PARKER SOLAR PROBE (NASA SPACECRAFT)

There’s a wind that emanates from the Sun. It blows not like a soft whistle but like a hurricane’s scream. Made of electrons, protons and heavier ions, the solar wind courses through the solar system at roughly 1 million mph (1.6 million kph), barreling over everything in its path. Yet through the wind’s roar, NASA’s Parker Solar Probe hears the small chirps, squeaks and rustles that hint at the origin of this mysterious and ever-present wind. The spacecraft’s FIELDS instrument can eavesdrop on the electric and magnetic fluctuations caused by plasma waves. The Parker Solar Probe it can “hear” when the waves and particles interact with one another, recording frequency and amplitude information about these plasma waves that scientists could then play as sound waves. And it results in some striking sounds. Solar wind sounds playlist: https://soundcloud.com/jhu-apl/sets/sounds-of-the-solar-wind Learn more about the Sounds of the Solar Wind: https://www.jhuapl.edu/FeatureStory/200114 More on solar wind sound from the Parker Solar Probe: http://parkersolarprobe.jhuapl.edu/News-Center/Show-Article.php?articleID=139

Scientists have revealed the results of the Parker Solar Probe’s first two flybys of the Sun, and LIGO has a new instrument called the quantum vacuum squeezer! Hosted by: Caitlin Hofmeister SciShow has a spinoff podcast! It's called SciShow Tangents. Check it out at http://www.scishowtangents.org ---------- Support SciShow by becoming a patron on Patreon: https://www.patreon.com/scishow ---------- Huge thanks go to the following Patreon supporters for helping us keep SciShow free for everyone forever: Kevin Carpentier, Eric Jensen, Matt Curls, Sam Buck, Christopher R Boucher, Avi Yashchin, Adam Brainard, Greg, Alex Hackman, Sam Lutfi, D.A. Noe, Piya Shedden, Scott Satovsky Jr, Charles Southerland, Patrick D. Ashmore, charles george, Kevin Bealer, Chris Peters ---------- Like SciShow? Want to help support us, and also get things to put on your walls, cover your torso and hold your liquids? Check out our awesome products over at DFTBA Records: http://dftba.com/scishow ---------- Looking for SciShow elsewhere on the internet? Facebook: http://www.facebook.com/scishow Twitter: http://www.twitter.com/scishow Tumblr: http://scishow.tumblr.com Instagram: http://instagram.com/thescishow ---------- Sources: https://www.nature.com/articles/d41586-019-03665-3 https://www.nasa.gov/press-release/first-nasa-parker-solar-probe-results-reveal-surprising-details-about-our-sun https://www.nasa.gov/mission_pages/iris/multimedia/layerzoo.html http://parkersolarprobe.jhuapl.edu/The-Mission/index.php#introduction http://news.mit.edu/2019/ligo-reach-quantum-noise-wave-1205 Images: https://svs.gsfc.nasa.gov/12911 http://parkersolarprobe.jhuapl.edu/The-Mission/index.php#Where-Is-PSP https://svs.gsfc.nasa.gov/30481 https://svs.gsfc.nasa.gov/12704 https://svs.gsfc.nasa.gov/13113 https://svs.gsfc.nasa.gov/20299 https://svs.gsfc.nasa.gov/13105 https://svs.gsfc.nasa.gov/11086 https://commons.wikimedia.org/wiki/File:Initial_and_Enhanced_LIGO_schematics.png

You can buy Universe Sandbox 2 here: http://amzn.to/2yJqwU6 Or get a shirt: https://teespring.com/stores/whatdamath Hello and welcome! My name is Anton and in this video, we will talk about new discoveries coming from the Parker Solar Probe. Papers: http://www.nature.com/articles/s41586-019-1818-7 https://www.nature.com/articles/s41586-019-1813-z https://www.nature.com/articles/s41586-019-1818-7 https://www.nature.com/articles/s41586-019-1818-7 Support this channel on Patreon to help me make this a full time job: https://www.patreon.com/whatdamath Space Engine is available for free here: http://spaceengine.org Enjoy and please subscribe. Twitter: https://twitter.com/WhatDaMath Facebook: https://www.facebook.com/whatdamath Twitch: http://www.twitch.tv/whatdamath Bitcoins to spare? Donate them here to help this channel grow! 1GFiTKxWyEjAjZv4vsNtWTUmL53HgXBuvu The hardware used to record these videos: CPU: https://amzn.to/2LZFQCJ Video Card: https://amzn.to/2M1W26C Motherboard: https://amzn.to/2JYGiQQ RAM: https://amzn.to/2Mwy2t4 PSU: https://amzn.to/2LZcrIH Case: https://amzn.to/2MwJZz4 Microphone: https://amzn.to/2t5jTv0 Mixer: https://amzn.to/2JOL0oF Recording and Editing: https://amzn.to/2LX6uvU Thank you to all Patreon supporters of this channel Specifically, great thanks to the following members: Morrison Waud Vlad Manshin Mark Teranishi TheHuntress Daniel Rosvall Ralph Spataro Lilith Dawn Albert B. Cannon Greg Lambros adam lee Jer Henry Spadoni Nick Dolgy Konrad Kummli UnexpectedBooks.com J Carter Gabriel Seiffert Shinne George Williams Jakub Glos Johann Goergen Lyndon Riley LS Greger Jake Salo Michael Tiganila Lauren Smith Olegas Budnik Dave Blair Sander Stols Kai Raphahn Sergio Ruelas Arikkat Unnikrishnan Steven Becky Tracy Burgess Gordon Cooper Steve Wotton Jayjay Volz Anataine Deva Honey Suzanne Lyons Daniel Coleman Matthew Lazear xyndicate Steven Aiello

