researchers were able to get a better picture of what was going on.

Source of the energetic electrons responsible for the far-ultraviolet (FUV) emissions at comet 67P/Churyumov-Gerasimenko: trajectories of solar-wind electrons inducing the FUV aurora around the comet; they undergo acceleration through the ambipolar electric field set up by the cometary plasma; the electron trajectories are shown with lines color-coded by energy and the ambipolar electric field acting on electrons is plotted with green arrows. Image credit: Galand et al, doi: 10.1038/s41550-020-1171-7.

This enabled them to unambiguously identify how 67P/Churyumov-Gerasimenko’s ultraviolet atomic emissions form. The data indicate 67P/Churyumov-Gerasimenko’s emissions are actually auroral in nature.

Electrons streaming out in the solar wind interact with the gas in the comet’s coma, breaking apart water and other molecules. The resulting atoms give off a distinctive far-ultraviolet light.

Invisible to the naked eye, far-ultraviolet has the shortest wavelengths of radiation in the ultraviolet spectrum.

Exploring the emission of 67P/Churyumov-Gerasimenko will enable the researchers to learn how the particles in the solar wind change over time, something that is crucial for understanding space weather throughout the Solar System.

By providing better information on how the Sun’s radiation affects the space environment they must travel through, such information could ultimately can help protect satellites and spacecraft, as well as astronauts traveling to the Moon and Mars.

References: M. Galand et al. Far-ultraviolet aurora identified at comet 67P/Churyumov-Gerasimenko. Nat Astron, published online September 21, 2020; doi: 10.1038/s41550-020-1171-7 link: https://www.nature.com/articles/s41550-020-1171-7

Cassini Finds Fresh Ice in Northern Hemisphere of Enceladus (Planetary Science)

Spectral data gathered by the Visual and Infrared Mapping Spectrometer (VIMS) onboard NASA’s Cassini spacecraft provide strong evidence that the northern hemisphere of Saturn’s moon Enceladus has been resurfaced with ice from its interior.

In these detailed infrared images of Enceladus, reddish areas indicate fresh ice that has been deposited on the surface. Image credit: NASA / JPL-Caltech / University of Arizona / LPG / CNRS / University of Nantes / Space Science Instituto.

Between 2004 and 2017, the VIMS instrument collected infrared data during 23 Enceladus close encounters, in addition to more distant surveys.

Dr. Gabriel Tobie, a researcher in the Laboratory of Planetology and Geodynamics at the University of Nantes, and colleagues used the VIMS data, combined with detailed images captured by Cassini’s Imaging Science Subsystem (ISS), to make the new global spectral map of Enceladus.

In 2005, the scientists discovered that Enceladus, which looks like a highly reflective, bright white snowball to the naked eye, shoots out enormous plumes of ice grains and vapor from an ocean that lies under the icy crust.

The new spectral map shows that infrared signals clearly correlate with that geologic activity, which is easily seen at the south pole.

That’s where the so-called ‘tiger stripes’ blast ice and vapor from the interior ocean.

But some of the same infrared features also appear in the northern hemisphere.

That tells the researchers not only that the northern area is covered with fresh ice but that the same kind of geologic activity — a resurfacing of the landscape — has occurred in both hemispheres.

The resurfacing in the north may be due either to icy jets or to a more gradual movement of ice through fractures in the crust, from the subsurface ocean to the surface.

“The infrared shows us that the surface of the south pole is young, which is not a surprise because we knew about the jets that blast icy material there,” Dr. Tobie said.

“Now, thanks to these infrared eyes, you can go back in time and say that one large region in the northern hemisphere appears also young and was probably active not that long ago, in geologic timelines.”

References: R. Robidel et al. 2020. Photometrically-corrected global infrared mosaics of Enceladus: New implications for its spectral diversity and geological activity. Icarus 349: 113848; doi: 10.1016/j.icarus.2020.113848

Hubble Spots Dark Matter-Rich Spiral Galaxy (Astronomy)

Astronomers using the NASA/ESA Hubble Space Telescope have captured a striking new photo of an unusual spiral galaxy called NGC 5585.

