Anonymous ID: e2c2df Aug. 14, 2024, 7:20 a.m. No.21410439   🗄️.is 🔗kun   >>0514 >>0602 >>0697

NASA Astronomy Picture of the Day

August 14, 2024

 

Meteors and Aurora over Germany

 

This was an unusual night. For one thing, the night sky of August 11 and 12, earlier this week, occurred near the peak of the annual Perseid Meteor Shower. Therefore, meteors streaked across the dark night as small bits cast off from Comet Swift-Tuttle came crashing into the Earth's atmosphere. Even more unusually, for central Germany at least, the night sky glowed purple. The red-blue hue was due to aurora caused by an explosion of particles from the Sun a few days before. This auroral storm was so intense that it was seen as far south as Texas and Italy, in Earth's northern hemisphere. The featured image composite was built from 7 exposures taken over 26 minutes from Ense, Germany. The Perseids occur predictably every August, but auroras visible this far south are more unusual and less predictable.

 

https://apod.nasa.gov/apod/astropix.html?

Anonymous ID: e2c2df Aug. 14, 2024, 7:47 a.m. No.21410545   🗄️.is 🔗kun   >>0602 >>0697

New TEMPO Cosmic Data Story Makes Air Quality Data Publicly Available

Aug 13, 2024

 

On May 30th, 2024, NASA and the Center for Astrophysics | Harvard & Smithsonian announced the public release of "high-quality, near real-time air quality data" from NASA’s TEMPO (Tropospheric Emissions: Monitoring of Pollution) mission.

The NASA Science Activation program's Cosmic Data Stories team, led by Harvard University in Cambridge, MA, has since released a new "Data Story" – an interactive, digital showcase of new science imagery, including ideas for exploration and scientific highlights shared in a brief video and narrative text – that provides a quick and easy way for the public to visualize this important, large data set from TEMPO.

 

TEMPO allows unprecedented monitoring of air quality down to neighborhood scales, with its hourly daytime scans over North America. Air pollutants like NO2, produced, for example, by the burning of fossil fuels, can trigger significant health issues, especially among people with pre-existing illnesses such as asthma.

The interactive views in the TEMPO Data Story provide public access to the same authentic data that scientists use and invite the public to explore patterns in their local air quality.

For example, how do NO2 emissions vary in our area throughout the day and week? What are possible sources of NO2 in our community? How does our air quality compare with that of other communities with similar population densities, or with nearby urban or rural communities?

TEMPO’s hyper-localized data will allow communities to make informed decisions and take action to improve their air quality.

 

The Cosmic Data Story team is grateful to TEMPO scientists, Xiong Liu and Caroline Nowlan, for providing the team with early access to the data and guidance on NO2 phenomena that learners can explore in the data.

The TEMPO Data Story, featured on TEMPO’s webpage for the public, adds Earth science data to the portfolio of Cosmic Data Stories that is already making astrophysics data accessible to the public.

 

TEMPO Team Atmospheric Physicist from the Harvard-Smithsonian Center for Astrophysics, Caroline Nowlan, had this to say: "TEMPO produces data that are really useful for scientists, but are also important for the general public and policy makers.

We are thrilled that the Cosmic Data Stories team has made a tool that allows everyone to explore TEMPO data and learn about pollution across North America and in their own communities."

 

The Cosmic Data Stories project is supported by NASA under cooperative agreement award number 80NSSC21M0002 and is part of NASA’s Science Activation Portfolio.

Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn

 

https://science.nasa.gov/learning-resources/science-activation/new-tempo-cosmic-data-story-makes-air-quality-data-publicly-available/

Anonymous ID: e2c2df Aug. 14, 2024, 7:57 a.m. No.21410586   🗄️.is 🔗kun   >>0602 >>0697

NASA Demonstrates ‘Ultra-Cool’ Quantum Sensor for First Time in Space

Aug 13, 2024

 

NASA’s Cold Atom Lab, a first-of-its-kind facility aboard the International Space Station, has taken another step toward revolutionizing how quantum science can be used in space.

Members of the science team measured subtle vibrations of the space station with one of the lab’s onboard tools — the first time ultra-cold atoms have been employed to detect changes in the surrounding environment in space.

 

The study, which appeared in Nature Communications on Aug. 13, also reports the longest demonstration of the wave-like nature of atoms in freefall in space.

The Cold Atom Lab science team made their measurements with a quantum tool called an atom interferometer, which can precisely measure gravity, magnetic fields, and other forces.

Scientists and engineers on Earth use this tool to study the fundamental nature of gravity and advance technologies that aid aircraft and ship navigation.

(Cell phones, transistors, and GPS are just a few other major technologies based on quantum science but do not involve atom interferometry.)

 

Physicists have been eager to apply atom interferometry in space because the microgravity there allows longer measurement times and greater instrument sensitivity, but the exquisitely sensitive equipment has been considered too fragile to function for extended periods without hands-on assistance.

The Cold Atom Lab, which is operated remotely from Earth, has now shown it’s possible.

“Reaching this milestone was incredibly challenging, and our success was not always a given,” said Jason Williams, the Cold Atom Lab project scientist at NASA’s Jet Propulsion Laboratory in Southern California.

“It took dedication and a sense of adventure by the team to make this happen.”

 

Space-based sensors that can measure gravity with high precision have a wide range of potential applications.

For instance, they could reveal the composition of planets and moons in our solar system, because different materials have different densities that create subtle variations in gravity.