Launched in 2018, NASA’s Parker Solar Probe spacecraft, with instruments developed and built by UC Berkeley, has now travelled closer to the sun than any other mission in history, actually penetrating the sun’s atmosphere, to investigate highly charged magnetic field. Now, that data has allowed solar physicists to map the source of a major component of the solar wind that continually peppers Earth’s atmosphere, while revealing strange magnetic field reversals that could be accelerating these particles toward our planet. These accelerated particles interact with Earth’s magnetic field, generating the colorful northern and southern lights but also potentially damaging the electrical grid and telecommunications networks on the surface, threatening orbiting satellites and perhaps endangering astronauts in space. The more solar physicists understand about the magnetic environment of the sun and how it flings solar wind particles out toward the planets, the better they will be able to predict events to prevent damage. “There was a major space weather event in 1859 that blew out telegraph networks on Earth and one in 1972 that set off naval mines in North Vietnam, just from the electrical currents generated by the solar storm,” said Stuart Bale, a University of California, Berkeley, professor of physics and lead author of an article about new results from the probe’s FIELDS experiment. “We’re much more of a technological society than we were in 1972, the communications networks and the power grid on Earth are extraordinarily complex, so big disturbances from the sun are potentially a very serious thing. If we could predict space weather, we could shut down or isolate parts of the power grid, or shut down satellite systems that might be vulnerable.” (Cont'd...) (Full Story: https://news.berkeley.edu/2019/12/04/parker-probe-traces-solar-wind-to-its-source-on-suns-surface/) Video by Roxanne Makasdjian and Stephen McNally (Animations and images courtesy of: NASA/JHUAPL, NASA GSFC/CIL/Brian Monroe, NASA GSFC/CIL/Krystofer Kim, Johns Hopkins University/APL/Steve Gribben) http://news.berkeley.edu/ http://www.facebook.com/UCBerkeley http://twitter.com/UCBerkeley http://instagram.com/ucberkeleyofficial

Parker Solar Probe - NASA's mission to touch the Sun - has revealed new discoveries about our star. Principal Investigators for some of the mission's instruments share their excitement about this new science.

NASA's Parker Solar Probe mission has returned unprecedented data from near the Sun, culminating in new discoveries published on Dec. 4, 2019, in the journal Nature. Among the findings are new understandings of how the Sun's constant outflow of material, the solar wind, behaves. Seen near Earth -- where it can interact with our planet's natural magnetic field and cause space weather effects that interfere with technology -- the solar wind appears to be a relatively uniform flow of plasma. But Parker Solar Probe's observations reveal a complicated, active system not seen from Earth. Music Credit: Smooth as Glass by The Freeharmonic Orchestra Read more: https://www.nasa.gov/feature/goddard/2019/nasas-parker-solar-probe-sheds-new-light-on-the-sun/ Video Credit: NASA's Goddard Space Flight Center Karen Fox (ADNET): Writer Sarah Frazier (ADNET): Writer Genna Duberstein (USRA): Producer Genna Duberstein (USRA): Editor Chris Smith (USRA): Narrator Adriana Manrique Gutierrez (USRA): Animator Jonathan North (USRA): Animator Scott Wiessinger (USRA): Animator Adam Szabo (NASA/GSFC): Scientist Russ Howard (NRL): Scientist Dave McComas (SwRI): Scientist Stuart Bale (University of California, Berkeley): Scientist Justin Kasper (University of Michigan): Scientist Nour Raouafi (Johns Hopkins University/APL): Scientist Eric Christian Ph.D. (NASA/HQ): Scientist Adam Szabo (NASA/GSFC): Project Support Please give credit for this item to: NASA's Goddard Space Flight Center This video is public domain and along with other supporting visualizations can be downloaded from the Scientific Visualization Studio at: http://svs.gsfc.nasa.gov/13282 If you liked this video, subscribe to the NASA Goddard YouTube channel: http://www.youtube.com/NASAExplorer Follow NASA’s Goddard Space Flight Center · Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard · Twitter http://twitter.com/NASAGoddardPix · Facebook: http://www.facebook.com/NASA.GSFC · Flickr http://www.flickr.com/photos/gsfc

Engineers and designers working on the Parker Solar Probe tackled challenges such as size, weight, and extreme heat. Their design combined unique materials and underwent rigorous testing to transform the Probe into a record-breaking spacecraft. This Is Not a Real Explosion, Here’s How Physics Made It Happen - https://youtu.be/OsUCD4wno6g Read More Why Won't Parker Solar Probe Melt? https://www.nasa.gov/feature/goddard/2018/traveling-to-the-sun-why-won-t-parker-solar-probe-melt "In space, the temperature can be thousands of degrees without providing significant heat to a given object or feeling hot. Why? Temperature measures how fast particles are moving, whereas heat measures the total amount of energy that they transfer. Particles may be moving fast (high temperature), but if there are very few of them, they won’t transfer much energy (low heat). Since space is mostly empty, there are very few particles that can transfer energy to the spacecraft." Who is Eugene Parker? https://www.nasa.gov/content/goddard/eugene-newman-parker "More than half a century later, the Parker Solar Probe mission will finally be able to provide key observations on Parker’s groundbreaking theories and ideas, which have informed a generation of scientists about solar physics and the magnetic fields around stars. Much of his pioneering work, which has been proven by subsequent spacecraft, defined a great deal of what we know about the how the sun–Earth system interacts." NASA Is Going to The Sun, Here’s Why That’s So Crazy https://www.seeker.com/videos/space/nasa-is-going-to-the-sun-heres-why-thats-so-crazy "From Earth, we can only ever see the corona during a total solar eclipse, which is why it is incredibly difficult to study. Because the density is so low, the corona’s brightness is overpowered by energy coming from the solar surface. As the last layer of the sun’s atmosphere, the corona extends millions of miles into space. Here, temperatures can rise to over one million degrees Celsius which is about 300 times hotter than the photosphere, the lowest layer of the sun’s atmosphere." ____________________ Science In The Extremes ventures to the ends of the earth to bring you pioneering research and innovations that are advancing our civilization and broadening our understanding of the universe. Follow intrepid researchers as they plunge into the deepest parts of the ocean, trek across the arctic tundra, and explore the cosmos, because being a scientist isn’t just about being in the lab. Seeker explains every aspect of our world through a lens of science, inspiring a new generation of curious minds who want to know how today’s discoveries in science, math, engineering and technology are impacting our lives and shaping our future. Our stories parse meaning from the noise in a world of rapidly changing information. Visit the Seeker website https://www.seeker.com/videos Subscribe now! http://www.youtube.com/subscription_center?add_user=dnewschannel Seeker on Twitter http://twitter.com/seeker Seeker on Facebook https://www.facebook.com/SeekerMedia/ Science in the Extremes on Facebook http://www.facebook.com/ScienceintheExtremes Seeker http://www.seeker.com/

