Whats the best metaphor/ explanation of blackholes youve ever heard?
Did you miss it? Astronaut Scott Kelly answered questions over the weekend on People Magazine’s Facebook page! Anything and everything from his favorite food in space to his year aboard the International Space Station.
Here are a few highlights from the conversation:
Follow Astronaut Scott Kelly during the remainder of his year in space: Facebook, Twitter, Instagram
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It’s the 1970s, and we’re about to send two spacecraft (Voyager 1 & 2) into space. These two spacecraft will eventually leave our solar system and become the most distant man-made objects…ever. How can we leave our mark on them in the case that other spacefarers find them in the distant future?
The Golden Record.
We placed an ambitious message aboard Voyager 1 and 2, a kind of time capsule, intended to communicate a story of our world to extraterrestrials. The Voyager message is carried by a phonograph record, a 12-inch gold-plated copper disk containing sounds and images selected to portray the diversity of life and culture on Earth.
The Golden Record Cover
The outward facing cover of the golden record carries instructions in case it is ever found. Detailing to its discoverers how to decipher its meaning.
In the upper left-hand corner is an easily recognized drawing of the phonograph record and the stylus carried with it. The stylus is in the correct position to play the record from the beginning. Written around it in binary arithmetic is the correct time of one rotation of the record. The drawing indicates that the record should be played from the outside in.
The information in the upper right-hand portion of the cover is designed to show how the pictures contained on the record are to be constructed from the recorded signals. The top drawing shows the typical signal that occurs at the start of the picture. The picture is made from this signal, which traces the picture as a series of vertical lines, similar to ordinary television. Immediately below shows how these lines are to be drawn vertically, with staggered “interlace” to give the correct picture rendition. Below that is a drawing of an entire picture raster, showing that there are 52 vertical lines in a complete picture.
Immediately below this is a replica of the first picture on the record to permit the recipients to verify that they are decoding the signals correctly. A circle was used in this picture to ensure that the recipients use the correct ratio of horizontal to vertical height in picture reconstruction.
The drawing in the lower left-hand corner of the cover is the pulsar map previously sent as part of the plaques on Pioneers 10 and 11. It shows the location of the solar system with respect to 14 pulsars, whose precise periods are given.
The drawing containing two circles in the lower right-hand corner is a drawing of the hydrogen atom in its two lowest states, with a connecting line and digit 1 to indicate that the time interval associated with the transition from one state to the other is to be used as the fundamental time scale, both for the time given on the cover and in the decoded pictures.
The Contents
The contents of the record were selected for NASA by a committee chaired by Carl Sagan of Cornell University and his associates.
They assembled 115 images and a variety of natural sounds, such as those made by surf, wind and thunder, birds, whales and other animals. To this, they added musical selections from different cultures and eras, and spoken greetings from Earth-people in fifty-five languages, and printed messages from President Carter and U.N. Secretary General Waldheim.
Listen to some of the sounds of the Golden Record on our Soundcloud page:
Golden Record: Greetings to the Universe
Golden Record: Sounds of Earth
Songs from Chuck Berry’s “Johnny B. Goode,” to Beethoven’s Fifth Symphony are included on the golden record. For a complete list of songs, visit: https://voyager.jpl.nasa.gov/golden-record/whats-on-the-record/music/
The 115 images included on the record, encoded in analog form, range from mathematical definitions to humans from around the globe. See the images here: https://voyager.jpl.nasa.gov/golden-record/whats-on-the-record/images/
Making the Golden Record
Many people were instrumental in the design, development and manufacturing of the golden record.
Blank records were provided by the Pyral S.A. of Creteil, France. CBS Records contracted the JVC Cutting Center in Boulder, CO to cut the lacquer masters which were then sent to the James G. Lee Record Processing center in Gardena, CA to cut and gold plate eight Voyager records.
The record is constructed of gold-plated copper and is 12 inches in diameter. The record’s cover is aluminum and electroplated upon it is an ultra-pure sample of the isotope uranium-238. Uranium-238 has a half-life of 4.468 billion years.
Learn more about the golden record HERE.
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Soaring over traffic in an air taxi, receiving packages faster, and participating in a sustainable, safer mode of transportation: all could be possible with a revolutionary new type of air transportation system in development called Advanced Air Mobility (AAM).
AAM could include new aircraft developed by industry, called electric vertical takeoff and landing vehicles, or eVTOLs, for use in passenger, package, or cargo delivery. It may also include new places for these aircraft to take off and land called vertiports.
Our work in Advanced Air Mobility will transform the way people and goods will move through the skies. This includes using Advanced Air Mobility for public good missions such as disaster, medical, and wildfire response.
Our vision for Advanced Air Mobility is to map out a safe, accessible, and affordable new air transportation system alongside industry, community partners, and the Federal Aviation Administration.
Once developed, passengers and cargo will travel on-demand in innovative, automated aircraft called eVTOLs, across town, between neighboring cities, or to other locations typically accessed today by car.
The addition of Advanced Air Mobility will benefit the public in several ways: easier access for travelers between rural, suburban, and urban communities; rapid package delivery; reduced commute times; disaster response, and new solutions for medical transport of passengers and supplies.
Various NASA simulation and flight testing efforts will study noise, automation, safety, vertiports, airspace development and operations, infrastructure, and ride quality, along with other focus areas like community integration.