This Hubble image shows the spiral galaxy NGC 5585. Hotspots of star formation can be seen along the galaxy’s faint spiral arms. These regions shine a brilliant blue, contrasting strikingly against the ever-black background of space. The color image is made up of observations from Hubble’s Advanced Camera for Surveys (ACS) in the near-infrared and optical parts of the spectrum. Two filters were used to sample various wavelengths. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / R. Tully / Gagandeep Anand.

NGC 5585 is located approximately 25.5 million light-years away in the constellation of Ursa Major.

The galaxy was discovered on April 17, 1789 by the German-born British astronomer William Herschel.

It is a member of the M101 group, a bright group of nearly 10 galaxies dominated by the Pinwheel Galaxy, also known as Messier 101 (M101).

Also known as LEDA 51210 and UGC 9179, NGC 5585 has a diameter of roughly 35,000 light-years.

“NGC 5585 is more than it appears,” the Hubble astronomers said.

“The many stars and dust and gas clouds that make up this galaxy contribute only a small fraction of its total mass.”

“As in many galaxies, this discrepancy can be explained by the abundant yet seemingly invisible presence of dark matter.”

“When compared with galaxies of a similar shape and size, NGC 5585 stands out by having a notably different composition,” they explained.

“Contributing to the total mass of the galaxy, it contains a far higher proportion of dark matter.”

Astronomers Find Two Massive Exoplanets In Nearby Binary System (Astronomy)

Astronomers presented the discovery of two planets orbiting the nearby (D=11.9 pc) K7 dwarf Gl 414A.

An artist’s impression of the Gliese 414 system.

Gliese 414 is located approximately 39 light-years away in the constellation of Ursa Major.

Also known as GJ 414, HD 97101 or HIP 54646, the system is 12.4 billion years old.

It consists of a relatively active K7V-type dwarf star, Gliese 414A, and its smaller M2V-type dwarf companion, Gliese 414B.

The physical separation between the two stars is around 408 AU (astronomical units).

The two newfound exoplanets, named Gliese 414Ab and c, orbit the larger star in the system.

The inner planet is a sub-Neptune in a 50.8-day eccentric orbit.

It is 2.95 times the size of Earth, 8.8 times as massive, and has a temperature of around 31 degrees Celsius (88 degrees Fahrenheit).

The outer planet is a sub-Saturn in a nearly circular orbit with an orbital period of 748.3 days.

It is 8.8 times the size of Earth, 56.3 times as massive, and has a temperature of minus 150 degrees Celsius (minus 238 degrees Fahrenheit).

The planets were found using radial velocity data from the HIRES instrument on the Keck I telescope at W.M. Keck Observatory and the Automated Planet Finder at Lick Observatory, as well as photometric data from KELT-North telescope at Winer Observatory.

Gliese 414Ac resides near the inner edge of the star’s habitable zone, but its minimum mass is large enough that it likely possesses a substantial volatile-rich envelope. This planet is a potential candidate for future direct imaging missions.

References: Cayla M. Dedrick et al. 2020. Two Planets Straddling the Habitable Zone of The Nearby K dwarf Gl 414A. AJ, in press; arXiv: 2009.06503

Neuroscience Study Finds ‘Hidden’ Thoughts In Visual Part Of Brain (Neuroscience)

How much control do you have over your thoughts? What if you were specifically told not to think of something—like a pink elephant?

Participants used the left side of their brains to come up with the thought, and the right side to try and suppress it.

A recent study led by UNSW psychologists has mapped what happens in the brain when a person tries to suppress a thought. The neuroscientists managed to ‘decode’ the complex brain activity using functional brain imaging (called fMRI) and an imaging algorithm.

Their findings suggest that even when a person succeeds in ignoring a thought, like the pink elephant, it can still exist in another part of the brain—without them being aware of it.

In their study they tracked the brain activity in 15 participants as they completed several visualizations and thought suppression exercises. Participants were given a written prompt—either green broccoli or a red apple—and challenged not to think of it. To make this task even harder, they were asked to not replace the image with another thought.