How Close Can We Get To The Sun? ► Subscribe: https://goo.gl/GmtyPv For more images and videos visit www.gettyimages.com More than ever before, humanity is heading toward the centre of the Solar System. With the Parker Solar Probe, NASA is aiming to get closer to the sun than ever before. But, what's the mission all about? And how close can we really expect to get? With cutting edge technology, state-of-the-art science and some genius minds in mission control, it all makes for one awesome adventure! What do you think? Let us know in the comments, and tell us more questions you'd like us to explore! Find more mind bending videos to satisfy your curiosity here: What If Earth Crashed Into Another Planet - https://www.youtube.com/watch?v=CcWA_z_jYmE What If Black Holes Can Change the Future? - https://www.youtube.com/watch?v=cu19nVzKhpM #TouchTheSun #ParkerSolarProbe #NASA #Sun #Solar #SolarProbe

According to Business Insider, a NASA spacecraft broke a record for the fastest human-made object. The Parker Solar Probe launched back in August to investigate the outer region of the Sun's atmosphere, the corona. The billion-dollar solar probe will reach speeds close to 213,200 miles-per-hour while flying past the Sun. During its mission, the probe will have to navigate clumps of plasma that are over 3 million degrees in Fahrenheit, as it orbits the Sun 15-million miles away from it's surface. https://www.businessinsider.com/nasa-parker-solar-probe-fastest-human-object-2018-11 http://www.wochit.com This video was produced by YT Wochit Tech using http://wochit.com

The sun is the very centerpiece of our solar system and the most important source of energy for life on Earth. And according to MNN, it's on the verge of receiving a visitor. On Oct. 29, NASA's Parker Solar Probe achieved a milestone by becoming the closest man-made object to the sun. Over the next several years, the probe will orbit closer to the sun with the closest approach being 3.83 million miles away. The mission was launched to study some of the sun's biggest secrets. https://www.mnn.com/earth-matters/space/blogs/nasa-mission-solar-probe-plus-explore-sun-outer-atmosphere http://www.wochit.com This video was produced by YT Wochit Tech using http://wochit.com

Consider supporting Space Fan News: https://patreon.com/DeepAstronomy to ensure you get current space & astronomy news each week! Earlier this month, the Parker Solar Probe sent back the first images from each of its four instruments while enroute to the Sun. These early observations – while not yet examples of the key science observations it will take closer to the Sun – show that each of the instruments is working well. Space Fan News Theme by Stephen Dubois available for download here: http://ancienteyesmusic.com Space Fan News Background Music by Colour the Landscapes: https://colourthelandscapes.bandcamp.com/ Follow DeepAstronomy on Twitter: @DeepAstronomy Like DeepAstronomy on Facebook: https://www.facebook.com/DeepAstronomy/ Like Space Fan News on Facebook: https://www.facebook.com/SpaceFanNews/

Following years of work and preparation, a United Launch Alliance Delta IV Heavy rocket launched NASA's Parker Solar Probe for an unprecedented mission to "kiss the Sun." The spacecraft aims to unravel 60 years' worth of mysteries surrounding the Sun’s corona and how it effects life on Earth. Learn more at: http://www.nasa.gov/parkersolarprobe

Watch in 360 degrees as a United Launch Alliance Delta IV Heavy rocket lifts off from Space Launch Complex-37 at Cape Canaveral Air Force Station in Florida carrying NASA's Parker Solar Probe. Roughly the size of a small car, the spacecraft lifted off at 3:31 a.m. EDT on Aug. 12, 2018, starting its historic mission to the Sun.

NASA's historic Parker Solar Probe mission that launched Aug. 12, 2018 from Space Launch Complex 37 on Cape Canaveral Air Force Station in Florida will revolutionize our understanding of the Sun. The Parker Solar Probe spacecraft will travel through the Sun’s atmosphere, closer to the surface than any spacecraft before it, facing brutal heat and radiation conditions — and ultimately providing humanity with the closest-ever observations of a star. This is a look at the moments leading up to T-Zero for NASA’s mission to "touch" the Sun. Learn more about the mission at: https://www.nasa.gov/parkersolarprobe

NASA’s Parker Solar Probe launched from Florida Sunday, Aug. 12 to begin its journey to the Sun, where it will undertake a landmark mission. The spacecraft will transmit its first science observations in December, beginning a revolution in our understanding of the star that makes life on Earth possible. The spacecraft – designed, built, and managed for NASA by the Johns Hopkins Applied Physics Laboratory – lifted off at 3:31 a.m. EDT on a United Launch Alliance Delta IV Heavy rocket from Space Launch Complex-37 at Cape Canaveral Air Force Station. At 5:33 a.m. EDT, the mission operations manager at APL reported that the spacecraft was healthy and operating nominally.

