New metallic blue ant species found in India by entomologists

The entomologist described a new species of ant. Parapara Tretina He is from Inguk village in the East Siang district of Arunachal Pradesh in northeastern India.

Paraparatretina NeelaHolotype worker: (A) Head viewed from the front, (B) Body viewed from the back, (C) Body viewed from the side. Images courtesy of Sahanashree other., doi: 10.3897/zookeys.1203.114168.

Parapara Tretina A genus of small ants, generally 1-2 mm in length, belonging to the subfamily. Formicidae.

They are typically found in the Afrotropical, Australasia, Indomalaya, Oceania and Palaearctic biogeographical regions.

They live in a variety of tropical environments, from rainforests to forest clearings, and can be found in a wide range of habitats, from leaf litter on the ground to high up in the tree canopy.

Currently, the genus contains 38 valid species and four valid subspecies.

Fourteen species are known from the Indomalaya biogeographic region. Parapara Tretina Acetate It was previously the only species known from the Indian subcontinent.

Specimen of a new worker ant species Parapara Tretina The specimens were collected from a secondary forest at an altitude of 803 metres (2,635 feet) in Ing village, East Siang district, Arunachal Pradesh, northeastern India.

“One evening, while I was exploring a tree hole about three metres high on a steep cattle track in the remote village of Inku, I saw something glow in the twilight,” he said. Dr. Dharma Rajan Priyadarsanan Ashoka Foundation for Ecological and Environmental Research and colleagues.

“In the dim light, two insects were sucked into the aspirator, which, to my surprise, I later discovered were ants.”

“Arunachal Pradesh, located in the Himalayan biodiversity hotspot, Cyan Valley “There is a world of unparalleled diversity, much of which remains to be explored,” they said.

“But this richness, both culturally and ecologically, faces unprecedented threats.”

“Large infrastructure projects such as dams, highways and military installations, along with climate change, are rapidly transforming the valley.”

“The impacts extend beyond the valley itself, as these mountains not only sustain their own diverse ecosystems but also play a vital role in ensuring the well-being of millions of people living downstream.”

Named Paraparatretina NeelaThe newly discovered species is a tiny ant measuring less than 2mm in length.

The body is primarily metallic blue, except for the antennae, mandibles, and legs.

The head is subtriangular, with large eyes and triangular mouthparts (mandible) bearing five teeth.

This species has a distinctive metallic blue colour that distinguishes it from other species in the genus.

“With the exception of marine sponges, blue colouration in animals is a relatively rare phenomenon,” the researchers said.

“But there are also some blue species among vertebrates, such as fish, frogs and birds, and invertebrates, such as spiders.”

“Blue is a common color in many insects, especially hymenoptera. Apidae, Chrysanthemum family and Ichneumonidaeit is very rare Formicidae. “

“Blue colors in insects are typically produced by the arrangement of biological photonic nanostructures rather than pigments, and have evolved independently in different groups.”

“This vibrant feature raises an intriguing question: Could it serve a purpose in communication, camouflage, or other ecological interactions? A closer look at the evolution of this conspicuous color and its relationship to elevation and biology could provide clues.” Paraparatretina Neela It points to exciting avenues for research.”

Discovery Paraparatretina Neela It has been reported paper In the journal Zookie.

_____

R. Sahanashree other2024. Amazing new species Parapara Tretina Donisthorpe (1947) (Hymenoptera, Formicidae, Formicinae), from the Eastern Himalayas of India. Zookie 1203: 159-172; doi: 10.3897/zookeys.1203.114168

Source: www.sci.news

VLT spots metallic scar on surface of white dwarf

A dynamically active planetary system orbits a significant portion of the white dwarf. These stars often exhibit surface metals accreted from a disk of debris. However, the complete journey of a planetesimal from its star-grazing orbit to its final dissolution in its host star is poorly understood. In a new paper, Astrophysics Journal Letter astronomers report the discovery that stars exist that are contaminated with cold metals. WD 0816-310 It cannibalized heavy elements from a planetary body as large as the dwarf planet Vesta.

