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The International Space Station (ISS) was thrown briefly out of control on Thursday when jet thrusters of a newly arrived Russian research module inadvertently fired a few hours after it was docked to the orbiting outpost, NASA officials said.

The seven crew members aboard – two Russian cosmonauts, three NASA astronauts, a Japanese astronaut, and a European space agency astronaut from France – were never in any immediate danger, according to NASA and Russian state-owned news agency RIA.

But the malfunction prompted NASA to postpone until at least August 3 its planned launch of Boeing’s new CST-100 Starliner capsule on a highly anticipated uncrewed test flight to the space station. The Starliner had been set to blast off atop an Atlas V rocket on Friday from the Kennedy Space Center in Florida.

Thursday’s mishap began about three hours after the multipurpose Nauka module had latched onto the space station, as mission controllers in Moscow were performing some post-docking “reconfiguration” procedures, according to NASA.

The module’s jets inexplicably restarted, causing the entire station to pitch out of its normal flight position some 250 miles above the Earth, leading the mission’s flight director to declare a “spacecraft emergency,” US space agency officials said.

An unexpected drift in the station’s orientation was first detected by automated ground sensors, followed 15 minutes later by a “loss of attitude control” that lasted a little over 45 minutes, according to Joel Montalbano, manager of NASA’s space station programme.

‘Tug-of-war’

Flight teams on the ground managed to restore the space station’s orientation by activating thrusters on another module of the orbiting platform, NASA officials said.

In its broadcast coverage of the incident, RIA cited NASA specialists at the Johnson Space Center in Houston, Texas, as describing the struggle to regain control of the space station as a “tug of war” between the two modules.

At the height of the incident, the station was pitching out of alignment at the rate of about a half a degree per second, Montalbano said during a NASA conference call with reporters.

The Nauka engines were ultimately switched off, the space station was stabilised and its orientation was restored to where it had begun, NASA said.

Communication with the crew was lost for several minutes twice during the disruption, but “there was no immediate danger at any time to the crew,” Montalbano said. He said “the crew really didn’t feel any movement.”

Had the situation become so dangerous as to require evacuation of personnel, the crew could have escaped in a SpaceX crew capsule still parked at the outpost and designed to serve as a “lifeboat” if necessary, said Steve Stich, manager of NASA’s commercial crew programme.

What caused the malfunction of the thrusters on the Nauka module, delivered by the Russian space agency Roscosmos, has yet to be determined, NASA officials said.

Montalbano said there was no immediate sign of any damage to the space station. The flight correction maneuvres used up more propellant reserves than desired, “but nothing I would worry about,” he said.

After its launch last week from Kazakhstan’s Baikonur Cosmodrome, the module experienced a series of glitches that raised concern about whether the docking procedure would go smoothly.

Roscosmos attributed Thursday’s post-docking issue to Nauka’s engines having to work with residual fuel in the craft, TASS news agency reported.

“The process of transferring the Nauka module from flight mode to ‘docked with ISS’ mode is underway. Work is being carried out on the remaining fuel in the module,” Roscosmos was cited by TASS as saying.

The Nauka module is designed to serve as a research lab, storage unit, and airlock that will upgrade Russia’s capabilities aboard the ISS.

A live broadcast showed the module, named after the Russian word for “science,” docking with the space station a few minutes later than scheduled.

“According to telemetry data and reports from the ISS crew, the onboard systems of the station and the Nauka module are operating normally,” Roscosmos said in a statement.

“There is contact!!!” Dmitry Rogozin, the head of Roscosmos, wrote on Twitter moments after the docking.

© Thomson Reuters 2021


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CERN’s LHCb Detects First CP Violation in Baryons, Shedding Light on Matter–Antimatter Puzzle

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CERN’s LHCb Detects First CP Violation in Baryons, Shedding Light on Matter–Antimatter Puzzle

The researchers used the LHCb detector at the Large Hadron Collider in CERN for the first time, and found that charge parity (CP) violation in baryons, including particles like neutrons and protons that make up most of the universe’s visible matter. CP violation describes that nature treats antiparticles and particles slightly differently. This was seen in mesons only, the particles which are composed of a pair of quark-antiquark; further, it is important to explain that the universe is comprised of matter and not antimatter.

LHCb Detects 2.45% Asymmetry in Beauty–Lambda Baryon Decay

As per Live Science, this discovery is focused on the beauty-lambda baryon to a proton, two pions and a kaon. From 2009 to 2018, the data was analysed, which amounts to millions of decays and the counterparts of the antiparticle. However, they found a 2.45% asymmetry, which confirms the CP violation in baryons. The study was published in the journal Nature. This confirms the Standard Model prediction and leads to new physics.