Our mission to touch the Sun is on its way, Administrator Bridenstine visits NASA spaceflight facilities, and an update on our first-ever asteroid sample return mission … a few of the stories to tell you about – This Week at NASA! This video is available for download from NASA's Image and Video Library: https://images.nasa.gov/details-Our%20Journey%20to%20Touch%20the%20Sun%20is%20Underway%20on%20This%20Week%20@NASA%20%E2%80%93%20August%2017,%202018.html

NASA's Parker Solar Probe is beginning its mission to the Sun after a successful launch Aug. 12 aboard a United Launch Alliance Delta IV Heavy rocket. The mission was first proposed in 1958 by heliophysics pioneer Dr. Eugene Parker, who viewed the launch from Kennedy and anticipates new discoveries from his namesake spacecraft.

Be sure to watch to the end for a Parker Solar Probe Dedication! aurora shows, especially at high latitudes. Two coronal holes are rotating through the Earth-strike zone, which means Earth will be preconditioned for activity! The news for amateur radio operators is not so great, as the last remaining bright region on the Earth-facing Sun rotates to the Sun's backside out of view. Solar flux has dropped and we are back at poor levels for radio propagation on Earth's dayside. Unfortunately, these conditions could easily continue over the next week or more. Learn the details of the coming solar storm, see why GPS users are smiling, and why "CW" for amateur radio operators may be the mode of choice. For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

A United Launch Alliance (ULA) Delta IV Heavy rocket carrying NASA’s Parker Solar Probe mission to the sun lifts off from Space Launch Complex-37 at Cape Canaveral Air Force Station, Florida, on Aug. 12, 2018. The mission is humanity’s first journey to the sun. Check out Dr. Eugene N. Parker watching the rocket set of on its journey to space.

NASA is launching humanity’s first ever mission to touch the Sun, and it could solve two of the most vexing mysteries in astrophysics. Watch More Space Crafts! | https://bit.ly/2w0YKD1 Read More: Parker Solar Probe https://www.nasa.gov/content/goddard/parker-solar-probe “NASA’s Parker Solar Probe will be the first-ever mission to ‘touch’ the Sun.” Launch Week Begins for Parker Solar Probe https://blogs.nasa.gov/parkersolarprobe/2018/08/07/launch-week-begins-for-parker-solar-probe/ “Teams preparing for launch of NASA’s Parker Solar Probe are beginning a busy week leading up to liftoff, scheduled for Saturday, Aug. 11, at 3:33 a.m.” Parker Solar Probe - Spacecraft http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Extreme-Environments “PSP will perform its scientific investigations in a hazardous region of intense heat and solar radiation. The spacecraft will fly close enough to the Sun to watch the solar wind speed up from subsonic to supersonic, and it will fly though the birthplace of the highest-energy solar particles.” ____________________ Seeker inspires us to see the world through the lens of science and evokes a sense of curiosity, optimism and adventure. Visit the Seeker website http://www.seeker.com/ Subscribe now! http://www.youtube.com/subscription_center?add_user=dnewschannel Seeker on Twitter http://twitter.com/seeker Seeker on Facebook https://www.facebook.com/SeekerMedia/ Space Crafts on Facebook https://www.facebook.com/SeekerSpaceCrafts/ Seeker http://www.seeker.com/

Watch and discuss live as United Launch Alliance (ULA) runs a second attempt to launch their Delta IV Heavy rocket with NASA’s Parker Solar Probe. The largest of the Delta 4 family, the Heavy version features three Common Booster Cores mounted together to form a triple-body rocket. The Parker Solar Probe will be the first-ever mission to “touch” the sun, or to directly contact the coronal material in the sun's fiercely hot upper atmosphere. During its seven-year mission orbiting the sun the probe, which is about the size of a small car, will swoop as close as 4 million miles (6.4 million kilometers) to the sun's photosphere, which is the layer of the star we think of as the surface. @OLHZN Discord Server: https://discord.gg/D55u3fa 1st launch attempt live stream: https://www.youtube.com/watch?v=dgpKY3I2Q0k ************************************************************** Donate to our 501(c)(3) non-profit charitable organization here: Donorbox: https://donorbox.org/olhzn Paypal Charity: https://www.paypal.com/fundraiser/charity/2727446 Amazon Smile: https://smile.amazon.com/ch/82-3099711 ************************************************************** Learn more about our weather balloon flights, data & videos at: http://overlookhorizon.com To learn more about our Arduino based flight computer, APRS transmitter, RTTY radio transmitter, ham radio balloon tracking methods or any of our other onboard technology and data sensors; visit http://overlookhorizon.com OUR FLIGHT SYSTEMS: Styrofoam Cooler: http://amzn.to/2pLYNkz Arduino MEGA: http://amzn.to/2pMh3KC Lightdow LD4000 Action Camera: http://amzn.to/2qFlsNu Rocketman Parachute: http://amzn.to/2pecXrx Adafruit PowerBoost: http://amzn.to/2q4v2fL uBlox Neo 6M GPS: http://amzn.to/2pMfUm1 DS18b20 Temperature Sensor: http://amzn.to/2qK4goZ Data Logging Shield: http://amzn.to/2pengvC BMP180 Pressure Sensor: http://amzn.to/2pLcSMW Piezo Speaker Alarm: http://amzn.to/2q4AEXb Orbtronics 18650 Lithium Ion Batteries: http://amzn.to/2pLD4XW Radar Reflector: http://amzn.to/2fmY7il Please Donate! Overlook Horizon Inc. is a 501(c)(3) non-profit charitable organization in the United States. If you're a fan of our high altitude balloon / weather balloon adventures and videos, please consider making a donation to our organization that is 100% tax-deductible in the US! Donations help us raise funds to to facilitate more flights, launches and adventures that we can share with students of all ages. We want to expand our reach and provide students a hands on opportunity to build, fly and analyze the science behind high altitude balloons, outer space and engineering. Any help is greatly appreciated. Donate Here: http://overlookhorizon.com/donate Connect on Facebook: https://www.facebook.com/overlookhorizon Instagram: https://www.instagram.com/olhzn Twitter: https://twitter.com/OLHZN Website: http://www.overlookhorizon.com Donate: https://donorbox.org/olhzn Support amateur space flight by purchasing a high altitude balloon (weather balloon) t-shirt from our apparel store: http://overlookhorizon.com/shirts Patch/Sticker giveaways: No Purchase Necessary. Purchase/donation does not enhance chance of winning. Void where prohibited or restricted by law. Valid only during the live broadcast. Official Rules: http://www.overlookhorizon.com/youtube-giveaway-rules/ -~-~~-~~~-~~-~- Watch a full flight with beautiful views from launch to the stratosphere and back over Finger Lakes in NY: https://www.youtube.com/watch?v=RZwq86wWknk -~-~~-~~~-~~-~-