After 12 seconds, participants confirmed whether they were able to successfully suppress the image or if the thought suppression failed. Eight people were confident they’d successfully suppressed the images—but their brain scans told a different story. They found that visual cortex—the part of the brain responsible for mental imagery—seemed to be producing thoughts without their awareness.

Brain neurons fired and then pulled oxygen into the blood each time a thought took place. This movement of oxygen, which was measured by the fMRI machine, created particular spatial patterns in the brain.

The researchers decoded these spatial patterns using an algorithm called multivoxel pattern analysis (MVPA). MVPA is a type of decoding algorithm based in machine learning that allows us to read thoughts. The algorithm could distinguish brain patterns caused by the vegetable/fruit prompts.

Eight study participants were confident they’d successfully suppressed the images of the red apple or green broccoli, but their brain scans suggested otherwise. Credit: Shutterstock

The scans showed that participants used the left side of their brains to come up with the thought, and the right side to try and suppress it. Prof. Pearson hopes this functional brain mapping will help future researchers know which areas of the brain to target for potential intrusive thought therapies. This study can help explain why forcefully trying not to think about something always fails. For example, for someone trying to quit smoking, trying not to think about having a cigarette is a very bad strategy.

These findings build on a behavioral study Prof. Pearson’s team at UNSW Science’s Future Minds Lab conducted last year, which tested how suppressed thoughts can influence perception.

They know that you can have conscious and unconscious perception in your visual cortex—for example, they can show someone an image of a spider, make the image invisible, but their brain will still process it. But until now, they didn’t know this also worked with thoughts.

Both studies point towards the elusive world of the “unconscious,” which Prof. Pearson plans to explore in his future work.

They’re interested in this idea that imagination can be unconscious—that these thoughts can appear and influence our behavior, without us even noticing. More evidence is starting to suggest unconscious thoughts do occur, and they can decode them.

References: Roger Koenig-Robert et al. Decoding Nonconscious Thought Representations during Successful Thought Suppression, Journal of Cognitive Neuroscience (2020). DOI: 10.1162/jocn_a_01617

We Now Know, How COVID-19 Trigger Fatal Levels Of Lung Inflammation (Medicine)

A hallmark of severe COVID-19 pneumonia is SARS-CoV-2 infection of the facultative progenitors of lung alveoli, the alveolar epithelial type 2 cells (AT2s). However, inability to access these cells from patients, particularly at early stages of disease, limits an understanding of disease inception.

Now, a team of infectious disease, pulmonary and regenerative medicine researchers at Boston University, studying human stem cell-derived lung cells called type 2 pneumocytes, infected with SARS-CoV-2, have shown that the virus initially suppresses the lung cells’ ability to call in the help of the immune system with interferons to fight off the viral invaders and instead activates an inflammatory pathway called NFkB.

According to the researchers, the inflammatory signals initiated by the infected pneumocytes attract an army of immune cells into lung tissue laden with infected and already dead and dying cells. Their data confirms that SARS-CoV-2 blocks cells from activating one of the anti-viral branches of the immune system early on after infection has set in. The signal the cells would typically send out, a tiny protein called interferon that they exude under threat of disease, are instead delayed for several days, giving SARS-CoV-2 plenty of time to spread and kill cells, triggering a buildup of dead cell debris and other inflammation.

References: Jessie Huang et al. SARS-CoV-2 Infection of Pluripotent Stem Cell-derived Human Lung Alveolar Type 2 Cells Elicits a Rapid Epithelial-Intrinsic Inflammatory Response, Cell Stem Cell (2020). DOI: 10.1016/j.stem.2020.09.013

Researchers Discovered Potential Cause Of Immunotherapy-Related Neurotoxicity (Neuroscience)

New research has uncovered the previously unknown presence of CD19—a B cell molecule targeted by chimeric antigen receptor (CAR) T cell immunotherapy to treat leukemia, lymphoma, and multiple myeloma—in brain cells that protect the blood brain barrier (BBB).

This discovery may potentially be the cause for neurotoxicity in patients undergoing CD19 directed CAR T cell immunotherapy, according to the research team led by Avery Posey, Ph.D., an assistant professor of Systems Pharmacology and Translational Therapeutics in the Perelman School of Medicine at the University of Pennsylvania and Research Health Science Specialist at the Corporal Michael J. Crescenz VA Medical Center in Philadelphia, PA. The study was published today in Cell.

