Our flying observatory SOFIA carries a telescope inside this Boeing 747SP aircraft. Scientists use SOFIA to study the universe — including stars, planets and black holes — while flying as high as 45,000 feet.
SOFIA is typically based at our Armstrong Flight Research Center in Palmdale, California, but recently arrived in Christchurch, New Zealand, to study celestial objects that are best observed from the Southern Hemisphere.
So what will we study from the land down under?
Eta Carinae, in the southern constellation Carina, is the most luminous stellar system within 10,000 light-years of Earth. It’s made of two massive stars that are shrouded in dust and gas from its previous eruptions and may one day explode as a supernova. We will analyze the dust and gas around it to learn how this violent system evolves.
We can study magnetic fields in the center of our Milky Way galaxy from New Zealand because there the galaxy is high in the sky — where we can observe it for long periods of time. We know that this area has strong magnetic fields that affect the material spiraling into the black hole here and forming new stars. But we want to learn about their shape and strength to understand how magnetic fields affect the processes in our galactic center.
Titan is Saturn’s largest moon and is the only moon in our solar system to have a thick atmosphere — it’s filled with a smog-like haze. It also has seasons, each lasting about seven Earth years. We want to learn if its atmosphere changes seasonally.
Titan will pass in front of a star in an eclipse-like event called an occultation. We’ll chase down the shadow it casts on Earth’s surface, and fly our airborne telescope directly in its center.
From there, we can determine the temperature, pressure and density of Titan’s atmosphere. Now that our Cassini Spacecraft has ended its mission, the only way we can continue to monitor its atmosphere is by studying these occultation events.
The Large Magellanic Cloud is a galaxy near our own, but it’s only visible from the Southern Hemisphere! Inside of it are areas filled with newly forming stars and the leftovers from a supernova explosion.
The Tarantula Nebula, also called 30 Doradus, is located in the Large Magellanic Cloud and shown here in this image from Chandra, Hubble and Spitzer. It holds a cluster of thousands of stars forming simultaneously. Once the stars are born, their light and winds push out the material leftover from their parent clouds — potentially leaving nothing behind to create more new stars. We want to know if the material is still expanding and forming new stars, or if the star-formation process has stopped. So our team on SOFIA will make a map showing the speed and direction of the gas in the nebula to determine what’s happening inside it.
Also in the Large Magellanic Cloud is Supernova 1987A, the closest supernova explosion witnessed in almost 400 years. We will continue studying this supernova to better understand the material expanding out from it, which may become the building blocks of future stars and planets. Many of our telescopes have studied Supernova 1987A, including the Hubble Space Telescope and the Chandra X-ray Observatory, but our instruments on SOFIA are the only tools we can use to study the debris around it with infrared light, which let us better understand characteristics of the dust that cannot be measured using other wavelengths of light.
For live updates about our New Zealand observations follow SOFIA on Facebook, Twitter and Instagram.
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The comprehensive test series called Green Run for our Space Launch System (SLS) rocket is underway at Stennis Space Center in Mississippi.
During Green Run, the rocket’s massive, 212-foot-tall core stage — the same flight hardware that will help launch Artemis I to the Moon – will operate together for the first time.
Here’s what you need to know about this top-to-bottom test series of our megarocket’s huge core:
Why is it called Green Run? “Green” refers to the new, untested hardware (AKA the core stage), and “run” represents the succession of tests the core stage paces through. One by one, this series will bring together several “firsts” for the rocket stage as the flight hardware undergoes eight different tests. Each test is designed to gradually bring our rocket’s core stage and all its systems to life for the first time.
So far, engineers have completed three of the series: the modal test, the avionics power-on, and the safety systems checkout. The safety systems are designed to end the test and shutdown systems automatically under undesirable conditions.
You can follow the progress of Green Run with this Green Run checklist infographic. Our team will be updating in real time as each Green Run test is completed.