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NASA launches its Parker Solar Probe to explore the sun's atmosphere.

NASA’s Parker Solar Probe mission launched Aug. 11 from Cape Canaveral Air Force Station in Florida. The mission will be the first to fly directly through the Sun’s corona – the hazardous region of intense heat and solar radiation in the Sun’s atmosphere that is visible during an eclipse. It will gather data that could help answer questions about solar physics that have puzzled scientists for decades. Gathering information about fundamental processes near the Sun can help improve our understanding of how our solar system’s star changes the space environment, where space weather can affect astronauts, interfere with satellite orbits, or damage spacecraft electronics. This video is available for download from NASA's Image and Video Library: https://images.nasa.gov/details-NHQ_2018_0812_Parker%20Solar%20Probe%20Mission%20Launches%20to%20Touch%20the%20Sun%20-.html

Following a postponement due to a violation of a launch limit, the countdown again is underway for the liftoff of NASA's Parker Solar Probe, atop a United Launch Alliance Delta IV Heavy rocket from Space Launch Complex 37 at Cape Canaveral Air Force Station. The probe will rely on measurements and imaging to revolutionize our understanding of the corona and the Sun-Earth connection. Liftoff is scheduled to lift off at 3:31 a.m. EDT on Aug. 12, 2018.

This launch attempt was scrubbed. Watch the next attempt here: https://www.youtube.com/watch?v=P34INukI6fw Watch and discuss live as United Launch Alliance (ULA) launches their Delta IV Heavy rocket with NASA’s Parker Solar Probe. The largest of the Delta 4 family, the Heavy version features three Common Booster Cores mounted together to form a triple-body rocket. The Parker Solar Probe will be the first-ever mission to “touch” the sun, or to directly contact the coronal material in the sun's fiercely hot upper atmosphere. During its seven-year mission orbiting the sun the probe, which is about the size of a small car, will swoop as close as 4 million miles (6.4 million kilometers) to the sun's photosphere, which is the layer of the star we think of as the surface. @OLHZN Discord Server: https://discord.gg/D55u3fa ************************************************************** Donate to our 501(c)(3) non-profit charitable organization here: Donorbox: https://donorbox.org/olhzn Paypal Charity: https://www.paypal.com/fundraiser/charity/2727446 Amazon Smile: https://smile.amazon.com/ch/82-3099711 ************************************************************** Learn more about our weather balloon flights, data & videos at: http://overlookhorizon.com To learn more about our Arduino based flight computer, APRS transmitter, RTTY radio transmitter, ham radio balloon tracking methods or any of our other onboard technology and data sensors; visit http://overlookhorizon.com OUR FLIGHT SYSTEMS: Styrofoam Cooler: http://amzn.to/2pLYNkz Arduino MEGA: http://amzn.to/2pMh3KC Lightdow LD4000 Action Camera: http://amzn.to/2qFlsNu Rocketman Parachute: http://amzn.to/2pecXrx Adafruit PowerBoost: http://amzn.to/2q4v2fL uBlox Neo 6M GPS: http://amzn.to/2pMfUm1 DS18b20 Temperature Sensor: http://amzn.to/2qK4goZ Data Logging Shield: http://amzn.to/2pengvC BMP180 Pressure Sensor: http://amzn.to/2pLcSMW Piezo Speaker Alarm: http://amzn.to/2q4AEXb Orbtronics 18650 Lithium Ion Batteries: http://amzn.to/2pLD4XW Radar Reflector: http://amzn.to/2fmY7il Please Donate! Overlook Horizon Inc. is a 501(c)(3) non-profit charitable organization in the United States. If you're a fan of our high altitude balloon / weather balloon adventures and videos, please consider making a donation to our organization that is 100% tax-deductible in the US! Donations help us raise funds to to facilitate more flights, launches and adventures that we can share with students of all ages. We want to expand our reach and provide students a hands on opportunity to build, fly and analyze the science behind high altitude balloons, outer space and engineering. Any help is greatly appreciated. Donate Here: http://overlookhorizon.com/donate Connect on Facebook: https://www.facebook.com/overlookhorizon Instagram: https://www.instagram.com/olhzn Twitter: https://twitter.com/OLHZN Website: http://www.overlookhorizon.com Donate: https://donorbox.org/olhzn Support amateur space flight by purchasing a high altitude balloon (weather balloon) t-shirt from our apparel store: http://overlookhorizon.com/shirts Patch/Sticker giveaways: No Purchase Necessary. Purchase/donation does not enhance chance of winning. Void where prohibited or restricted by law. Valid only during the live broadcast. Official Rules: http://www.overlookhorizon.com/youtube-giveaway-rules/ -~-~~-~~~-~~-~- Watch a full flight with beautiful views from launch to the stratosphere and back over Finger Lakes in NY: https://www.youtube.com/watch?v=RZwq86wWknk -~-~~-~~~-~~-~-

You guys have heard of this right? Just a friendly reminder that it's launching tonight and the Delta IV always puts on a good show.

