Latest Posts by 91001tv - Page 2
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Solar System: Things to Explore on Your Phone This Week
Let our apps lead you on a journey of exploration across the Earth, through the solar system and beyond. Here are some to download today:
1. Actually, it is rocket science Rocket Science 101 let’s you select your favorite mission and build a rocket to take you to destinations near and far. Learn how launch vehicles are configured and how their boosters and other component parts work together to successfully launch spacecraft.
iOS Google Play
2. Go to Mars (sort of) Be A Martian lets you experience Mars as if you were there! Join an international community of explorers. See the latest images of the Red Planet! Learn about Mars, ask questions, and check out behind-the-scenes videos of the missions.
iOS Google Play
3. All the Earth science With Earth Now, watch Earth science satellites in real time as they gather data about our home planet. Get real-time images of the places we call home. Check out global climate data, including surface air temperature, carbon dioxide, carbon monoxide, ozone, and sea level variations.
iOS Google Play
4. Pretty pictures Discover stunning images and videos of our planet Earth, space, stars and planets with Space Images. Find your favorite galaxies and explore our celestial neighborhood.
iOS Google Play
5. Ch-ch-ch-changes Images of Change give you a close-up view of our ever-changing planet. Inside this app, before and after image pairs show areas that have been subject to natural disasters or seen significant change over time.
iOS
Last but not least: NASA on the go With our official NASA app, explore and discover the latest images, videos, mission information, news, feature stories, tweets, NASA TV and featured content from across America’s space program.
iOS Google Play
Our apps let you explore our latest images, videos,and mission news.
Discover the full list of 10 apps showcasing our solar system this week HERE.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
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If you have a "smart" mobile phone, then you have a digital camera in your pocket, backpack or purse. The camera sensor built into these phones provide high resolution images that are captured in a digital format readily displayed, saved and shared with others. This same technology is now being built into flexible scopes for inspecting the internal channels of medical devices. This approach to flexible scope design offers a number of advantages over traditional fiber optics.
First, and foremost, is an incredible improvement of the image quality. With fiber optics, as the number of glass fibers are reduced, the resolution or quality of the image is also reduced. In very small bundles, below 5mm in diameter, the image can be blurry. Conversely, with the use of modern digital camera technology, the optical imaging sensor is actually placed right at the tip of the scope, delivering a clear, well defined image.
Another issue often experienced with fiber optics, is their delicate nature. A fiber optic scope has thousands of individual strands of glass. These strands are very delicate and when flexed and bent, they easily break. Not so with modern digital camera technology. The only thing running through the shaft of these flexible inspection scopes are wires that relay the bits and bytes from the image sensor at the tip - and deliver the power to that image sensor as well as the LED light also located at the tip.
Power and lighting bring up another important advancement made possible by digital imaging technology - unlike with traditional fiber optic systems that require a separate light source and some kind of individually powered camera coupling mechanism - the digital imaging technology found in flexible inspection scopes, including the lighting, camera and image capturing system, are all powered by the USB port of a desktop or laptop computer.
#AskSteveNow
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Viking 40th Anniversary - on Livestream.com
What’s On Board the Next SpaceX Cargo Launch?
Cargo and supplies are scheduled to launch to the International Space Station on Monday, July 18 at 12:45 a.m. EDT. The SpaceX Dragon cargo spacecraft will liftoff from our Kennedy Space Center in Florida.
Among the arriving cargo is the first of two international docking adapters, which will allow commercial spacecraft to dock to the station when transporting astronauts in the near future as part of our Commercial Crew Program.
This metallic ring, big enough for astronauts and cargo to fit through represents the first on-orbit element built to the docking measurements that are standardized for all the spacecraft builders across the world.
Its first users are expected to be the Boeing Starliner and SpaceX Crew Dragon spacecraft, which are both now in development.
What About the Science?!
Experiments launching to the station range from research into the effects of microgravity on the human body, to regulating temperature on spacecraft. Take a look at a few:
A Space-based DNA Sequencer
DNA testing aboard the space station typically requires collecting samples and sending them back to Earth to be analyzed. Our Biomolecule Sequencer Investigation will test a new device that will allow DNA sequencing in space for the first time! The samples in this first test will be DNA from a virus, a bacteria and a mouse.
