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A vibrant aurora display during a geomagnetic storm.  (Image credit: Shutterstock)

Earth’s thermosphere recently hit a near 20-year temperature peak after soaking up energy from geomagnetic storms that bashed Earth this year. The temperature in the second-highest layer of the atmosphere will likely continue to climb over the next few years as the sun’s activity ramps up, which could impact Earth-orbiting satellites, experts warn.

The thermosphere extends from the top of the mesosphere, at around 53 miles (85 kilometers) above ground, to the bottom of the exosphere, which begins at around 372 miles (600 km) above the ground, according to NASA. Beyond the exosphere is outer space.

For more than 21 years, NASA has measured the thermosphere temperature via infrared radiation emitted by carbon dioxide and nitric oxide molecules. Scientists convert data collected by NASA’s Thermosphere, Ionosphere, Mesosphere, Energetics and Dynamics (TIMED) satellite, into the Thermosphere Climate Index (TCI), which is measured in terawatts, or TW. (1 TW is equal to 1 trillion watts.)

The TCI value, which spiked on March 10, peaked at 0.24 TW, Martin Mlynczak, a leading researcher on the TIMED mission at NASA’s Langley Research Center in Virginia and creator of the TCI, told Live Science. The last time the TCI was this high was Dec. 28, 2003. (The temperature spike data has been submitted to a journal but has not yet been peer-reviewed.)

Related: 10 solar storms that blew us away in 2022

The temperature spike was caused by three geomagnetic storms in January and February — major disturbances to Earth’s magnetic field that are triggered by chunks of fast-moving magnetized plasma, known as coronal mass ejections (CMEs), and less often by streams of highly charged particles, known as solar wind, which are both spat out by the sun.  

“These ‘storms’ deposit their energy in the thermosphere and cause it to heat up,” Mlynczak said. “The increased heating results in increased levels of infrared emission from nitric oxide and carbon dioxide in the thermosphere.” Normally, infrared emissions after a storm cool the thermosphere, he added, but when the storms come back to back the temperature stays high.

Since the spike, at least two more geomagnetic storms have hit our planet — one on March 24, which was the most powerful solar storm to hit Earth for more than six years, and another equally powerful storm on April 24. The TCI values following these storms have remained high but have not yet passed the March peak, Mlynczak said.

A graph showing how the TCI value rises and falls with each solar cycle.  (Image credit: Marty Mlynczak (NASA Langley Research Center) and Linda Hunt (Science and Technology Corporation))

Geomagnetic storms become more frequent and intense during solar maximum, a part of the roughly 11-year solar cycle in which the sun is most active and covered in dark sunspots and plasma loops that spit out CMEs and solar wind. 

As a result, Earth’s thermosphere also follows a roughly 11-year cycle, Mlynczak said. Government scientists from NASA and NOAA predicted the next solar maximum will arrive in 2025, which means the warming trend will likely continue over the next few years. 

Changes to the thermosphere can pose challenges for satellites in low-Earth orbit that are positioned around the thermosphere’s upper boundary, Mlynczak said.

“The thermosphere expands as it warms,” Mlynczak said, resulting in “increased aerodynamic drag on all satellites and on space debris.” This increased drag can pull satellites closer to Earth, he said, which could cause satellites to crash into one another or completely fall out of orbit, as SpaceX Starlink satellites did in February 2022 after a surprise geomagnetic storm.

Satellite operators can avoid these issues by positioning their spacecraft in a higher orbit when needed, but the unpredictability of space weather makes it hard to know when these manoeuvres are required until it is often too late.related stories—Hidden tide in Earth’s magnetospheric ‘plasma ocean’ revealed in new study

—Mysterious aurora-like phenomenon ‘STEVE’ appears during strongest solar storm for more than half a decade

—Powerful X-class flare spat out a rare ‘solar tsunami,’ and you can hear it smashing into Earth

Solar maximum could also arrive sooner than predicted. A recent study published Jan. 30 in the journal Frontiers in Astronomy and Space Sciences suggests that the solar activity peak could arrive as early as late 2023 and be more powerful than initially predicted. If this scenario plays out, then the risk of a satellite disaster further increases.  

However, over longer timescales, temperatures in the thermosphere are declining, because excess CO2 in the thermosphere due to climate change increases infrared emissions into space, a May 8 study in the journal Earth Atmospheric and Planetary Sciences found. 

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Science

NASA to Launch First Quantum Sensor for Gravity Monitoring in Space

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NASA to Launch First Quantum Sensor for Gravity Monitoring in Space

NASA’s Jet Propulsion Laboratory, commercial companies, and academic institutions together are developing the first space-based quantum sensors for gravitational measurement. Two groups of very cold rubidium atoms will be used as weights for the Quantum Gravity Gradiometer Pathfinder (QGGPf) instrument, ensuring accurate measurements over long periods. Measuring gravity with a volume of 0.3 cubic yards (0.25 cubic meters) and weighing just over 275 pounds (125 kg), the instrument will be smaller and lighter than conventional space-based gravity instruments.