These areas all need to be further researched before Advanced Air Mobility could be integrated into our skies. We’re helping emerging aviation markets navigate the creation of this new transportation system.
We provide various test results to the FAA to help with new policy and standards creation. We aim to give industry and the FAA recommendations for requirements to build a scalable Advanced Air Mobility system to help enable the industry to flourish by 2030.
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Big news for our Nancy Grace Roman Space Telescope! Thanks to some new “shades” – an infrared filter that will help us see longer wavelengths of light – the mission will be able to spot water ice on objects in the outer solar system, see deeper into clouds of gas and dust, and peer farther across space. We’re gearing up for some super exciting discoveries!
You probably know that our solar system includes planets, the Sun, and the asteroid belt in between Mars and Jupiter – but did you know there’s another ‘belt’ of small objects out past Neptune? It’s called the Kuiper belt, and it’s home to icy bodies that were left over from when our solar system formed.
A lot of the objects there are like cosmic fossils – they haven’t changed much since they formed billions of years ago. Using its new filter, Roman will be able to see how much water ice they have because the ice absorbs specific wavelengths of infrared light, providing a “fingerprint” of its presence. This will give us a window into the solar system’s early days.
Clouds of dust and gas drift throughout our galaxy, sometimes blocking our view of the stars behind them. It’s hard for visible light to penetrate this dusty haze because the particles are the same size or even larger than the light’s wavelength. Since infrared light travels in longer waves, it hardly notices the tiny particles and can pass more easily through dusty regions.
With Roman’s new filter, we’ll be able to see through much thicker dust clouds than we could have without the upgrade. It’ll be much easier to study the structure of our home galaxy, the Milky Way.
Roman’s expanded view will also help us learn more about brown dwarfs – objects that are more massive than planets, but not massive enough to light up like stars. The mission will find them near the heart of the galaxy, where stars explode more often.
These star explosions, called supernovae, are so extreme that they create and disperse new elements. So near the center of the galaxy, there should be higher amounts of elements that aren’t as common farther away, where supernovae don’t happen as often.
Astronomers think that may affect how stars and planets form. Using the new filter, Roman will probe the composition of brown dwarfs to help us understand more.
Roman’s upgraded filter will also help us see farther across space. As light travels through our expanding universe, its wavelength becomes stretched. The longer it travels before reaching us, the longer its wavelength becomes. Roman will be able to see so far back that we could glimpse some of the first stars and galaxies that ever formed. Their light will be so stretched that it will mostly arrive as infrared instead of visible light.
We’re still not sure how the very first galaxies formed because we’ve found so few of these super rare and faint beasts. But Roman will have such a big view of the universe and sharp enough vision that it could help us find a lot more of them. Then astronomers can zoom in on them with missions like our James Webb Space Telescope for a closer look.
Roman will help us explore these cosmic questions and many more! Learn more about the mission here: https://roman.gsfc.nasa.gov/
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After moving quite slowly for decades, the outlet glacier of Vavilov Ice Cap began sliding dozens of times faster than is typical. The ice moved fast enough for the fan-shaped edge of the glacier to protrude from an ice cap on October Revolution Island and spread widely across the Kara Sea. The Landsat images above were acquired on July 1, 2013, June 18, 2015, and June 24, 2018, respectively.
“The fact that an apparently stable, cold-based glacier suddenly went from moving 20 meters per year to 20 meters per day was extremely unusual, perhaps unprecedented,” said University of Colorado Boulder glaciologist Michael Willis. “The numbers here are simply nuts. Before this happened, as far as I knew, cold-based glaciers simply didn’t do that...couldn’t do that.”
Willis and his colleagues are still piecing together what triggered such a dramatic surge. They suspect that marine sediments immediately offshore are unusually slippery, perhaps containing clay. Also, water must have somehow found its way under the land-based part of the glacier, reducing friction and priming the ice to slide.
Full story here: go.nasa.gov/2Z931lc
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How does time work in a black hole?
How exactly will it work? And whats the goal of the project?
The International Space Station is a perfect environment for creating protein crystal structures for research.
In microgravity, protein molecules form more orderly, high-quality crystals. Studying these structures helps scientists understand their function and contributes to development of more effective treatments for diseases.
Experiments often need more than one try to generate ideal crystals, though. Researchers may have to return samples to Earth for analysis and then try again on a later mission on the space station.
Scientists are testing new methods of growing crystals that allow crew members to observe imperfections, make real-time adjustments, and try growing them again right away. This dramatically reduces the time and cost of conducting experiments aboard the space station and opens up the orbiting lab to more users. More efficient use of time and resources can produce research results in less time and lead to development of better drugs sooner.
Learn more @ISS_Research!
Have you ever wanted to design something that could fly around the Moon? This is your opportunity. The Artemis II astronauts will use a zero gravity indicator during their mission to demonstrate when the Orion spacecraft has reached microgravity. This plushie needs to be soft, small, and importantly, remind us of home. The Moon Mascot contest challenges people of all ages from all over the world to submit a design to be made by NASA’s Thermal Blanket Lab and flown aboard Artemis II. To submit a design for the contest, visit: freelancer.com/moon-mascot
Hello! @Astro_Jessica here ready to take your @nasa questions! @sxsw
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