If I landed on the moon I would simply not have stomach issues due to drinking high-potassium orange juice.
RIP to John Young but I’m different
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let's talk about Bridgerton tea, my ask is open

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YOU ARE THE REASON
he wasn't even looking at me and he found me
One Nice Bug Per Day

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will byers stan first human second

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If I landed on the moon I would simply not have stomach issues due to drinking high-potassium orange juice.
RIP to John Young but I’m different
fuck everything else happy birthday sputnik
Inside - Vadim Sadovski
The Poles of Mars.
L: The North Pole, pictured down to the equator R: The South Pole, in more detail
Credit: ESA
Ferrofluids – those distinctively spiky liquids – are made up of magnetically sensitive nanoparticles in a carrier liquid, and although they respond to applied magnetic fields, they retain no magnetism outside of that field. But researchers have now succeeded in making actual liquid magnets. Shown above, these drops also contain ferromagnetic nanoparticles. But unlike traditional ferrofluids, in these drops the nanoparticles are not entirely free to move. They’re jammed together at the interface, so when a magnetic field is applied, the nanoparticles will align like tiny bar magnets. When that magnetic field is removed, though, the nanoparticles cannot easily reconfigure, so they remain aligned and the drops continue being magnetic.
Researchers hope these ultrasoft magnets, which can be manipulated remotely through magnetic fields, will be useful in the future for applications like targeted drug delivery. In theory one could introduce, say, chemotherapy drugs into one of these liquid magnets, then use magnetic fields to guide it directly to a cancerous tumor. (Image and research credit: X. Liu et al.; via Science News; submitted by Kam-Yung Soh)
Starry Greetings!
Here is comic 1 out of 2 for the last month of aquatic space month!
This topic is about: The watery disk of a black hole!
https://news.nationalgeographic.com/news/2011/07/110726-most-massive-water-cloud-quasar-black-hole-space-science/
https://www.wired.com/2011/07/black-hole-holds-universes-biggest-water-supply/
Engineer James O’Kane wears a prototype Apollo moonsuit, produced by International Latex Corporation, 1965.
Back in February 2013, the skies over Russia were lit by the fall and explosion of a large meteor. The scavenger hunt for meteorite pieces that followed turned up lots of conically-shaped chunks of rock, consistent with other meteors. Why do so many meteorites end up in this shape? There are a couple factors influencing it.
The first is that erosion during flight tends to shape initially spherical meteor chunks into broad cones. And that shape, it turns out, is remarkably stable in flight. By dropping cones of various geometries, researchers can test how stable they are in flight: do they change orientation, flutter back and forth, or drop straight down? Slender cones (below) tend to invert and tumble. Very broad cones flutter back and forth as they fall. But for an intermediate cone angle – similar to the one found in meteorites – the cones stay perfectly oriented, so once the rock erodes into that cone, it will keep that shape. (Image and video credit: K. Amin et al.)
50 years ago, three Apollo astronauts rode this 363 foot tall rocket, the Saturn V, embarking on one of the greatest missions of mankind – to step foot on another world. On July 20, 1969, astronauts Buzz Aldrin, Michael Collins and Neil Armstrong made history when they arrived at the Moon. Thanks to the Saturn V rocket, we were able to complete this epic feat, returning to the lunar surface a total of six times. The six missions that landed on the Moon returned a wealth of scientific data and almost 400 kilograms of lunar samples.
In honor of this historic launch, the National Air and Space Museum is projecting the identical rocket that took our astronauts to the Moon on the Washington Monument in Washington, D.C.
This week, you can watch us salute our Apollo 50th heroes and look forward to our next giant leap for future missions to the Moon and Mars. Tune in to a special two-hour live NASA Television broadcast at 1 p.m. ET on Friday, July 19. Watch the program at www.nasa.gov/live.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
Awesomely named NASA engineer Allyn “Hap” Hazard tries out a moonsuit of his own design, California, September 1960.