This type of measurement is already being performed by the U.S.-German collaboration GRACE-FO (Gravity Recovery and Climate Experiment Follow-on), which detects slight changes in gravity to track the movement of water and ice on Earth. An atom interferometer could provide additional precision and stability, revealing more detail about surface mass changes.

 

Precise measurements of gravity could also offer insights into the nature of dark matter and dark energy, two major cosmological mysteries. Dark matter is an invisible substance five times more common in the universe than the “regular” matter that composes planets, stars, and everything else we can see.

Dark energy is the name given to the unknown driver of the universe’s accelerating expansion.

 

“Atom interferometry could also be used to test Einstein’s theory of general relativity in new ways,” said University of Virginia professor Cass Sackett, a Cold Atom Lab principal investigator and co-author of the new study.

“This is the basic theory explaining the large-scale structure of our universe, and we know that there are aspects of the theory that we don’t understand correctly.

This technology may help us fill in those gaps and give us a more complete picture of the reality we inhabit.”

 

About the size of a minifridge, the Cold Atom Lab launched to the space station in 2018 with the goal of advancing quantum science by putting a long-term facility in the microgravity environment of low Earth orbit.

The lab cools atoms to almost absolute zero, or minus 459 degrees Fahrenheit (minus 273 degrees Celsius).

At this temperature, some atoms can form a Bose-Einstein condensate, a state of matter in which all atoms essentially share the same quantum identity. As a result, some of the atoms’ typically microscopic quantum properties become macroscopic, making them easier to study.

 

Quantum properties include sometimes acting like solid particles and sometimes like waves.

Scientists don’t know how these building blocks of all matter can transition between such different physical behaviors, but they’re using quantum technology like what’s available on the Cold Atom Lab to seek answers.

In microgravity, Bose-Einstein condensates can reach colder temperatures and exist for longer, giving scientists more opportunities to study them.

The atom interferometer is among several tools in the facility enabling precision measurements by harnessing the quantum nature of atoms.

 

Due to its wave-like behavior, a single atom can simultaneously travel two physically separate paths.

If gravity or other forces are acting on those waves, scientists can measure that influence by observing how the waves recombine and interact.

 

https://www.nasa.gov/missions/station/iss-research/cold-atom-laboratory/nasa-demonstrates-ultra-cool-quantum-sensor-for-first-time-in-space/

Anonymous ID: e2c2df Aug. 14, 2024, 8:16 a.m. No.21410650   🗄️.is 🔗kun   >>0697

Colossal X-class solar flare erupts from 'rule-breaking' sunspot and Earth is in the firing line

August 14, 2024

 

The active sun is kicking into overdrive.

In the early morning hours today (Aug. 14), the sun unleashed the most powerful class of solar flare, in a potent X-class eruption.

The solar flare peaked at 2:40 a.m. EDT (0640 GMT) and caused shortwave radio blackouts over the sunlit portion of Earth at the time of the eruption, Asia and the Indian Ocean.

 

What makes this X-class solar flare particularly interesting is that it erupted from 'rule-breaking' sunspot AR3784 which had already garnered the attention of solar scientists and aurora chasers due to its strange polarity.

The sunspot's polarity breaks a hundred-year-old rule, Hale's Law, whereby sunspots in the Northern Hemisphere should be polarized -+. Instead, sunspot AR3784 is polarized ±, a whole 90-degree twist, according to Spaceweather.com.

It's not the first sunspot to break the rule, according to spaceweather.com, it happens approximately 3% of the time. However, a majority of "rule-breakers" show a "reversed polarity" of +- instead of -+, but AR3784 lies somewhere between the two.

 

Experts at Spaceweather.com suggested that the "magnetic underpinnings of this sunspot are corkscrewing in an unusual way. If opposite magnetic polarities get twisted together too tightly, there could be an X-class solar flare." Lo and behold the sunspot did just that.

Solar flares are eruptions on the sun's surface that release intense bursts of electromagnetic radiation.

These flares occur when built-up magnetic energy in the solar atmosphere is suddenly released.

They are classified by size into different categories, with X-class flares being the most powerful. M-class flares are 10 times less intense than X-class, followed by C-class flares, which are 10 times weaker than M-class. B-class flares are 10 times weaker than C-class, and A-class flares, which are 10 times weaker than B-class, have no significant effects on Earth.

Within each class, numbers from 1 to 10 (and beyond for X-class) indicate the relative strength of the flare.

 

Powerful solar flares like the one released this morning can often be accompanied by a coronal mass ejection — a large plume of plasma and magnetic field from the sun — it has yet to be confirmed whether a CME joined this eruption.

Aurora hunters cross your fingers and charge those cameras! (If you hope to snap a photo of the northern lights, check out our guide on where and how to photograph auroras.)

CMEs carry electrically charged particles known as ions, and when these collide with Earth's magnetosphere, they can trigger geomagnetic storms.

During these storms, the ions interact with gases in Earth's atmosphere, releasing energy in the form of light. This phenomenon is recognized as the northern lights, or aurora borealis, in the Northern Hemisphere, and as the southern lights, or aurora australis, in the Southern Hemisphere.

 

If a CME is confirmed, we could be in for yet more geomagnetic storms and heightened aurora activity, so get those cameras charged just in case. We await further confirmation.

One thing we do know that accompanied the X-flare was a strong radio blackout on Earth.

The shortwave radio blackouts detected over Asia and the Indian Ocean resulted from the intense burst of X-rays and extreme ultraviolet radiation emitted during the X-flare.

 

https://www.space.com/x-class-solar-flare-eruption-rule-breaking-sunspot-video