How big is it? Picture your smartphone…then cut it in half. This miniature device has the potential to identify microbes, diagnose diseases and evaluate crew member health, and even help detect DNA-based life elsewhere in the solar system.
OsteoOmics
OsteoOmics is an experiment that will investigate the molecular mechanisms that dictate bone loss in microgravity. It does this by examining osteoblasts, which form bone; and osteoclasts, which dissolves bone. New ground-based studies are using magnetic levitation equipment to simulate gravity-related changes. This experiment hopes to validate whether this method accurately simulates the free-fall conditions of microgravity.
Results from this study could lead to better preventative care or therapeutic treatments for people suffering bone loss, both on Earth and in space!
Heart Cells Experiment
The goals of the Effects of Microgravity on Stem Cell-Derived Heart Cells (Heart Cells) investigation include increasing the understanding of the effects of microgravity on heart function, the improvement of heart disease modeling capabilities and the development of appropriate methods for cell therapy for people with heart disease on Earth.
Phase Change Material Heat Exchanger (PCM HX)
The goal of the Phase Change Material Heat Exchanger (PCM HX) project is to regulate internal spacecraft temperatures. Inside this device, we’re testing the freezing and thawing of material in an attempt to regulate temperature on a spacecraft. This phase-changing material (PCM) can be melted and solidified at certain high heat temperatures to store and release large amounts of energy.
Watch Launch!
Live coverage of the SpaceX launch will be available starting at 11:30 p.m. EDT on Sunday, July 17 via NASA Television.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Juno: Inside the Spacecraft
Our Juno spacecraft was carefully designed to meet the tough challenges in flying a mission to Jupiter: weak sunlight, extreme temperatures and deadly radiation. Lets take a closer look at Juno:
It Rotates!
Roughly the size of an NBA basketball court, Juno is a spinning spacecraft. Cartwheeling through space makes the spacecraft’s pointing extremely stable and easy to control. While in orbit at Jupiter, the spinning spacecraft sweeps the fields of view of its instruments through space once for each rotation. At three rotations per minute, the instruments’ fields of view sweep across Jupiter about 400 times in the two hours it takes to fly from pole to pole.
It Uses the Power of the Sun
Jupiter’s orbit is five times farther from the sun than Earth’s, so the giant planet receives 25 times less sunlight than Earth. Juno will be the first solar-powered spacecraft we’ve designed to operate at such a great distance from the sun. Because of this, the surface area of the solar panels required to generate adequate power is quite large.
Three solar panels extend outward from Juno’s hexagonal body, giving the overall spacecraft a span of about 66 feet. Juno benefits from advances in solar cell design with modern cells that are 50% more efficient and radiation tolerant than silicon cells available for space missions 20 years ago. Luckily, the mission’s power needs are modest, with science instruments requiring full power for only about six out of each 11-day orbit.
It Has a Protective Radiation Vault
Juno will avoid Jupiter’s highest radiation regions by approaching over the north, dropping to an altitude below the planet’s radiation belts, and then exiting over the south. To protect sensitive spacecraft electronics, Juno will carry the first radiation shielded electronics vault, a critical feature for enabling sustained exploration in such a heavy radiation environment.
Juno Science Payload:
Gravity Science and Magnetometers – Will study Jupiter’s deep structure by mapping the planet’s gravity field and magnetic field.
Microwave Radiometer – Will probe Jupiter’s deep atmosphere and measure how much water (and hence oxygen) is there.
JEDI, JADE and Waves – These instruments will work to sample electric fields, plasma waves and particles around Jupiter to determine how the magnetic field is connected to the atmosphere, and especially the auroras (northern and southern lights).
JADE and JEDI
Waves
UVS and JIRAM – Using ultraviolet and infrared cameras, these instruments will take images of the atmosphere and auroras, including chemical fingerprints of the gases present.
UVS
JIRAM
JunoCam – Take spectacular close-up, color images.
Follow our Juno mission on the web, Facebook, Twitter, YouTube and Tumblr.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
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Solar System: Things to Know This Week
Our solar system is huge, so let us break it down for you. Here are a few things you should know this week:
1. Science at the Edge
As the New Horizons spacecraft speeds away at more than 31,000 miles per hour (14 km/s) it continues to explore the Kuiper Belt, the region of icy bodies beyond Neptune. New Horizons has now twice observed 1994 JR1, a 90-mile-wide object orbiting more than 3 billion miles from the sun.