“Our work has revealed that there is CD19 expression in a subset of cells that are, one, not B cells, and two, potentially related to the neurotoxicity we observe in patients treated with CAR T cell therapy targeting CD19,” Posey said. “The next question is, can we identify a better target for eliminating B cell related malignancies other than CD19, or can we engineer around this brain cell expression of CD19 and build a CAR T cell that makes decisions based on the type of cell it encounters—for instance, CAR T cells that kill the B cells they encounter, but spare the CD19 positive brain cells?”

As so often happens in scientific endeavors, the path to this discovery was made somewhat by chance. Kevin Parker, a Ph.D. student at Stanford and co-author on the paper, was at home analyzing previously published single cell sequencing data sets in his spare time. He found CD19 expression in a data set of fetal brain samples that looked odd, because the accepted wisdom was that CD19 only existed in B cells. So his lab reached out to the pioneers of CAR T cell immunotherapy, Penn Medicine.

“I suggested we test this as a preclinical model. When we treated the mouse model with CAR T cells targeting the mouse version of CD19, we found what looks like the start of neurotoxicities,” Posey said.

The team observed an increase in BBB permeability when mouse CD19 was targeted by CAR T cells, even in mice that lack B cells, but not when human CD19 was targeted as a control treatment (mice do not express human CD19).

“Even more interesting, this BBB permeability was more severe when the CAR T cells were fueled by a costimulatory protein called CD28 than when the CAR T cells used 4-1BB,” Posey said “This difference in the severity of BBB permeability correlates with what we know about the clinical observations of CAR T cell-related neurotoxicities—the frequency of patients experiencing high-grade neurotoxicity is lower for those that received the 4-1BB-based CAR T cells.”

His team sought to investigate the higher incidence of neurotoxicity in CD19-directed immunotherapies, compared to treatments targeting other B cell proteins, such as CD20. Notably, CD19 CAR T cells are sensitive to even low levels of CD19 antigen density, emphasizing the importance of identifying any potential reservoir of CD19 other than B cells.

The researchers’ discovery of CD19 molecules in the brain provides evidence that this increase in neurotoxicity is due to CD19-directed CAR T cell immunotherapies. Posey said, though, that generally this neurotoxicity is temporary and patients recover.

This research also highlights the potential utility of developing a comprehensive human single-cell atlas for clinical medicine. Sequencing is an unbiased, genome-wide measurement of gene expression that can capture even rare populations of cells. These rare cell types might otherwise be missed in measurements of bulk tissue due to their low frequency, but as this study demonstrates could be critically important in understanding the clinical effects of targeted therapy. While current CAR T cells recognize only a single antigen, future generations of CAR T cells may be able to discriminate between unique combinations of target antigens to improve thei

r cell-type specificity. The researchers envision that a comprehensive database of gene expression across all human cell types will enable the precise identification of cell type-specific target antigens which can be used to design safe and effective cellular immunotherapies.

“That’s what we think one of the biggest take-home messages is,” Posey said. “The incredible usefulness of single cell atlas or single cell sequencing technology to determine whether a potential immunotherapy or drug target is going to be present somewhere in the body that we would not normally expect it based on conventional thought and whether this expression may lead to toxicity.”

CD19 is thought to be a lineage-restricted molecule—behaving in a functionally and structurally limited way. But this study shows that some small percentage of brain cells also express CD19.

“We would not have identified that through bulk sequencing, where we’re looking at a population of cells versus a single cell type,” Posey said. “It’s only through single cell sequencing that we’re able to identify that there’s this very small percentage of cells in the brain that also contain this molecule, contrary to popular thought.”