Everyone Missed An Apollo 11 Mistake, And It Almost Killed The Astronauts Returning To Earth
“Fortunately for everyone, they did get lucky. During the technical debriefing in the aftermath of Apollo 11, the fly-by of the Service Module past the Command Module was noted by Buzz Aldrin, who also reported on the Service Module’s rotation, which was far in excess of the design parameters. Engineer Gary Johnson hand-drew schematics for rewiring the Apollo Service Module’s jettison controller, and the changes were made just after the next flight: Apollo 12.
Those first four crewed trips to the Moon — Apollo 8, 10, 11 and 12 — could have all ended in potential disaster. If the Service Module had collided with the Command Module, a re-entry disaster similar to Space Shuttle Columbia could have occurred just as the USA was taking the conclusive steps of the Space Race.”
The flight plan for Apollo 11 was straightforward, if not quite simple. Follow the same trajectory to the Moon that Apollo 8 and Apollo 10 undertook, then successfully enter lunar orbit, launch the Lunar Module, descend to the surface and land softly, perform the scheduled EVA, then ascend back to the Command and Service Module, return to Earth, jettison the Service Module, re-enter, and deploy the parachute to successfully splash down in the Pacific Ocean. Only uncovered well after the mission, there was a huge flaw: the Service Module wasn’t programmed to jettison properly! If things had gone differently, the Command Module could have been damaged, and would have burned up in the atmosphere, killing all on board.
Come learn about the Apollo 11 mistake that Armstrong, Aldrin, and Collins were lucky to survive!
August 13, 1969 – New Yorkers cheer Apollo 11 astronauts Buzz Aldrin, Michael Collins, and Neil Armstrong in a parade down 42nd Street.
Asteroid belt
The asteroid belt is the circumstellar disc in the Solar System located roughly between the orbits of the planets Mars and Jupiter. It is occupied by numerous irregularly shaped bodies called asteroids or minor planets. The asteroid belt is also termed the main asteroid belt or main belt to distinguish it from other asteroid populations in the Solar System such as near-Earth asteroids and trojan asteroids. About half the mass of the belt is contained in the four largest asteroids: Ceres, Vesta, Pallas, and Hygiea. The total mass of the asteroid belt is approximately 4% that of the Moon, or 22% that of Pluto, and roughly twice that of Pluto’s moon Charon (whose diameter is 1200 km).
The asteroid belt formed from the primordial solar nebula as a group of planetesimals. Planetesimals are the smaller precursors of the protoplanets. Between Mars and Jupiter, however, gravitational perturbations from Jupiter imbued the protoplanets with too much orbital energy for them to accrete into a planet.
source | images: NASA, SOFIA/Lynette Cook, ESO/M. Kornmesser
POUR ONE OUT FOR COMRADE OPPORTUNITY
and send a thank you postcard to the Opportunity team for all their hard work!
“Okay boys, nice job so far; just one more. And this time, Neil, will you put your hand on Buzz’s shoulder? Need to communicate good crew cohesiveness.
Buzz and Neil look like they’re taking prom pics
Ellen Ochoa at Work on the Shuttle : During National Hispanic Heritage Month, we’re celebrating the achievements of astronaut Ellen Ochoa and other Hispanic astronauts and professionals at NASA. Floating upside down and reading a checklist may not be how most of us perform the day’s work, but it was for Ochoa on Space Shuttle Discovery’s STS-96 mission. (via NASA)
NASA Tech Launching on the Falcon Heavy
Later this month, a SpaceX Falcon Heavy rocket will take to the skies for the third time to launch the Department of Defense’s Space Test Program-2 (STP-2) mission. Several exciting, one-of-a-kind NASA technology and science payloads are among the two-dozen spacecraft aboard.
First, let’s talk about that Falcon Heavy rocket. Its 27 engines generate thrust at liftoff equal to that of approximately 18 airplanes, and it can lift over 140,000 pounds.
Managed by the U.S. Air Force Space and Missile Systems Center, STP-2 is the first government-contracted Falcon Heavy launch. It will reuse the two side boosters recovered after the April flight. SpaceX describes it as one of the most challenging launches in the company’s history.
