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Why Won’t Our Parker Solar Probe Melt?

This summer, our Parker Solar Probe will launch to travel closer to the Sun than any mission before it, right into the Sun’s outer atmosphere, the corona.

The environment in the corona is unimaginably hot: The spacecraft will travel through material with temperatures greater than 3 million degrees Fahrenheit. 

So…why won’t it melt? 

The Difference Between Heat and Temperature

Parker Solar Probe was designed from the ground up to keep its instruments safe and cool, but the nature of the corona itself also helps. The key lies in the difference between heat and temperature.

Temperature measures how fast particles are moving, while heat is the total amount of energy that they transfer. The corona is an incredibly thin and tenuous part of the Sun, and there are very few particles there to transfer energy – so while the particles are moving fast (high temperature), they don’t actually transfer much energy to the spacecraft (low heat).

It’s like the difference between putting your hand in a hot oven versus putting it in a pot of boiling water (don’t try this at home!). In the air of the oven, your hand doesn’t get nearly as hot as it would in the much denser water of the boiling pot. 

So even though Parker Solar Probe travels through a region with temperatures of several million degrees, the surface of its heat shield will reach only about 2,500 F.

The Heat Shield

Of course, thousands of degrees Fahrenheit is still way too hot for scientific instruments. (For comparison, lava from volcano eruptions can be anywhere between 1,300 to 2,200 F.) 

To withstand that heat, Parker Solar Probe is outfitted with a cutting-edge heat shield, called the Thermal Protection System. This heat shield is made of a carbon composite foam sandwiched between two carbon plates. The Sun-facing side is covered with a specially-developed white ceramic coating, applied as a plasma spray, to reflect as much heat as possible.

The heat shield is so good at its job that even though the Sun-facing side of the shield will be at 2,500 F, the instruments in its shadow will remain at a balmy 85 F.

Parker Solar Probe Keeps its Cool

Several other designs on the spacecraft help Parker Solar Probe beat the heat. 

Parker Solar Probe is not only studying the Sun – it’s also powered by it. But even though most of the surface area of its solar arrays can be retracted behind the heat shield, even that small exposed segment would quickly make them overheat while at the Sun.  

To keep things cool, Parker Solar Probe circulates a single gallon of water through its solar arrays. The water absorbs heat as it passes behind the arrays, then radiates that heat out into space as it flows into the spacecraft’s radiator. 

It’s also important for Parker Solar Probe to be able to think on its feet, since it takes about eight minutes for information to travel between Earth and the Sun. If we had to control the spacecraft from Earth, by the time we knew something went wrong, it would be too late to fix it. 

So Parker Solar Probe is smart: Along the edges of the heat shield’s shadow are seven sensors. If any of these sensors detect sunlight, they alert the central computer and the spacecraft can correct its position to keep the sensors – and the rest of the instruments – safely protected behind the heat shield.

Over the course of its seven-year mission, Parker Solar Probe will make 24 orbits of our star. On each close approach to the Sun, it will sample the solar wind, study the Sun’s corona, and provide unprecedentedly close up observations from around our star – and armed with its slew of innovative technologies, we know it will keep its cool the whole time. 

Parker Solar Probe launches summer 2018 on its mission to study the Sun. Keep up with the latest on the mission at nasa.gov/solarprobe or follow us on Twitter and Facebook.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

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space edition - tag yourself

moonlight: sleep deprived af, genius ideas at 2:00 am, constantly underestimated, tangled earbuds, pretends like they don’t care but actually cares a lot, unscented candles

comet: will fight you for their friends, perfect eyeliner, doesn’t get angry but instead just fucking glares at you until you crumble, loves thunderstorms, cat person

stars: has no idea what they’re doing 167% of the time, artsy, likes halsey, string lights everywhere, loves fuzzy socks and blankets, probably wears space buns

alien: secretly is super good at makeup but doesn’t wear it often, lots of coffee, probably has a pet fish, reads young adult fantasy novels, closet conspiracy theorist, arms and papers always covered in doodles

black hole: 97% of their wardrobe is hoodies, professional procrastinator, can write, probably owns essential oils, eats ramen at 1:00 am, only writes in pen, actually really cool but doesn’t know it

spacedust: bath bombs, a+ insta feed, long flowy skirts and tops, city person, pretends to have their shit together, secretly loves kermit memes, probably dyed their hair at one point

NGC 7380, Wizard in Cepheus

NASA’s Fermi Traces Source of Cosmic Neutrino to Monster Black Hole

NASA - Fermi Gamma-ray Space Telescope logo. July 12, 2018 For the first time ever, scientists using NASA’s Fermi Gamma-ray Space Telescope have found the source of a high-energy neutrino from outside our galaxy. This neutrino traveled 3.7 billion years at almost the speed of light before being detected on Earth. This is farther than any other neutrino whose origin scientists can identify. High-energy neutrinos are hard-to-catch particles that scientists think are created by the most powerful events in the cosmos, such as galaxy mergers and material falling onto supermassive black holes. They travel at speeds just shy of the speed of light and rarely interact with other matter, allowing them to travel unimpeded across distances of billions of light-years.