Quantum sensors offer enormous promise for sensitivity; estimates suggest they could be as much as ten times more sensitive in tracking gravity than conventional sensors. Approved to begin at the end of the decade, the technology validation project aims to test novel atomic-scale atomic manipulation of interactions between light and matter. To progress the sensor head technology and the laser optical system, NASA is working with small companies. The QGGPf instrument could lead to planetary science and fundamental physics applications.

NASA’s Quantum Gravity Sensor to Reveal Earth’s Subsurface

According to a NASA post, the Jet Propulsion Laboratory, private companies, and academic institutions are developing the first space-based quantum sensor for measuring gravity. This mission, supported by NASA’s Earth Science Technology Office (ESTO), will pave the way for groundbreaking observations of everything from petroleum reserves to global supplies of fresh water. Its gravitational field is dynamic and changing every day as geologic processes distribute mass throughout its surface. Sensitive instruments called gravity gradiometers can map the subtleties of Earth’s gravitational field and link them to belowground structures such as mineral deposits and aquifers.

The Quantum Gravity Gradiometer Pathfinder (QGGPf) instrument will use two clouds of ultracold rubidium atoms as test masses. The difference in acceleration between these matter waves will measure the difference in acceleration between these matter waves to locate gravitational anomalies. This system allows for space-based gravity measurements to remain accurate over long periods and is smaller and lighter than traditional space-based gravity instruments.

NASA Tests Atomic-Scale Tech to Advance Space Sensors and Earth Science

The main purpose of this technology validation mission is to test a collection of novel technologies for manipulating interactions between light and matter at the atomic scale. With JPL partnering with AOSense and Infleqtion to enhance sensor head technology and NASA’s Goddard Space Flight Center working with Vector Atomic to advance the laser optical system, the project involves notable partnerships between NASA and a few quantum-focused entrepreneurs.

Ultimately, the findings of this Pathfinder project might increase our capacity to explore Earth, understand far-off worlds, and value the role gravity plays in creating the universe.

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Science

NASA’s Hubble Shares Detailed Mosaic of the Sombrero Galaxy

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NASA’s Hubble Shares Detailed Mosaic of the Sombrero Galaxy

NASA’s Hubble Space Telescope, on its 35th anniversary, reprocessed a detailed image of the Sombrero Galaxy (Messier 104) on April 11, shared by the European Space Agency. This improvised image, generated from numerous Hubble images, signals fine dust structures, the luminous galactic nucleus with a backdrop occupied by stars and various distant galaxies. This mosaic, taken from the updated data and refined processing techniques, makes it a significant upgrade to previous Hubble observations. This release marks a milestone in the so-far legacy of the Hubble Space Telescope, showcasing the evolution of modern techniques and escalation into archival space imagery.

Research and Discovery

Katie Noll and other scientists of the European Space Agency worked in collaboration with NASA using the Hubble Space Telescope. New imaging technology and methods were used to build upon the original Hubble image released in October 2003. On November 25, 2024, the James Webb Space Telescope also offered a fresh image and perspective on the galaxy, further enriching the research.
The Sombrero Galaxy is located about 30 million light years away in the Virgo constellation and is renowned for its unique shape that resembles a sombrero hat. Its sharp and edgy orientation, titled just six degrees, throws a dramatic view with a dust-laced disc and a brightening central bulge.

Structure and Star Formation

In terms of star formation, the Sombrero Galaxy is visually rich but surprisingly calm. Within its dusty disc, less than one solar mass is transformed into stars every year. This galaxy is so silent that even its massive black hole, with a weight of nine billion solar masses, stays inactive or dormant. Looking into the structure of the galaxy, it is baffling as it displays the classic disc of spiral galaxies.
However, it also features a halo and bump similar to those of elliptical galaxies. This uneven combination leaves scientists unsure of whether it should be kept in the category of elliptical or somewhere in between.

Future Exploration

The crucial part is analysing the chemical composition of stars in the galaxy’s halo. In the precise measurements done by Hubble there revealed an astonishing presence of metal-rich stars was revealed in its outer region. Researchers believe that the Sombrero Galaxy could have blended with other large galaxies billions of years ago, resulting in the mysterious hybrid structure observed in the present.

Scientists are looking forward to fusing Hubble’s optical data with infrared imaging from the James Webb Space Telescope for future investigation of the galaxy’s structure. This multi-wavelength research could unleash deeper insights about its formation and clarify how galaxy mergers can shape its evolution.

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Politics

Who’s nicer – Lords or MPs?

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Who's nicer - Lords or MPs?

👉 Click here to listen to Electoral Dysfunction on your podcast app 👈

The two baronesses of the podcast finally lift the lid on the House of Lords in this special Q&A episode. What’s it really like on the red benches in parliament? And if you’re a Lord, are you a has-been?

Also – was Tony Blair actually cool in the 90s? Or was it just a more optimistic time in politics?

Come and join us LIVE on Tuesday 20th May at Cadogan Hall in London, tickets available now: https://www.aegpresents.co.uk/event/electoral-dysfunction-live/

Remember you can also watch us on YouTube!

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