It’s a big deal to us at NASA because we’re launching some pretty cool technologies. The tech will support our future exploration plans by helping improve future spacecraft design and performance. Here’s a bit about each:
Deep Space Atomic Clock
Time is the heartbeat of space navigation. Today, we navigate in deep space by using giant antennas on Earth to send signals to spacecraft, which then send those signals back to Earth. Atomic clocks on Earth measure the time it takes a signal to make this two-way journey. Only then can human navigators on Earth use large antennas to tell the spacecraft where it is and where to go.
Our Jet Propulsion Laboratory has been perfecting an atomic clock fit for exploration missions. The Deep Space Atomic Clock is the first atomic clock designed to fly on a spacecraft destined for beyond Earth’s orbit. The timepiece is lighter and smaller—no larger than a toaster oven—than its refrigerator-sized, Earthly counterparts.
This miniaturized clock could enable one-way navigation: a spacecraft receives a signal from Earth and can determine its location immediately using its own, built-in navigation system. Even smaller versions of the clock are being investigated right now that could be used for the growing number of small to mid-size satellites. As we go forward to the Moon with the Artemis program, precise measurements of time are key to mission success.
The Deep Space Atomic Clock is the primary payload onboard the General Atomics Electromagnetic Systems Orbital Test Bed satellite and will perform a year-long demonstration in space.
Enhanced Tandem Beacon Experiment (E-TBEx)
Two tiny satellites will study how signals can be muddled as they travel through hard-to-predict bubbles in the upper atmosphere. Signals sent from satellites down to Earth (and vice versa) can be disrupted by structured bubbles that sometimes form in Earth’s upper atmosphere. Because this region is affected both by weather on Earth and conditions in space, it’s hard to predict just when these bubbles will form or how they’ll mess with signals.
The E-TBEx CubeSats (short for Enhanced Tandem Beacon Experiment) will try to shed some light on that question. As these little satellites fly around Earth, they’ll send radio signals (like the ones used by GPS) to receiving stations on the ground. Scientists will be able to look at the signals received and see if they were jumbled as they traveled through the upper atmosphere down to Earth — which will help us track when these bubbles are forming and how much they’re interfering with our signals.
Green Propellant Infusion Mission (GPIM)
For decades, we have relied on a highly toxic spacecraft fuel called hydrazine. The Green Propellant Infusion Mission (GPIM) will lay the foundation to replace conventional chemical propulsion systems with a safer and more efficient alternative for next-generation spacecraft.
GPIM will demonstrate a new propellant in space for the first time. Concocted by the U.S. Air Force Research Laboratory, this innovative, “green” fuel—which actually has more of a peach hue—is expected to improve overall spacecraft performance due to its higher density, increased thrust and lower freezing point in comparison with hydrazine.
GPIM’s propulsion system, developed by Aerojet Rocketdyne, consists of new compatible tanks, valves and thrusters. During the two-month-long demonstration on a Ball Aerospace spacecraft, engineers will conduct orbital maneuvers to demonstrate the performance of the propellant and propulsion system.
Space Environment Testbeds (SET)
It’s not easy being a spacecraft; invisible, energetic particles zip throughout space — and while there are so few that space is considered a vacuum, what’s there still packs a punch. Tiny particles — like those seen here impacting a detector on a Sun-studying spacecraft — can wreak havoc with the electronics we send up into space.
Space Environment Testbeds — or SET, for short — is a mission to study space radiation and how it affects spacecraft and electronics in orbit. What looks like snow flurries in these animated images, for example, is actually a solar radiation storm of incredibly fast particles, unleashed by a solar eruption. Energetic particles from the Sun or deep space can spark memory damage or computer upsets on spacecraft, and over time, degrade hardware.
By studying radiation effects and different methods to protect satellites, SET will help future missions improve spacecraft design, engineering and operations.
Follow @NASA_Technology and @NASASun on Twitter for news about the STP-2 launch and our missions aboard.
Check out www.nasa.gov/spacex to stay up-to-date on the launch day and time. Don’t forget to tune into our launch coverage, scheduled to start about 30 minutes before liftoff!
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.