A United Launch Alliance Delta IV Heavy rocket will launch NASA's Parker Solar Probe mission to the sun. The Parker Solar Probe mission will be the 10th launch of the Delta IV Heavy configuration rocket, which is the only rocket currently flying with the capability of launching this mission.

It will take multiple rockets and a series of gravity assists to put the newest solar probe where it needs to be. Learn more about this story at www.newsy.com/82396/ Find more videos like this at www.newsy.com Follow Newsy on Facebook: www.facebook.com/newsyvideos Follow Newsy on Twitter: www.twitter.com/newsy

The Parker Solar Probe will be the first-ever mission to "touch" the Sun, traveling directly into the Sun's atmosphere about 4 million miles from the surface. Read the story: https://go.nasa.gov/2KEExYZ NASA launch schedule: https://go.nasa.gov/2JfklMB The Sun contains 99.8 of the mass in our solar system. Its gravitational pull is what keeps everything here, from tiny Mercury to the gas giants to the Oort Cloud, 186 billion miles away. But even though the Sun has such a powerful pull, it's surprisingly hard to actually go to the Sun: It takes 55 times more energy to go to the Sun than it does to go to Mars. Why is it so difficult? The answer lies in the same fact that keeps Earth from plunging into the Sun: Our planet is traveling very fast - about 67,000 miles per hour - almost entirely sideways relative to the Sun. The only way to get to the Sun is to cancel that sideways motion. Since Parker Solar Probe will skim through the Sun's atmosphere, it only needs to drop 53,000 miles per hour of sideways motion to reach its destination, but that's no easy feat. In addition to using a powerful rocket, the Delta IV Heavy, Parker Solar Probe will perform seven Venus gravity assists over its seven-year mission to shed sideways speed into Venus' well of orbital energy. These gravity assists will draw Parker Solar Probe's orbit closer to the Sun for a record approach of just 3.83 million miles from the Sun's visible surface on the final orbits. Though it's shedding sideways speed to get closer to the Sun, Parker Solar Probe will pick up overall speed, bolstered by Sun's extreme gravity - so it will also break the record for the fastest-ever human-made objects, clocking in at 430,000 miles per hour on its final orbits. Music: Percs and Pizz from Killer Tracks. Credit: NASA's Godddard Space flight Center

In this video, we look at the Solar Parker Probe in detail. First by understanding who Dr. Parker was, and what he theorized about Solar Winds. Then we go into how the probe will make it to the Sun, using multiple gravity assists of Venus. After that, we discuss the Corona of the Sun, and how the probe will be able to survive the high-temperature environment with it’s innovative and autonomous design. Then we look at the different instrument onboard, and what they will be able to tell us about solar winds. If you are interested in reading more about this topic, check out the official NASA page: https://www.nasa.gov/content/goddard/parker-solar-probe-humanity-s-first-visit-to-a-star Thanks for watching! And consider subscribing if you enjoyed this video! Twitter: https://twitter.com/wolf_martian Facebook: https://fb.me/MartianWolf Patreon: https://www.patreon.com/MartianWolf Heading Home by Nekzlo @nekzlo Music provided by Free Music for Vlogs youtu.be/YGL35p7LLqo ------------------------------ • Contact the artist: @nekzlo www.instagram.com/nekzlo/ twitter.com/Nekzlo_Music open.spotify.com/artist/75LSn0DiQyH6LnHBT8fOEK ------------------------------ #Sun #NASA

NASA is going to fly its Parker Solar Probe closer to the sun than any spacecraft in history. The probe's mission is to study the solar corona to better protect our tech-driven lifestyle against destructive solar storms that could take us back to the stone ages. Tech Insider tells you all you need to know about tech: gadgets, how-to's, gaming, science, digital culture, and more. Subscribe to our channel and visit us at: http://www.businessinsider.com/sai TI on Facebook: https://www.facebook.com/techinsider TI on Instagram: https://www.instagram.com/tech_insider/ TI on Twitter: https://twitter.com/techinsider INSIDER on Snapchat: https://insder.co/2KJLtVo

The Parker Solar Probe will help scientists learn more about the solar wind, an exotic stew of magnetic forces, plasma and particles. NASA Science: http://science.nasa.gov/

UC Berkeley's Phyllis Whittlesey, instrument lead for the SPAN electron analyzers, and Davin Larson, institutional principal investigator, discuss the Solar Wind Electrons Alphas and Protons (SWEAP) investigation and how it will help scientists make precise measurements of particles in the solar wind. Learn more: https://www.nasa.gov/content/goddard/... http://parkersolarprobe.jhuapl.edu/

Johns Hopkins APL's Jennifer Fischer, deputy systems assurance manager, and Research Support Instruments' Mark Boies, WISPR instrument systems engineer, discuss the spacecraft's sole white-light imaging instrument. WISPR - the Wide-field Imager for Solar PRobe (WISPR) - consists of two telescopes that will take images of the solar corona and inner heliosphere. The experiment will also provide images of the solar wind, shocks and other structures as they approach and pass the spacecraft. Learn more: https://www.nasa.gov/content/goddard/parker-solar-probe http://parkersolarprobe.jhuapl.edu/

Johns Hopkins APL's Eric Wallis, lead thermal multi-layer insulation engineer, discusses the spacecraft's custom built thermal blankets role and function with APL's Felipe Ruiz, deputy lead mechanical engineer. We also get to see the thermal blanket team - Neal Bachtell, Tony Ahan, Lynsey Gwilliam, and Helen O'Conner - at work installing Parker Solar Probe's critical thermal blankets. Learn more: https://www.nasa.gov/content/goddard/... http://parkersolarprobe.jhuapl.edu/