CP violation was known in the 960s, first in kaons, then in the beauty mesons during 2001 and later in charm mesons during 2019. Baryons are made of three quarks, and remain enigmatic still. This CP violation directly tests the phenomenon’s universality with different types of particles and adds an important piece to the asymmetric antimatter mystery.

Breakthrough Offers New Clues to Matter–Antimatter Imbalance

However, the difference of 2.45% is not enough to determine the dominance of matter. We need to know the CP violation in baryons, which provides a promising and fresh direction in the search for physics. Scientists even found local asymmetry in decay channels specifically. This signals a rich substructure of deeper theory and exploration.

This research underscored CERN’s strength to probe basic symmetries at never-before-known precisions. Further, for 2030, the upgrades are scheduled, and there are large sets of data to be analysed with even more precise CP violation. This unlocks the new aspects of the universe and historical physics.

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Hubble Unveils Dark Matter Web in Stunning Abell 209 Galaxy Cluster Image

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Hubble Unveils Dark Matter Web in Stunning Abell 209 Galaxy Cluster Image

NASA/ESA’s Hubble Space Telescope has released a striking new picture of the large galaxy cluster Abell 209, 2.8 billion light-years from us in the Cetus constellation. The enormous cluster contains over 100 galaxies held together by gravity, but what is seen is only half the tale. Underneath the shining galaxies is a tangled web of unseen scaffolding—hot, diffuse gas and a vast amount of dark matter. Although invisible, these elements define the universe through their gravitational pull. The strong lenses of Hubble enable scientists to study these invisible elements and the twisted spacetime that they create.

Technological advancement

According to NASA website, the new image was taken with Hubble’s Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). Twelve exposures taken through different color filters were combined to make the full view. The final picture has a golden glow from dozens of bright elliptical galaxies clustering at the center, along with a few blue spiral galaxies at the edges. , Hubble avoids Earth’s blur to make distant galaxies appear pinpoint-sharp . In visible light, the largest galaxies appear as smooth golden orbs, while the spiral galaxies shine a faint blue. Hubble demonstrates a technological brilliance by merging optical and infrared data into one striking cosmic portrait.

Scientific revealations

Hubble scientists say images like this can help answer fundamental questions about dark matter and dark energy. The space between Abell 209’s galaxies is laced with X-ray–hot gas and dominated by dark matter. Only about 5% of the cosmos is ordinary matter; roughly 25% is dark matter and 70% is dark energy.

A massive cluster acts like a natural lens: its gravity slightly warps the light from more distant galaxies. In the Hubble image, a few faint background galaxies appear stretched into curved streaks. By measuring these distortions, scientists can map the cluster’s total mass (including dark matter). This lets them test theories about how the universe has grown under the influence of dark matter and dark energy

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Magnetic Wave Detection Uncovers Elusive Lithium in Mercury’s Thin Exosphere

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Magnetic Wave Detection Uncovers Elusive Lithium in Mercury’s Thin Exosphere

Using a new technique based on magnetic-wave analysis, scientists have, for the first time, discovered lithium in the atmosphere of Mercury. Published in Nature Communications, the study constitutes the first detection of lithium around the smallest planet in our solar system. The exosphere of Mercury, Unlike thickened atmospheres, the thin shell of particles that constitutes Mercury’s exosphere can render direct searching methods inadequate. Instead of searching for atoms, scientists analysed pick-up ion cyclotron waves—an electromagnetic fingerprint left behind when solar wind interacts with freshly ionised lithium. These faint signals finally confirmed lithium’s long-speculated presence.

MESSENGER Data Reveals Lithium Traces from Meteoroid Impacts in Mercury’s Exosphere

As per the Austrian Academy of Sciences, the research team led by Daniel Schmid reviewed four years of magnetic field data collected by NASA’s MESSENGER spacecraft. Twelve short-lived events—each lasting mere minutes—revealed these lithium-specific wave signatures.

The waves are generated when solar ultraviolet radiation ionises lithium atoms, and temporary lithium wind blows the ionised atoms into space, which increases the speed of the formation of electromagnetic instabilities. These perturbations induce oscillations at a single cyclotron frequency, determined by the mass and charge of lithium (such that it is identified as lithium indirectly by magnetic measurements).

Lithium has been difficult to find, as the rare alkali metal is thinly scattered. The traditional particle detectors on Mariner 10 and MESSENGER couldn’t directly capture it. The most likely candidate is meteoroid impacts, which would cause heated vapour clouds in the collision and throw lithium into the exosphere.

Mercury’s surface is continuously replenished by extraterrestrial bombardment, according to a study linking detected events to meteoroid strikes by objects 13-21 centimetres in radius. These high-speed collisions can vaporise up to 150 times their own mass, endowing the atmosphere with volatiles such as lithium.

Schmid’s study reveals that such processes could also account for the retention or acquisition of volatile elements in other airless bodies, which would transform our understanding of the geochemical story of Mercury and open up new steps in exosphere exploration.

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