References: Kevin R. Parker et al. Single-Cell Analyses Identify Brain Mural Cells Expressing CD19 as Potential Off-Tumor Targets for CAR-T Immunotherapies. Cell. Published: September 21, 2020. DOI:doi.org/10.1016/j.cell.2020.08.022 link: https://www.cell.com/cell/fulltext/S0092-8674(20)31013-8?_returnURL=https%3A%2F%2Flinkinghub.elsevier.com%2Fretrieve%2Fpii%2FS0092867420310138%3Fshowall%3Dtrue

How To Make A Replication Origin In Multicellular Eukaryotes? (Biology)

Loading of replicative helicases onto DNA is a key event during the initiation of chromosomal DNA replication. It takes place at specific chromosomal regions termed origins and is facilitated by the ORC protein complex. By resolving the cryo-EM structures of DNA-bound ORC, researchers from the Bleichert group (now at Yale) broaden our understanding of how DNA replication is initiated in animals.

Accurate replication of chromosomal DNA is essential for the survival and propagation of living organisms. Prior to cell division, many different proteins work together and duplicate genomes by semi-conservative replication so that copied chromosomes can be segregated into daughter cells. Genome integrity is sustained by highly efficient and accurate DNA replication exactly once per cell cycle. Failure to replicate DNA precisely can alter gene copy number and chromosome ploidy, which can give rise to genomic instability and a variety of human diseases.

Eukaryotic DNA replication initiation relies on the origin recognition complex (ORC), a DNA-binding ATPase that loads the Mcm2–7 replicative helicase onto replication origins. In yeast, origins are defined by a conserved consensus sequence that is recognized by ORC. By contrast, how replication origins are defined in animals (or metazoans) has remained unclear, but chromatin cues and local DNA structure are thought to help mediate the recognition of the origins. In a new paper, researchers reported cryo-electron microscopy (cryo-EM) structures of DNA-bound Drosophila ORC with and without the co-loader Cdc6.

These structures reveal that Orc1 and Orc4 constitute the primary DNA binding site in the ORC ring and cooperate with the winged-helix domains to stabilize DNA bending. A loop region near the catalytic Walker B motif of Orc1 directly contacts DNA, allosterically coupling DNA binding to ORC’s ATPase site.

Correlating structural and biochemical data showed that DNA sequence modulates DNA binding and remodeling by ORC, and that DNA bending promotes Mcm2–7 loading in vitro. Together, these findings explain the distinct DNA sequence-dependencies of metazoan and S. cerevisiae initiators in origin recognition and support a model in which DNA geometry and bendability contribute to Mcm2–7 loading site selection in metazoans.

References: Schmidt, J.M., Bleichert, F. Structural mechanism for replication origin binding and remodeling by a metazoan origin recognition complex and its co-loader Cdc6. Nat Commun 11, 4263 (2020). https://doi.org/10.1038/s41467-020-18067-7 link: https://www.nature.com/articles/s41467-020-18067-7

If There Is Life On Venus, How Could It Have Got There? Origin Of Life Experts Explain (Astronomy)

The recent discovery of phosphine in the atmosphere of Venus is exciting, as it may serve as a potential sign of life (among other possible explanations).

Credit: Shutterstock

The researchers, who published their findings in Nature Astronomy, couldn’t really explain how the phosphine got there.

They explored all conceivable possibilities, including lightning, volcanoes and even delivery by meteorites. But each source they modeled couldn’t produce the amount of phosphine detected.

Most phosphine in Earth’s atmosphere is produced by living microbes. So the possibility of life on Venus producing phosphine can’t be ignored.

But the researchers, led by UK astronomer Jane Greaves, say their discovery “is not robust evidence for life” on Venus. Rather, it’s evidence of “anomalous and unexplained chemistry,” of which biological processes are just one possible origin.

If life were to exist on Venus, how could it have come about? Exploring the origins of life on Earth might shed some light.

The ingredients for life (as we know it)

Understanding how life formed on Earth not only helps us understand our own origins, but could also provide insight into the key ingredients needed for life, as we know it, to form.

The details around the origins of life on Earth are still shrouded in mystery, with multiple competing scientific theories. But most theories include a common set of environmental conditions considered vital for life. These are:

Venus has 90 times the atmospheric pressure of Earth. Credit: NASA

Liquid water

Water is needed to dissolve the molecules needed for life, to facilitate their chemical reactions. Although other solvents (such as methane) have been suggested to potentially support life, water is most likely. This is because it can dissolve a huge range of different molecules and is found throughout the universe.