Image above: NASA’s Fermi (top left) has achieved a new first—identifying a monster black hole in a far-off galaxy as the source of a high-energy neutrino seen by the IceCube Neutrino Observatory (sensor strings, bottom). Image Credits: NASA/Fermi and Aurore Simonnet, Sonoma State University. The neutrino was discovered by an international team of scientists using the National Science Foundation’s IceCube Neutrino Observatory at the Amundsen–Scott South Pole Station. Fermi found the source of the neutrino by tracing its path back to a blast of gamma-ray light from a distant supermassive black hole in the constellation Orion. “Again, Fermi has helped make another giant leap in a growing field we call multimessenger astronomy,” said Paul Hertz, director of the Astrophysics Division at NASA Headquarters in Washington. “Neutrinos and gravitational waves deliver new kinds of information about the most extreme environments in the universe. But to best understand what they’re telling us, we need to connect them to the ‘messenger’ astronomers know best—light.” Scientists study neutrinos, as well as cosmic rays and gamma rays, to understand what is going on in turbulent cosmic environments such as supernovas, black holes and stars. Neutrinos show the complex processes that occur inside the environment, and cosmic rays show the force and speed of violent activity. But, scientists rely on gamma rays, the most energetic form of light, to brightly flag what cosmic source is producing these neutrinos and cosmic rays. “The most extreme cosmic explosions produce gravitational waves, and the most extreme cosmic accelerators produce high-energy neutrinos and cosmic rays,” says Regina Caputo of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, the analysis coordinator for the Fermi Large Area Telescope Collaboration. “Through Fermi, gamma rays are providing a bridge to each of these new cosmic signals.” The discovery is the subject of two papers published Thursday in the journal Science. The source identification paper also includes important follow-up observations by the Major Atmospheric Gamma Imaging Cherenkov Telescopes and additional data from NASA’s Neil Gehrels Swift Observatory and many other facilities.

Image above: The discovery of a high-energy neutrino on September 22, 2017, sent astronomers on a chase to locate its source—a supermassive black hole in a distant galaxy. Image Credits: NASA’s Goddard Space Flight Center. On Sept. 22, 2017, scientists using IceCube detected signs of a neutrino striking the Antarctic ice with energy of about 300 trillion electron volts—more than 45 times the energy achievable in the most powerful particle accelerator on Earth. This high energy strongly suggested that the neutrino had to be from beyond our solar system. Backtracking the path through IceCube indicated where in the sky the neutrino came from, and automated alerts notified astronomers around the globe to search this region for flares or outbursts that could be associated with the event. Data from Fermi’s Large Area Telescope revealed enhanced gamma-ray emission from a well-known active galaxy at the time the neutrino arrived. This is a type of active galaxy called a blazar, with a supermassive black hole with millions to billions of times the Sun’s mass that blasts jets of particles outward in opposite directions at nearly the speed of light. Blazars are especially bright and active because one of these jets happens to point almost directly toward Earth.

Image above: Fermi-detected gamma rays from TXS 0506+056 are shown as expanding circles. Their maximum size, color—from white (low) to magenta (high)—and associated tone indicate the energy of each ray. Image Credits: NASA/DOE/Fermi LAT Collab. Fermi scientist Yasuyuki Tanaka at Hiroshima University in Japan was the first to associate the neutrino event with the blazar designated TXS 0506+056 (TXS 0506 for short). “Fermi’s LAT monitors the entire sky in gamma rays and keeps tabs on the activity of some 2,000 blazars, yet TXS 0506 really stood out,” said Sara Buson, a NASA Postdoctoral Fellow at Goddard who performed the data analysis with Anna Franckowiak, a scientist at the Deutsches Elektronen-Synchrotron research center in Zeuthen, Germany. “This blazar is located near the center of the sky position determined by IceCube and, at the time of the neutrino detection, was the most active Fermi had seen it in a decade.”

Visualizing Gamma Rays From Blazar TXS 0506+056

Video above: Fermi-detected gamma rays from TXS 0506+056 are shown as expanding circles. Their maximum size, color—from white (low) to magenta (high)—and associated tone indicate the energy of each ray. The first sequence shows typical emission; the second shows the 2017 flare leading to the neutrino detection. Video Credits: NASA/DOE/Fermi LAT Collab., Matt Russo and Andrew Santaguida/SYSTEM Sounds. NASA’s Fermi Gamma-ray Space Telescope is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy and with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden and the United States. The NASA Postdoctoral Fellow program is administered by Universities Space Research Association under contract with NASA. For more about NASA’s Fermi mission, visit: https://www.nasa.gov/fermi Fermi Gamma-Ray Space Telescope: http://www.nasa.gov/mission_pages/GLAST/main/index.html Related links: The source identification paper: http://science.sciencemag.org/cgi/doi/10.1126/science.aat1378 Major Atmospheric Gamma Imaging Cherenkov Telescopes: https://magic.mpp.mpg.de/ NASA’s Neil Gehrels Swift Observatory: https://www.nasa.gov/mission_pages/swift/main Deutsches Elektronen-Synchrotron: http://www.desy.de/index_eng.html Images (mentioned), Video (mentioned), Text, Credits: NASA/Felicia Chou/Sean Potter/GSFC/Dewayne Washington. Greetings, Orbiter.ch Full article

Spiral Galaxy NGC253 and Globular Cluster NGC288

by Eddie Trimarchi

Just let Earth enjoy the theory of general relativity, Mars.