2. A Spaceship, Refined
This artist’s rendering shows our Europa mission spacecraft, which is being developed for a launch sometime in the 2020s. The mission will place a spacecraft in orbit around Jupiter to explore the giant planet’s moon Europa. This updated concept image shows tow large solar arrays extending from the sides of the spacecraft, to which the mission’s ice-penetrating radar antennas are attached. A saucer-shaped high-gain antenna is also side mounted with a magnetometer boom placed next to it. Find out more about the spacecraft HERE.
3. Sojourn at Saturn
The Cassini spacecraft is hard at work this week, orbiting Saturn to study the planet and its rings. The recent pictures are spectacular, take a look at them HERE.
4. Talking Juno
Our Juno mission arrives at Jupiter on July 4, and that presents a unique opportunity for educators, science communicators and anyone interested in space exploration. We are providing a growing set of Juno-related information resources. Take a look at them HERE.
5. Now THAT’S a Long Distance Call
How do explorers on Earth talk to astronauts and robotic spacecraft flung across the far reaches of space? They use the remarkable technology deployed by our Space Communications and Navigation (SCaN) Program Office. This month, SCaN is celebrating its 10th anniversary of managing the ultimate network. Find out how it works HERE.
Want to learn more? Read our full list of the 10 things to know this week about the solar system HERE.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
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Eight Things to Know About Our Flying Observatory
Our flying observatory, called SOFIA, is the world’s largest airborne observatory. It is a partnership with the German Aerospace Center (DLR). SOFIA studies the life cycle of stars, planets (including Pluto’s atmosphere), how interstellar dust can contribute to planet formation, analyzes the area around black holes, and identifies complex molecules in space.
1. A Telescope in an Airplane
SOFIA stands for the Stratospheric Observatory for Infrared Astronomy. It is a Boeing 747SP aircraft that carries a 100-inch telescope to observe the universe while flying between 38,000 and 45,000 feet – the layer of Earth’s atmosphere called the stratosphere.
2. The Short Aircraft Means Long Flights
SP stands for “special performance.” The plane is 47 feet shorter than a standard 747, so it’s lighter and can fly greater distances. Each observing flight lasts 10-12 hours.
3. It Flies with A Hole in the Side of the Plane…
The telescope is behind a door that opens when SOFIA reaches altitude so astronomers on board can study the universe. The kind of light SOFIA observes, infrared, is blocked by almost all materials, so engineers designed the side of the aircraft to direct air up-and-over the open cavity, ensuring a smooth flight.
4. …But the Cabin is Pressurized!
A wall, called a pressure bulkhead, was added between the telescope and the cabin so the team inside the aircraft stays comfortable and safe. Each flight has pilots, telescope operators, scientists, flight planners and mission crew aboard.
5. This Telescope Has to Fly
Water vapor in Earth’s atmosphere blocks infrared light from reaching the ground. Flying at more than 39,000 feet puts SOFIA above more than 99% of this vapor, allowing astronomers to study infrared light coming from space. The airborne observatory can carry heavier, more powerful instruments than space-based observatories because it is not limited by launch weight restrictions and solar power.
6. Studying the Invisible Universe
Humans cannot see what is beyond the rainbow of visible light. However, many interesting astronomical processes happen in the clouds of dust and gas that often surround the objects SOFIA studies, like newly forming stars. Infrared light can pass through these clouds, allowing astronomers to study what is happening inside these areas.
7. The German Telescope
The telescope was built our partner, the German Aerospace Center, DLR. It is made of a glass-ceramic material called Zerodur that does not change shape when exposed to extremely cold temperatures. The telescope has a honeycomb design, which reduces the weight by 80%, from 8,700 lb to 1,764 lb. (Note that the honeycomb design was only visible before the reflective aluminum coating was applied to the mirror’s surface).
8. ZigZag Flights with a Purpose
The telescope can move up and down, between 20-60 degrees above the horizon. But it can only move significantly left and right by turning the whole aircraft. Each new direction of the flight means astronomers are studying a new celestial object. SOFIA’s flight planners carefully map where the plane needs to fly to best observe each object planned for that night.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
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QuantumSummit by Steven Bledsoe Via Flickr: CalTechPasadena | #BLK2274
What’s Up for January?
