Science & Technology
Over this weekend, two asteroids - 2020 MU1 (120ft diameter or half the wingspan of a 747 jet) and 2020 ML (73ft diameter, roughly half the height of the Arc de Triomphe in Paris) - are expected to shoot past us at a distance of 4.4 million and 2.7 million miles respectively.
Lest anyone get too comfortable and breathe a sigh of relief, however, NASA warns that a further three space rocks are expected in these parts next week.
The discovery was made by a Yutu 2 drive team member in July 2019, during lunar day 8 of the rover's mission, which is part of China's Chang'e 4 mission to explore the far side of the moon. A report by Our Space, a Chinese-language science-outreach publication, revealed the discovery on Aug. 17 and described the substance using the term "胶状物" ("jiao zhuang wu"), which can be translated as "gel-like."
This description, along with the initial absence of images, sparked wide interest as well as speculation among lunar scientists.
However the substance is, as expected by scientists, made up of rock. In their article in "Earth and Planetary Science Letters", Gou Sheng and colleagues analyzed data from Yutu 2's panoramic and hazard avoidance cameras, and the rover's Visible and Near-Infrared Spectrometer (VNIS) instrument.

The tropics are the birthplace of most rosids, a massive group of flowering plants that includes this hibiscus, a member of the mallow family. But researchers found new rosid species are evolving in temperate zones twice as quickly as the tropics, a finding that challenges a longstanding hypothesis.
The tropics are the birthplace of most species of rosids, a group that makes up more than a quarter of flowering plants, ranging from mangroves to roses to oaks. But in an analysis of about 20,000 rosid species, researchers found the speed of tropical rosid evolution lags far behind that of younger communities in temperate habitats.
Although rosids originated 93-115 million years ago, the rate at which the group diversified, or formed new species, dramatically increased over the last 15 million years, a period of global cooling and expanding temperate habitats. Today, rosids are diversifying far faster in places such as the southeastern U.S. than in equatorial rainforests, said study co-lead author Ryan Folk, assistant professor of biological sciences and herbarium curator at Mississippi State University.

An image of the near side of the moon based on data from NASA's Lunar Reconnaissance Orbiter.
NASA's prolific Lunar Reconnaissance Orbiter (LRO) found rich evidence of iron and titanium oxides under the surface of the moon, which may show a close connection with Earth's early history.
Scientists have been debating how the moon formed for decades. The leading theory suggests that a Mars-size world collided with Earth billions of years ago. The colliding world shattered upon impact and blasted part of the proto-Earth's surface into space. The debris surrounded Earth with a ring; the moon we see today is the result of that ring slowly collapsing under its own gravity.
The moon's chemical composition, however, doesn't show clear evidence of that theory. The lunar highlands on the moon, visible from the Earth as bright regions, have rocks with smaller amounts of metal-bearing minerals relative to our planet.

Supernova 2020nlb in the galaxy M85 in Virgo was a 17th-magnitude blip at discovery but has grown brighter each night. Now at magnitude 12.2 (July 7th), it's bright enough to see in a 6-inch telescope. M85's supernova is currently almost a full magnitude brighter than the 13.1-magnitude field star immediately to its northeast. The supernova sits 1.0″ east and 43.2″ north of the core. North is up.
The first of the pair, dubbed 2020nlb, was discovered by the Asteroid Terrestrial-impact Last Alert System (ATLAS) on June 25th in the 10th-magnitude galaxy M85. Located in Coma Berenices 60 million light-years from Earth, M85 is an elliptical galaxy a quarter again as large our Milky Way. The "M" stands for Charles Messier, an 18th century French astronomer who compiled a list of galaxies, star clusters and nebulae he stumbled on during searches for his favorite prey, comets.

NGC 7789, also known as Caroline's Rose, is an old open star cluster of the Milky Way, which lies about 8,000 light-years away toward the constellation Cassiopeia. It hosts a few White Dwarfs of unusually high mass, analyzed in this study.
Findings from a study published today in Nature Astronomy show that the final breaths of these dying stars, called white dwarfs, shed light on carbon's origin in the Milky Way.
"The findings pose new, stringent constraints on how and when carbon was produced by stars of our galaxy, ending up within the raw material from which the Sun and its planetary system were formed 4.6 billion years ago," says Jeffrey Cummings, an Associate Research Scientist in the Johns Hopkins University's Department of Physics & Astronomy and an author on the paper.

NGC 7789, also known as Caroline's Rose, is an old open star cluster of the Milky Way, which lies about 8,000 light-years away toward the constellation Cassiopeia. It hosts a few white dwarfs of unusually high mass that were analyzed in this study.
Approximately 90 percent of all stars end their lives as white dwarfs, very dense stellar remnants that gradually cool and dim over billions of years. With their final few breaths before they collapse, however, these stars leave an important legacy, spreading their ashes into the surrounding space through stellar winds enriched with chemical elements, including carbon, newly synthesized in the star's deep interior during the last stages before its death.
Every carbon atom in the universe was created by stars, through the fusion of three helium nuclei. But astrophysicists still debate which types of stars are the primary source of the carbon in our own galaxy, the Milky Way. Some studies favor low-mass stars that blew off their envelopes in stellar winds and became white dwarfs, while others favor massive stars that eventually exploded as supernovae.
In the new study, published July 6 in Nature Astronomy, an international team of astronomers discovered and analyzed white dwarfs in open star clusters in the Milky Way, and their findings help shed light on the origin of the carbon in our galaxy. Open star clusters are groups of up to a few thousand stars, formed from the same giant molecular cloud and roughly the same age, and held together by mutual gravitational attraction. The study was based on astronomical observations conducted in 2018 at the W. M. Keck Observatory in Hawaii and led by coauthor Enrico Ramirez-Ruiz, professor of astronomy and astrophysics at UC Santa Cruz.
Their study gives new insight into the swirling flow of iron 2800 kilometers below the planet's surface and how it has influenced the movement of the magnetic field during the past hundred thousand years.
Our magnetic field is generated and maintained by a convective flow of molten metal that forms the Earth's outer core. Motion of the liquid iron creates the electric currents that power the field, which not only helps guide navigational systems but also helps shield us from harmful extra terrestrial radiation and hold our atmosphere in place.
Anyone scared of snakes on the ground may not want to read this story — because the reptiles are also in the sky.
The paradise snake, which is native to south and southeast Asia, has been known to scientists for some time. But they never really understood how the species — and others like it — are able to glide through the air.
Researchers at Virginia Tech conducted controlled tests with the snakes in an indoor environment.
Comment: Another fascinating take on the paradise snake
- Misapplying information theory.
- Misinterpreting research related to protein rarity.
- Misunderstanding the creative potential of evolutionary processes.
Skeptics of information-based design arguments typically misunderstand the nature of biological information (see here and here). For instance, one physicist, Randy Isaac, stated the following:
We first note that, from a thermodynamics perspective, living cells are dynamic, open systems that continually exchange energy, entropy, and information with their surrounding environment...Thus there is plenty of opportunity for information to be transformed from one variable to another, from various physical states to useful information-bearing variables. Information in a cell is not conserved, just as entropy is not conserved in an open system.His analysis reveals a common confusion between what is termed the Shannon measure of information and semantic information (more generally, specified complexity).











Comment: See also:
- Biologists call to overhaul flawed taxonomic categories
- Why Darwinism Is Wrong, Dead Wrong - Part 1: Intelligent Design and Information
- Darwinism, Creationism... How About Neither?
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