The world’s tallest rocket stage is tested in an equally giant test stand. We upgraded the B-2 Test Stand used for the Saturn V rocket stages during the Apollo Program and, later, for the Space Shuttle Program. Now, the B-2 Test Stand is customized for testing our SLS core stage. When all four core stage engines fire up, they can generate some serious heat. So, the B-2 Test Stand will use roughly 100,000 gallons of water every 18 seconds to protect the stand and the hardware.
Speaking of engines firing up, the core stage will really show what it is capable of during the grand finale of Green Run. The goal is for the entire core stage to operate as one for up to 8.5 minutes — and that includes an impressive firing of all four RS-25 engines simultaneously. Just like at launch, more than 733,000 gallons of liquid propellant will flow from the two propellant tanks through the fuel lines to feed the RS-25 engines. When operating at sea level on the test stand, the cluster of four RS-25 engines will produce just over 1.6 million pounds of thrust – the same amount it will produce during the early phase of launch. During ascent, the core stage will produce a maximum thrust of over 2 million pounds.
All the Green Run tests, check outs and the 100 terabytes of collected data certify the core stage design and help verify the stage is ready for launch. To put the sheer amount of data collected during Green Run into perspective, just one terabyte is the equivalent of roughly 500 hours of movies. Even the Library of Congress’s collection only amounts to a total of 15 terabytes!
The next time our SLS rocket’s core stage fires up will be on the launch pad at Kennedy Space Center for the debut of the Artemis program. This inaugural SLS flight will be just the beginning of increasingly complex missions that will enable human exploration to the Moon and, ultimately, Mars.
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Jupiter’s vibrant bands of light belts and dark regions appear primed for their close-up during our Juno spacecraft’s 10th flyby on Feb. 7. This flyby was a gravity science positioned pass. During orbits that highlight gravity experiments, Juno is positioned toward Earth in a way that allows both transmitters to downlink data in real-time to one of the antennas of our Deep Space Network. All of Juno’s science instruments and the spacecraft’s JunoCam were in operation during the flyby, collecting data that is now being returned to Earth. The science behind this beautifully choreographed image will help us understand the origin and structure of the planet beneath those lush, swirling clouds.
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How long does each project take (approximately) . . . PS: you guys are so awesome >:D
Every day, our spacecraft and people are exploring the solar system. Both the public and the private sectors are contributing to the quest. For example, here are ten things happening just this week:
1. We deliver.
The commercial space company Orbital ATK is targeting Saturday, Nov. 11 for the launch of its Cygnus spacecraft on an Antares rocket from Wallops Flight Facility in Wallops Island, Virginia. Cygnus is launching on a resupply mission to the International Space Station, carrying cargo and scientific experiments to the six people currently living on the microgravity laboratory.
2. See for yourself.
Social media users are invited to register to attend another launch in person, this one of a SpaceX Falcon 9 rocket carrying the Dragon spacecraft from Cape Canaveral Air Force Station in Florida. This launch, currently targeted for no earlier than December, will be the next commercial cargo resupply mission to the International Space Station. The deadline to apply is Nov. 7. Apply HERE.
3. Who doesn't like to gaze at the Moon?
Our Lunar Reconnaissance Orbiter (LRO) sure does—and from very close range. This robotic spacecraft has been orbiting Earth's companion since 2009, returning views of the lunar surface that are so sharp they show the footpaths made by Apollo astronauts. Learn more about LRO and the entire history of lunar exploration at NASA's newly-updated, expanded Moon site: moon.nasa.gov
4. Meanwhile at Mars...
Another sharp-eyed robotic spacecraft has just delivered a fresh batch of equally detailed images. Our Mars Reconnaissance Orbiter (MRO) surveys the Red Planet's surface daily, and you can see the very latest pictures of those exotic landscapes HERE. We currently operate five—count 'em, five—active missions at Mars, with another (the InSight lander) launching next year. Track them all at: mars.nasa.gov.