WD 0816-310 is a magnetic white dwarf star located 63 light-years away in the constellation Papis. Image credit: L. Calçada / ESO.

Dr Stefano Vanullo, an astronomer at the Armagh Observatory and Planetarium, said: 'It is common for some white dwarfs – slowly cooling embers of stars like our Sun – to cannibalize parts of planetary systems. known,” he said.

“Now we find that the star's magnetic field plays a key role in this process, causing scars on the white dwarf's surface.”

The metal signatures the researchers observed on WD 0816-310 are concentrations of metal imprinted on the white dwarf's surface.

Professor Jay Farihi of University College London said: “These metals come from fragments of a planet the size of, or possibly even larger than, Vesta, which at about 500 kilometers in diameter is the second largest asteroid in the solar system. I have proven that.”

To observe WD 0816-310, astronomers FORS2 equipment upon ESO's super large telescope (VLT).

They also relied on archival data from VLT. X shooter instrument This is to confirm the survey results.

The authors noticed that the strength of the metal detections changed as the star rotated, indicating that the metals were concentrated in specific areas on the white dwarf's surface, rather than being spread smoothly across the surface. Suggests.

They also found that these changes were synchronized with changes in the white dwarf's magnetic field, indicating that this metallic scar is located at one of its magnetic poles.

Taken together, these clues indicate that the magnetic field funneled metal into the star, creating the scar.

“Surprisingly, the material was not evenly mixed on the star's surface, as theory predicted. Instead, this scar was a concentrated patch of planetary material that guided falling debris. “We've never seen anything like this before,” said John Landstreet, a professor at Western University.

“ESO offers a unique combination of capabilities needed to observe faint objects like white dwarfs and make sensitive measurements of the star's magnetic field,” Vanullo said.

_____

Stefano Vanullo other. 2024. Discovery of magnetically induced metal accretion on contaminated white dwarfs. APJL 963, L22; doi: 10.3847/2041-8213/ad2619

Source: www.sci.news

Bizarre White Dwarf Leaves Metallic Marks Following Consumption of Planet

Artist’s impression of WD 0816-310. Astronomers have discovered scars imprinted on the surface left when a star swallows a planet.

ESO/L. Calzada

Astronomers have discovered a white dwarf star with strange metallic scars on its surface. The scar likely formed when the star tore apart and ate a small planet in its orbit.

Researchers often find white dwarfs with traces of metal in their atmospheres that came from planets that fell into the star. It has long been thought that metals should be evenly distributed across the surfaces of these so-called contaminated white dwarfs; Jay Farihi Researchers at University College London have discovered a strange concentration of metal debris.

Researchers monitored the star, called WD 0816-310, for two months using the Very Large Telescope in Chile. They discovered that the white dwarf had an opaque piece of metal on top of one of its magnetic poles, blocking some of the star’s light as it rotated. This position indicates that material may have been funneled into the star by its magnetic field. “This is the same process that causes auroras on Earth: charged particles follow magnetic fields to the surface,” Farihi said.

The planet that WD 0816-310 destroyed was small, probably about the same size as the solar system’s asteroid Vesta, which is about 525 kilometers in diameter. Its interior is now prominently displayed on its host star, which could make it relatively easy to study what its geochemistry was like before it was engulfed. Such studies may even be one of the best ways to observe small worlds outside our solar system, even after they disappear.

And there may be many other stars that have been similarly damaged. “When we find something outlandish, it’s often because they all looked that way and we just weren’t asking the right questions,” Farihi says. “This is the first, but it probably won’t be the last.” In fact, researchers have already discovered two white dwarfs that appear to have similar scars. If we go back and observe similar stars over and over again, we may discover even more stars.

topic:

Source: www.newscientist.com