On June 27, 2018, Parker Solar Probe’s heat shield – called the Thermal Protection System, or TPS – was installed on the spacecraft. A mission sixty years in the making, Parker Solar Probe will make a historic journey to the Sun’s corona, a region of the solar atmosphere. With the help of its revolutionary heat shield, now permanently attached to the spacecraft in preparation for its August 2018 launch, the spacecraft’s orbit will carry it to within 4 million miles of the Sun's fiercely hot surface, where it will collect unprecedented data about the inner workings of the corona. The eight-foot-diameter heat shield will safeguard everything within its umbra, the shadow it casts on the spacecraft. At Parker Solar Probe’s closest approach to the Sun, temperatures on the heat shield will reach nearly 2,500 degrees Fahrenheit, but the spacecraft and its instruments will be kept at a relatively comfortable temperature of about 85 degrees Fahrenheit. The heat shield is made of two panels of superheated carbon-carbon composite sandwiching a lightweight 4.5-inch-thick carbon foam core. The Sun-facing side of the heat shield is also sprayed with a specially formulated white coating to reflect as much of the Sun’s energy away from the spacecraft as possible. The heat shield itself weighs only about 160 pounds – here on Earth, the foam core is 97% air. Learn more at https://www.nasa.gov/content/goddard/parker-solar-probe http://parkersolarprobe.jhuapl.edu/index.php

Project Scientist Nicky Fox of Johns Hopkins APL and APL Space Exploration Sector Head Mike Ryschkewitsch talk about the amazing team and dedication needed to produce Parker Solar Probe: the coolest, hottest mission under the Sun. Learn more: https://www.nasa.gov/content/goddard/... http://parkersolarprobe.jhuapl.edu/

The University of Michigan's Justin Kasper, principal investigator for the Solar Wind Electrons Alphas and Protons (SWEAP) Investigation, discusses how the instruments of SWEAP will count the most abundant particles in the solar wind -- electrons, protons and helium ions -- and measure their properties such as velocity, density, and temperature. SWEAP includes the Solar Probe Cup, which is the only instrument mounted outside the protective heat shield of the spacecraft. Learn more: https://www.nasa.gov/content/goddard/... http://parkersolarprobe.jhuapl.edu/

In In this video. we look at NASA's Parker Solar Probe, which is expected to Launch later this week. We discuss why this mission is important, how it will help scientists understand Solar Winds, and what we will be able to do with that information. We also briefly discuss some key aspects of the probe itself, and what it is able to do. Thanks for watching! And consider subscribing if you enjoyed this video! Twitter: https://twitter.com/wolf_martian Facebook: https://fb.me/MartianWolf Patreon: https://www.patreon.com/MartianWolf Heading Home by Nekzlo @nekzlo Music provided by Free Music for Vlogs youtu.be/YGL35p7LLqo ------------------------------ • Contact the artist: @nekzlo www.instagram.com/nekzlo/ twitter.com/Nekzlo_Music open.spotify.com/artist/75LSn0DiQyH6LnHBT8fOEK ------------------------------ #TouchtheSun

The Wide-Field Imager for Parker Solar Probe is the only imaging instrument aboard the spacecraft. WISPR looks at the large-scale structure of the corona and solar wind before the spacecraft flies through it. About the size of a shoebox, WISPR takes images from afar of structures like coronal mass ejections, or CMEs, jets and other ejecta from the Sun. These structures travel out from the Sun and eventually overtake the spacecraft, where the spacecraft’s other instruments take in-situ measurements. WISPR helps link what’s happening in the large-scale coronal structure to the detailed physical measurements being captured directly in the near-Sun environment. WISPR was designed and developed by the Solar and Heliophysics Physics Branch at the Naval Research Laboratory in Washington, DC (principal investigator Russell Howard), which will also develop the observing program. Learn more: http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Instruments

NASA’s coolest hottest mission is getting closer to launch. The Parker Solar Probe was transported to the pad and lifted into place atop the United Launch Alliance Delta IV Heavy rocket that will carry it into space. Chuck Dovale, deputy program manager for the Launch Services Program, was among three employees who received a Distinguished Service Medal presented by NASA Administrator Jim Bridenstine.

Surveyor of the invisible forces, the FIELDS instrument suite captures the scale and shape of electric and magnetic fields in the Sun’s atmosphere. FIELDS measures waves and turbulence in the inner heliosphere with high time resolution to understand the fields associated with waves, shocks and magnetic reconnection, a process by which magnetic field lines explosively realign FIELDS was designed, built, and is operated by a team lead by the Space Sciences Laboratory at the University of California, Berkeley (principal investigator Stuart D. Bale) Learn more: http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Instruments