Mild temperatures

Temperatures higher than 122℃ destroy most complex organic molecules. This would make it almost impossible for carbon-based life to form in very hot environment.

A process to concentrate molecules

As the origin of life would have required a large amount of organic molecules, a process to concentrate organics from the diluted surrounding environment would be required—either through absorption onto mineral surfaces, evaporation or floating on top of water in oily slicks.

A complex natural environment

For life to have originated, there would have had to be a complex natural environment wherein a diverse range of conditions (temperature, pH and salt concentrations) could create chemical complexity. Life itself is incredibly complex, so even the most primitive versions would need a complex environment to originate.

Trace metals

A range of trace metals, amassed through water-rock interactions, would be needed to promote the formation of organic molecules.

So if these are the conditions required for life, what does that tell us about the likelihood of life forming on Venus?

This is a computer-generated picture of the Eistla Regio region on Venus’s surface. Credit: NASA

It’s unlikely today …

The possibility of life as we know it forming on the surface of present-day Venus is incredibly low. An average surface temperature above 400℃ means the surface can’t possibly have liquid water and this heat would also destroy most organic molecules.

Venus’s milder upper atmosphere, however, has temperatures low enough for water droplets to form and thus could potentially be suitable for the formation of life.

That said, this environment has its own limitations, such as clouds of sulfuric acid which would destroy any organic molecules not protected by a cell. For example, on Earth, molecules such as DNA are rapidly destroyed by acidic conditions, although some bacteria can survive in extremely acidic environments.

Also, the constant falling of water droplets from Venus’s atmosphere down to its extremely hot surface would destroy any unprotected organic molecules in the droplets.

Beyond this, with no surfaces or mineral grains in the Venusian atmosphere on which organic molecules could concentrate, any chemical building blocks for life would be scattered through a diluted atmosphere—making it incredibly difficult for life to form.

… but possibly less unlikely in the past

Bearing all this in mind, if atmospheric phosphine is indeed a sign of life on Venus, there are three main explanations for how it could have formed.

Life may have formed on the planet’s surface when its conditions were very different to now.

Modeling suggests the surface of early Venus was very similar to early Earth, with lakes (or even oceans) of water and mild conditions. This was before a runaway greenhouse effect turned the planet into the hellscape it is today.

If rocks from Earth containing microbial life entered Venus’s orbit in the past, this life may have adapted to Venus’s atmospheric conditions. Credit: Shutterstock

If life formed back then, it might have adapted to spread into the clouds. Then, when intense climate change boiled the oceans away—killing all surface-based life—microbes in the clouds would have become the last outpost for life on Venus.

Another possibility is that life in Venus’s atmosphere (if there is any) came from Earth.

The planets of our inner solar system have been documented to exchange materials in the past. When meteorites crash into a planet, they can send that planet’s rocks hurtling into space where they occasionally intersect with the orbits of other planets.

If this happened between Earth and Venus at some point, the rocks from Earth may have contained microbial life that could have adapted to Venus’s highly acidic clouds (similar to Earth’s acid-resistant bacteria).

A truly alien explanation

The third explanation to consider is that a truly alien form of life (life as we don’t know it) could have formed on Venus’s 400℃ surface and survives there to this day.

Such a foreign life probably wouldn’t be carbon-based, as nearly all complex carbon molecules break down at extreme temperatures.

Although carbon-based life produces phosphine on Earth, it’s impossible to say only carbon-based life can produce phosphine. Therefore, even if totally alien life exists on Venus, it may produce molecules that are still recognizable as a potential sign of life.

It’s only through further missions and research that we can find out whether there is, or was, life on Venus. As prominent scientist Carl Sagan once said: “extraordinary claims require extraordinary evidence.”

Luckily, two of the four finalist proposals for NASA’s next round of funding for planetary exploration are focused on Venus.

These include VERITAS, an orbiter proposed to map the surface of Venus, and DAVINCI+, proposed to drop through the planet’s skies and sample different atmospheric layers on the way down.

This article is republished from The Conversation under a Creative Commons license.