5. Always curious.
One of those missions is the Curiosity rover. It's currently climbing a rocky highland dubbed Vera Rubin Ridge, turning its full array of instruments on the intriguing geology there. Using those instruments, Curiosity can see things you and I can't.
6. A new Dawn.
Our voyage to the asteroid belt has a new lease on life. The Dawn spacecraft recently received a mission extension to continue exploring the dwarf planet Ceres. This is exciting because minerals containing water are widespread on Ceres, suggesting it may have had a global ocean in the past. What became of that ocean? Could Ceres still have liquid today? Ongoing studies from Dawn could shed light on these questions.
7. There are eyes everywhere.
When our Mars Pathfinder touched down in 1997, it had five cameras: two on a mast that popped up from the lander, and three on the rover, Sojourner. Since then, photo sensors that were improved by the space program have shrunk in size, increased in quality and are now carried in every cellphone. That same evolution has returned to space. Our Mars 2020 mission will have more "eyes" than any rover before it: a grand total of 23, to create sweeping panoramas, reveal obstacles, study the atmosphere, and assist science instruments.
8. Voyage to a hidden ocean.
One of the most intriguing destinations in the solar system is Jupiter's moon Europa, which hides a global ocean of liquid water beneath its icy shell. Our Europa Clipper mission sets sail in the 2020s to take a closer look than we've ever had before. You can explore Europa, too: europa.nasa.gov
9. Flight of the mockingbird.
On Nov. 10, the main belt asteroid 19482 Harperlee, named for the legendary author of To Kill a Mockingbird, makes its closest approach to Earth during the asteroid's orbit around the Sun. Details HERE. Learn more about asteroids HERE. Meanwhile, our OSIRIS-REx mission is now cruising toward another tiny, rocky world called Bennu.
10. What else is up this month?
For sky watchers, there will be a pre-dawn pairing of Jupiter and Venus, the Moon will shine near some star clusters, and there will be meteor activity all month long. Catch our monthly video blog for stargazers HERE.
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Today in the NASA Village… Can you Grow Cheese in Space?
Did you know there are several programs where students can apply to have their experiments flown on the International Space Station? The FISE (Foundation for International Space Education) encourages students of all ages to design and propose real experiments to fly in low Earth orbit. Thomas and Nick Hall are two brothers that participated in this program.
When asked what his greatest hurdle was with growing cheese in space, student researcher Thomas replied, “One of the biggest hurdles I face is just simply staying focused. Being a Student Experimenter is very difficult especially in between the ages of 14 and 18, mainly because those are most kids High School years and during these years many kids are either drowned with homework, hanging out with friends, or out partying.”
It is so important we get young students interested early in perusing topics that are out of this world. The experiments chosen are carried out by the astronauts on-board the space station. In the case of cheese balls, Karen Nyberg carried out the experiment and reported back the findings (apparently she was unable to grow the cheese).
When Nick Hall was asked about his experiment to grow toothpaste, he said the most inspiring part was, “Thomas Hall III. My brother was the most inspiring because he was also doing the experiment so he was helping me do the experiment.”
The story of the Hall brothers is a great reminder that experimentation is just that, trials and test of ideas, but ultimately reminds us of the importance of the relationships we have developed on the ground.
Do you have an idea for a research project in space? Do you have a student researcher in mind? Find out how to apply at Student Spaceflight Experiments Program (SSEP) and learn more about space station education opportunities at STEM on Station.
Next time on the NASA Village… The Latest Fashion Sucks.
Do you want more stories? Find our NASA Villagers here!
The Geostationary Operational Environmental Satellite-R Series (GOES-R) is the nation’s next generation of geostationary weather satellites. It is the first of four satellites to be launched for the National Oceanic and Atmospheric Administration (NOAA).
The GOES-R satellite will provide advanced imaging with increased spatial resolution and faster coverage for more accurate forecasts, real-time mapping of lightning activity and improved monitoring of solar activity. For the first time, GOES-R will be able to monitor the Earth in near real-time.