A meteor shower, a binocular comet and the winter circle of stars. Here are the details:
Quadrantid Meteor Shower
The Quadrantid meteor shower on Jan. 4 will either sizzle or fizzle for observers in the U.S. The shower may favor the U.S. or it could favor Europe depending on which prediction turns out to be correct. For viewing in the United States, observers should start at 3 a.m. EST. The peak should last about two hours with rates of 120 meteors per hour predicted in areas with a dark sky.
Comet Catalina
In the middle of the month, midnight to predawn will be primetime for viewing Comet Catalina. It should be visible with binoculars if you have a dark sky, but a telescope would be ideal. Between the 14th and 17th the comet will pass by two stunning galaxies: M51, the whirlpool galaxy and M101, a fainter spiral galaxy.
Constellation Orion
Winter is also the best time to view the constellation Orion in the southeastern sky. Even in the city, you’ll see that it’s stars have different colors. Not telescope needed, just look up a few hours after sunset! The colorful stars of Orion are part of the winter circle of stars.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
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What’s Up for December?
View Mars right now, and prepare for 2016, the best Mars viewing year since 2005! Last month early risers watched small, reddish Mars dance with brighter Jupiter and Venus just before sunrise.
This month Mars rises earlier-by about 2 a.m. local time. Its reddish color is unmistakable, even without a telescope. It’s easy to see below the Moon and Jupiter on December 4. You won’t see many features this month, because the planet is almost 10 times smaller than nearby Jupiter appears and 350 times smaller than the Moon appears to us on Earth.
You should also be able to see Mars’ north polar region this month, because it’s currently tilted towards Earth.
You’ll be amazed at the changes you’ll see during 2016. January through December are all prime Mars observing months. Between January and May next year, Mars triples in apparent diameter as its orbit around the sun brings it closer to Earth. You’ll even be able to see the areas on Mars where NASA’s Mars landers are located.
By October, Mars shrinks in apparent size to less than half its May diameter as it speeds away from Earth. Mars shrinks even further from October through December, returning to the same size we saw in January 2016 by year’s end.
So put Mars viewing on your calendar for 2016. You won’t see Mars this size again until 2018, when Mars will put on an even better show.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Carbon and Our Changing Climate
Carbon is the backbone of life on Earth. We are made of carbon, we eat carbon and our civilizations are built on carbon. We need carbon, but that need is also entwined with one of the most serious problems facing us today: global climate change.
Forged in the heart of aging stars, carbon is the fourth most abundant element in the Universe. Most of Earth’s carbon – about 65,500 billion metric tons – is stored in rocks. The rest is in the ocean, atmosphere, plants, soil and fossil fuels.
Over the long term, the carbon cycle seems to maintain a balance that prevents all of Earth’s carbon from entering the atmosphere, or from being stored entirely in rocks. This balance helps keep Earth’s temperature relatively stable, like a thermostat.
Today, changes in the carbon cycle are happening because of people. We disrupt the cycle by burning fossil fuels and clearing land. Our Orbiting Carbon Observatory-2 (OCO-2) satellite is providing our first detailed, global measurements of CO2 in the atmosphere at the Earth’s surface. OCO-2 recently released its first full year of data, critical to analyzing the annual CO2 concentrations in the atmosphere.
The above animation shows carbon dioxide released from two different sources: fires and massive urban centers known as megacities. The animation covers a five day period in June 2006. The model is based on real emission data and is then set to run so that scientists can observe how greenhouse gas behaves once it has been emitted.
All of this extra carbon needs to go somewhere. So far, land plants and the ocean have taken up about 55 percent of the extra carbon people have put into the atmosphere while about 45 percent has stayed in the atmosphere. The below animation shows the average 12-month cycle of all plant life on Earth (on land and in the ocean). Eventually, the land and oceans will take up most of the extra carbon dioxide, but as much as 20 percent may remain in the atmosphere for many thousands of years.
Excess carbon in the atmosphere warms the planet and helps plants on land grow more. Excess carbon in the ocean makes the water more acidic, putting marine life in danger. Forest and other land ecosystems are also changing in response to a warmer world. Some ecosystems – such as thawing permafrost in the Arctic and fire-prone forests – could begin emitting more carbon than they currently absorb.
To learn more about NASA’s efforts to better understand the carbon and climate challenge, visit: http://www.nasa.gov/carbonclimate/.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com