P.S. Today (in 1905) the theory of special relativity was revealed!

This is so important. I have two years left of my Bachelor degree, and it took me 16 years to get my associate. Never give up, even if you have to put those goals on hold (sometimes multiple times), because life happens. Make yours worth it.

just because someone’s accomplishing more than you are right now doesn’t mean you’re failing. success isn’t a race

‘That was a quick flight’: How astronauts kept ice cool while their rocket malfunctioned at 4,970mph and plummeted back to Earth in harrowing 7G 'ballistic re-entry’ before hugging their loved-ones on the landing pad as Russia opens CRIMINAL probe.

Two astronauts kept ice cool as their rocket traveling at thousands of miles an hour malfunctioned on the edge of space while carrying them to the International Space Station, cockpit audio reveals.

Russian Aleksey Ovchinin and American Nick Hague made it back to Earth alive this morning after the booster on their Soyuz rocket broke at 164,000 feet and the rocket automatically turned back during a dramatic 7G 'ballistic re-entry’.

Ovchinin retained an enviable sang-froid as he realised what was happening, after they were rocked violently around in their seats by the force of the booster malfunction.

'An accident with the booster, 2 minutes, 45 seconds. That was a quick flight,’ he said in a calm voice in a streamed video of the incident.  

'We’re tightening our seatbelts,’ Ovchinin said on the video.

At that moment the two astronauts were experiencing weightlessness, when in an ordinary launch they should still have been pinned to the back of their seats by the force of the rocket surging upwards at 4,970mph.  

Russia says it has opened a criminal investigation and grounded all Soyuz flights. The accident comes weeks after a hole was discovered in the International Space Station amid talk from the Russian space authorities of deliberate sabotage.  

Video footage from the launch at the Baikonur Cosmodrome shows a large plume of smoke coming from the rocket at the moment it failed and footage from inside the capsule shows the two astronauts being violently shaken about.

The accident bears similarities to the 1986 Challenger disaster when one of its boosters failed at lift-off causing an explosion that killed seven.

Astronauts have been involved in Soyuz malfunctions twice before, one in 1983 when a crew was forced to eject from a Soyuz rocket as it exploded on the launchpad. In 1975 a Soyuz capsule crashed back to Earth from 90 miles up after a rocket failure, but the crew survived.

The rocket, which was designed in the 1960s, has also had one booster fail in similar fashion to today’s malfunction. In 2002 a booster rocket malfunctioned and the rocket which was carrying a satellite crashed in Kazakhstan killing one person on the ground.

In total Soyuz rockets have been launched 745 times of which 21 have failed. Thirteen of those failures have been since 2010, calling into question the continued reliability of the rocket.

Search and rescue teams were scrambled to the touchdown location as NASA revealed the descent meant the Russian-built Soyuz MS-10 spacecraft had to take 'a sharper angle of landing compared to normal’.

The Russians have suspended Soyuz flights to the space station while they investigate the cause of the booster failure.

The Soyuz is the only way to get people to the space station at the moment but officials insist the astronauts currently on the space station have enough supplies.  

NASA rookie Nick Hague and second-time flyer Aleksey Ovchinin of the Russian space agency were setting off for a six-month mission at the International Space Station Thursday, on a relatively rare two-man launch.

A spokesperson for NASA said that rescue teams have now reached Hague and Ovchinin and they’ve been taken out of the capsule and were in 'good condition’.

The craft’s landing engines and parachute system were said to have done their job as normal despite the enormous G-force acting on both the shuttle and crew during the landing.

Shortly after the incident rescue crews and paratroopers were rushed the emergency landing site in the barren Kazakh steppe to provide support for the crew.

NASA had issued a worrying tweet on Thursday morning saying: 'There’s been an issue with the booster from today’s launch. Teams have been in contact with the crew.’

'The capsule is returning via a ballistic descent, which is a sharper angle of landing compared to normal. Search and rescue teams are heading towards the expected touchdown location of the spacecraft and crew.’  

Cosmonaut Alexander Volkov commented: 'The guys are lucky that they remained alive. They had reached a good height so it was possible to descend in their capsule.’

More info, pictures, diagrams, videos at this link:  https://www.dailymail.co.uk/news/article-6264339/Rocket-launch-booster-malfunction-forces-astronauts-return-Earth-ballistic-entry.html

photography / hipster / indie / grunge