Once in geostationary orbit (the orbit around the Earth’s equator), it will provide images of weather patterns and severe storms across the continental U.S. as regularly as every five minutes. Images of smaller, more detailed areas, where storm activity is present, will be taken as frequently as every 30 seconds.
These images can be used to aid in formulating regular forecasts, term forecasting, such as seasonal predictions and drought outlooks.
In addition, the satellite will constantly monitor space weather conditions, such as solar flares, to provide advance notice of potential communication and navigation disruptions.
The satellite will also assist researchers in understanding the interactions between land, oceans, the atmosphere and climate.
Improve hurricane tracking and intensity forecasts
Increase thunderstorm and tornado warning lead time
Give earlier warning of ground lightning strike hazards
Improve detection of heavy rainfall and flash flooding risks
Improve air quality warnings and alerts
Give better fire detection and intensity estimation
Improve solar flare warnings for communications and navigation disruptions
Give more accurate monitoring of energetic particles responsible for radiation hazards to humans and spacecraft
Improve monitoring of space weather to get better geomagnetic storm forecasting.
The better we can predict what’s coming, the better we can prepare.
The GOES-R satellite is targeted for a launch on Saturday, Nov. 19, aboard a United Launch Alliance Atlas V rocket.
The one-hour launch window opens at 5:42 p.m. EST. Liftoff will occur from our Kennedy Space Center in Florida.
Join us leading up to launch by tuning in during the following times:
Thursday, Nov. 17 Prelaunch News Conference - 1 p.m. EST Watch HERE
GOES-R Mission Briefing - 2 p.m. EST Watch HERE
Friday, Nov. 18 GOES-R Social Presentations – 1:30 p.m. EST Watch HERE
Saturday, Nov. 19 NASA Edge Prelaunch Program – 3:45 p.m. EST Watch HERE
Launch Coverage & Commentary – 4:45 p.m. EST Watch HERE
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Asteroids are the storytellers of our solar system’s youth. They are the closest we can get to the original material that makes up the sun, planets, and moons.
This week, our OSIRIS-REx spacecraft made history when it touched a pristine, ancient asteroid named Bennu to collect a sample from the surface. The intrepid spacecraft will now bring the asteroid sample – and its stories – back home to Earth.
Why is it that asteroid Bennu holds the history of our origins? Let’s go back to the beginning...
About 4.5 billion years ago, our solar system began as a spinning, swirling cloud made up of tiny bits of gaseous and rocky material. Most of that material – more than 99% of it – gathered in the center and went on to become the Sun.
The leftovers began to spin around the Sun, colliding into one another and forming larger and larger objects, eventually becoming planets, dwarf planets, and moons.
But asteroids didn't become part of planets or moons. So, while the material in planets and moons were superheated and altered during the formation of the solar system and weathered by geologic processes over time, asteroids remained pristine.
Each asteroid holds knowledge from that special time in our solar system’s history. Each one contains information about the chemicals, minerals, and molecules that were present when the solar system was just starting to form.
With missions like OSIRIS-REx, we are going on a journey to these ancient worlds, seeking to learn what they remember, seeking to expand our knowledge, and deepen our understanding of our origins.
Learn more about the OSIRIS-REx mission HERE, or follow the mission on Facebook, Twitter and Instagram.
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The moment has arrived- it's time to decide the NASA Earth Observatory's all-time best image. After four grueling rounds of voting, two contenders remain: Ocean Sand, Bahamas (#5 seed) versus Raikoke Erupts (#6 seed).
The road to the finals has been full of surprises. All top seeds have been knocked out. In one semifinal, Ocean Sand garnered 50.6 percent of the votes to squeak out a win over the overall favorite, Twin Blue Marbles. In the other matchup, Raikoke Erupts trounced Where the Dunes End, 66.5 to 33.5 percent.
Now you have to pick a champion. Will it be a gorgeous, artistic image from the very early years of Earth Observatory or stunning natural-color views of an explosive event from 2019? Which image will you crown as the best in the EO archives: Ocean Sand, Bahamas or Raikoke Erupts? Voting ends on April 28 at 9 a.m. U.S. Eastern Time.