Viewers like you help make PBS (Thank you 😃) . Support your local PBS Member Station here: https://to.pbs.org/DonateSPACE Parker Space Probe successfully launched on August 12!!! http://parkersolarprobe.jhuapl.edu/ Help Us with the PBS Digital Studios Survey: https://to.pbs.org/2018YTSurvey Check Out PBS ReInventors: http://youtube.com/pbsreinventors You can further support us on Patreon at https://www.patreon.com/pbsspacetime Get your own Space Time t­-shirt at http://bit.ly/1QlzoBi Tweet at us! @pbsspacetime Facebook: facebook.com/pbsspacetime Email us! pbsspacetime [at] gmail [dot] com Comment on Reddit: http://www.reddit.com/r/pbsspacetime Help translate our videos! https://www.youtube.com/timedtext_cs_... Previous Episode: Reversing Entropy with Maxwell's Demon https://youtu.be/KR23aMjIHIY The Sun: an entity worshipped as a god throughout time and across cultures. The source of all life and sustenance for our little blue space rock, and also a force of unthinkable destructive power. But soon humanity will reach out its collective hand and come closer to touching the Sun than we ever have before with the launch of the Parker Solar Probe. Hosted by Matt O'Dowd Written by Drew Rosen and Matt O'Dowd Graphics by Grayson Blackmon Assistant Editing and Sound Design by Mike Petrow Made by Kornhaber Brown (www.kornhaberbrown.com) Special thanks to our Patreon Big Bang, Quasar and Hypernova Supporters: Big Bang CoolAsCats David Nicklas Anton Lifshits Joey Redner Fabrice Eap Quasar Tambe Barsbay Mayank M. Mehrota Mars Yentur Mark Rosenthal Dean Fuqua Roman Pinchuk ColeslawPurdie Vinnie Falco Hypernova Donal Botkin Edmund Fokschaner Matthew O’Connor Eugene Lawson Barry Hatfield Martha Hunt Joseph Salomone Chuck Zegar Craig Peterson Jordan Young Ratfeast John Hofmann Thanks to our Patreon Gamma Ray Burst Supporters: James Hughes Fabian Olesen Kris Fernet Jane Meyers James Flowers Greg Allen Denys Ivanov Nick Virtue Alexey Eromenko Nicholas Rose Scott Gossett Mark Vasile Patrick Murray سلطان الخليفي Alex Seto Michal-Peanut Karmi Erik Stein Kevin Warne JJ Bagnell Avi Goldfinger John Pettit Florian Stinglmayr Benoit Pagé-Guitard Nathan Leniz Brandon Labonte David Crane Greg Weiss Shannan Catalano Brandon Cook

Eugene Parker, professor emeritus of physics at the University of Chicago, and namesake of NASA's Parker Solar Probe mission, discusses his work in solar physics and the spacecraft that bears his name with Parker Solar Probe project scientist Nicola Fox, from the Johns Hopkins Applied Physics Lab. Parker Solar Probe is part of NASA’s Living With a Star program to explore aspects of the Sun-Earth system that directly affect life and society. The Living With a Star flight program is managed by the agency’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate in Washington. The Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland, manages the mission for NASA. APL designed and built the spacecraft and will also operate it. Thanks to the University of Chicago for footage and images of Dr. Parker Learn more at https://www.nasa.gov/content/goddard/parker-solar-probe and http://parkersolarprobe.jhuapl.edu/index.php

The Integrated Science Investigation of the Sun—IS☉IS, pronounced ee-sis and including the symbol for the Sun in its acronym—on board Parker Solar Probe uses two complementary instruments in one combined scientific investigation to measure particles across a wide range of energies. By measuring electrons, protons and ions, IS☉IS will understand the particles’ life cycles—where they came from, how they became accelerated and how they move out from the Sun through interplanetary space The two energetic particle instruments on IS☉IS are called EPI-Lo and EPI-Hi (EPI stands for Energetic Particle Instrument). IS☉IS is led by Princeton University in Princeton, New Jersey (principal investigator David McComas), and was built largely at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, and Caltech, in Pasadena, California, with significant contributions from Southwest Research Institute in San Antonio, Texas, and NASA’s Goddard Space Flight Center in Greenbelt, Maryland The IS☉IS Science Operations Center is operated at the University of New Hampshire in Durham. Learn more: http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Instruments

NASA's aiming to answer "three foundational questions" about the sun. Learn more about this story at www.newsy.com/81879/ Find more videos like this at www.newsy.com Follow Newsy on Facebook: www.facebook.com/newsyvideos Follow Newsy on Twitter: www.twitter.com/newsy

ULA Trajectory Engineer Nick Driver on launching NASA's Parker Solar Probe mission atop ULA's Delta IV Heavy rocket. Usually used for large satellites, in this case the heavy lifter is being used to give a small spacecraft a high-energy delivery to the sun.

NASA's Parker Solar Probe will explore the sun's atmosphere wearing a nearly 5-inch coat of carbon-composite solar shields. According to CNN, the mission is expected to launch in early August. This is NASA's first mission to the sun and its outermost atmosphere. It's not a mission that any human can make, so NASA is sending a roughly 10-foot-high probe on the historic mission. The probe will be closer to the sun than any spacecraft has ever reached before. https://www.cnn.com/2018/07/20/us/nasa-parker-solar-probe/index.html http://www.wochit.com This video was produced by YT Wochit Tech using http://wochit.com

NASA's Parker Solar Probe is heading to the Sun. Why won't the spacecraft melt? Thermal Protection System Engineer Betsy Congdon (Johns Hopkins APL) outlines why Parker can take the heat. Read more: https://www.nasa.gov/feature/goddard/2018/traveling-to-the-sun-why-won-t-parker-solar-probe-melt Music credit: Cheeky Chappy [Main Track] by Jimmy Kaleth, Ross Andrew McLean Credit: NASA's Goddard Space Flight Center Genna Duberstein (USRA): Lead Producer/Lead Editor Rob Andreoli (AIMM): Lead Videographer Betsy Congdon (Johns Hopkins University/APL): Lead Engineer Ryan Fitzgibbons (USRA): Narrator Genna Duberstein (USRA): Writer Steve Gribben (Johns Hopkins University/APL ): Animator Brian Monroe (USRA): Animator Josh Masters (USRA): Animator Michael Lentz (USRA): Animator Genna Duberstein (USRA): Animator Mary P. Hrybyk-Keith (TRAX International Corporation): Illustrator This video is public domain and along with other supporting visualizations can be downloaded from the Scientific Visualization Studio at: https://svs.gsfc.nasa.gov/12867 If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAExplorer Follow NASA’s Goddard Space Flight Center · Facebook: https://www.facebook.com/NASA.GSFC · Twitter https://twitter.com/NASAGoddard · Flickr https://www.flickr.com/photos/gsfc/ · Instagram https://www.instagram.com/nasagoddard/