Thank you for helping us celebrate Earth Observatory’s 20th anniversary and the 50th anniversary of Earth Day!
Vote here: https://earthobservatory.nasa.gov/tournament-earth
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What in the world is a polar vortex? On Earth, it’s a large area of low pressure and extremely cold air that usually swirls over the Arctic, with strong counter-clockwise winds that trap the cold around the Pole. But disturbances in the jet stream and the intrusion of warmer mid-latitude air masses can disturb this polar vortex and make it unstable, sending Arctic air south into middle latitudes.
That has been the case in late January 2019 as frigid weather moves across the Midwest and Northern Plains of the United States, as well as interior Canada. Forecasters are predicting that air temperatures in parts of the continental United States will drop to their lowest levels since at least 1994, with the potential to break all-time record lows for January 30 and 31. With clear skies, steady winds, and snow cover on the ground, as many as 90 million Americans could experience temperatures at or below 0 degrees Fahrenheit (-18° Celsius), according to the National Weather Service (NWS).
The Goddard Earth Observing System Model above shows this air temperature movement at 2 meters (around 6.5 feet above the ground) from January 23-29. You can see some portions of the Arctic are close to the freezing point—significantly warmer than usual for the dark of mid-winter—while masses of cooler air plunge toward the interior of North America.
Science Behind the Polar Vortex / Credit: NOAA
Meteorologists predicted that steady northwest winds (10 to 20 miles per hour) were likely to add to the misery, causing dangerous wind chills below -40°F (-40°C) in portions of 12 states. A wind chill of -20°F can cause frostbite in as little as 30 minutes, according to the weather service.
Not sure how cold that is? Check out the low temperatures on January 30, 2019 in some of the coldest places on Earth—and a planetary neighbor:
-46°F (-43°C) -- Chesterfield, Newfoundland
-36°F (-33°C) -- Yukon Territory, Canada
-33°F (-27°C) -- Fargo, North Dakota (Within the Polar Vortex)
-28°F (-18°C) -- Minneapolis, Minnesota (Within the Polar Vortex)
-27°F (-33°C) -- Amundsen-Scott South Pole Station, Antarctica
-24°F (-31°C) -- Chicago, Illinois (Within the Polar Vortex)
-15°F (5°C) -- Barrow, Alaska
-99°F (-73°C) -- Mars
Learn more about the science behind the polar vortex and how NASA is modeling it here: https://go.nasa.gov/2Wtmb43.
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Holiday lights don’t come in one shape or size, just like they don’t only appear on Earth. Take a look at a few of these celestial light shows:
1. Galactic Wreath of Lights
This festive image captured by our Hubble Space Telescope resembles a holiday wreath made of sparkling lights. This galactic wreath is located around 6,500 light-years away.
2. Red and Green Aurora
This beautiful aurora was captured by Astronaut Scott Kelly while aboard the International Space Station. He shared it with his Twitter followers on June, 22 during his Year in Space mission. This image of Earth’s aurora is festive with its red and green lights.
3. Holiday Snow Angel
Our Hubble Space Telescope captured this stunning image of what looks like a soaring, celestial snow angel. This picture shows a bipolar star-forming region, called Sharpless 2-106.
4. Cosmic Holiday Ornament
This festive-looking nearby planetary nebula resembles a glass-blown holiday ornament with a glowing ribbon entwined. This cosmic decoration was spotted by our Hubble Space Telescope.
5. Holiday Lights on the Sun
Even the sun gets festive with it’s festive looking solar flares. This significant flare was seen by our Solar Dynamics Observatory (SOHO) on Dec. 19, 2014. Even though solar flares are powerful bursts of radiation, it cannot pas through Earth’s atmosphere to physically affect humans on the ground. That said, when intense enough, the radiation can disturb the atmosphere in the layer where GPS and communications signals travel.
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