You followed fictional astronaut, Callie Rodriguez, on her journey to the Moon in our First Woman graphic novel, “Issue No. 1: From Dream to Reality.”
In the brand new “Issue No. 2: Expanding our Universe,” find out how Callie and her robotic sidekick RT escape the lunar lava tunnel and what challenges await them on the lunar surface.
See Callie and her new crewmates work together as a team and navigate the unexpected as they take on a challenging mission to deploy a next-generation telescope on the far side of the Moon. Now available digitally in English at nasa.gov/CallieFirst and in Spanish at nasa.gov/PrimeraMujer!
Along with the new chapter, the First Woman app – available in the Apple and Google Play stores – has been updated with new immersive, extended reality content. Explore the lunar surface and learn about the real technologies we’re building to make living and working on the Moon – and eventually, Mars – possible.
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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!
How much rain falls in a hurricane? How much snow falls in a nor’easter? What even is a nor’easter? These are the sorts of questions answered by our Global Precipitation Measurement Mission, or GPM.
GPM measures precipitation: Rain, snow, sleet, freezing rain, hail, ice pellets. It tells meteorologists the volume, intensity and location of the precipitation that falls in weather systems, helping them improve their forecasting, gather information about extreme weather and better understand Earth’s energy and water cycles.
And putting all that together, one of GPM’s specialties is measuring storms.
GPM is marking its fifth birthday this year, and to celebrate, we’re looking back on some severe storms that the mission measured in its first five years.
1. The Nor’easter of 2018
A nor’easter is a swirling storm with strong northeasterly winds and often lots of snow. In January 2018, the mission’s main satellite, the Core Observatory, flew over the East Coast in time to capture the development of a nor’easter. The storm dumped 18 inches of snow in parts of New England and unleashed winds up to 80 miles per hour!
2. Hurricane Harvey
Hurricane Harvey came to a virtual halt over eastern Texas in August 2017, producing the largest rain event in U.S. history. Harvey dropped up to 5 feet of rain, causing $125 billion in damage. The Core Observatory passed over the storm several times, using its radar and microwave instruments to capture the devastating deluge.
3. Typhoon Vongfong
In October 2014, GPM flew over one of its very first Category 5 typhoons – tropical storms with wind speeds faster than 157 miles per hour. The storm was Typhoon Vongfong, which caused $48 million in damage in Japan, the Philippines and Taiwan. We were able to see both the pattern and the intensity of Vongfong’s rain, which let meteorologists know the storm’s structure and how it might behave.
4. Near Real-Time Global Precipitation Calculations
The Core Observatory isn’t GPM’s only satellite! A dozen other satellites from different countries and government agencies come together to share their microwave measurements with the Core Observatory. Together, they are called the GPM Constellation, and they create one of its most impressive products, IMERG.
IMERG stands for “Integrated Multi-satellitE Retrievals for GPM,” and it uses the info from all the satellites in the Constellation to calculate global precipitation in near real time. In other words, we can see where it’s raining anywhere in the world, practically live.
5. Hurricane Ophelia
Hurricane Ophelia hit Ireland and the United Kingdom in October 2017, pounding them with winds up to 115 miles per hour, reddening the skies with dust from the Sahara Desert and causing more than $79 million in damages. Several satellites from the Constellation passed over Ophelia, watching this mid-latitude weather system develop into a Category 3 hurricane – the easternmost Category 3 storm in the satellite era (since 1970).
From the softest snow to the fiercest hurricanes, GPM is keeping a weather eye open for precipitation around the world. And we’re on cloud nine about that.
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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.
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
Summer in the northern hemisphere brings monsoon season, causing heavy rains and flooding that trigger landslides. Next time you see a landslide in the news, online, or in your neighborhood, submit it to our citizen science project Landslide Reporter to build the largest open global landslide catalog and help us and the public learn more about when and where they occur.
After a storm, the soil and rock on a slope can become saturated with water and begin to slide downwards, posing a danger to people and destroying roads, houses and access to electricity and water supplies.
Orbiting the Earth right now, the Global Precipitation Measurement (GPM) mission is a group of 10 satellites that measure rain, snow, sleet and other precipitation worldwide every three hours. This data tells us where and when heavy rain is falling and if it could lead to disasters.
We're using GPM data to understand where and when landslides are happening. A global landslide model uses information about the environment and rainfall to anticipate where landslides are likely to happen anytime around the world every three hours.
If you find a landslide reported online or in your neighborhood, you can provide the event details in Landslide Reporter, our citizen science project.
Your detailed reports are added into an open global landslide inventory available at Landslide Viewer. We use citizen science contributions along with other landslide data to check our prediction model so we can have a better picture of how rainfall, slope steepness, forest cover, and geology can trigger a landslide.
When you report a landslide, you improve our collection of landslide data for everyone.
Help support landslide efforts worldwide by contributing to Landslide Reporter, and you can help inform decisions that could save lives and property today! Learn more about the project at https://landslides.nasa.gov. You can also follow the project on Twitter and Facebook.
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For the first time ever, we've found a massive crater hiding under one of Earth's ice sheets. Likely caused by a meteor, it was uncovered in Greenland by a team of international scientists using radar data.
The data was collected by missions like our Operation IceBridge, which flies planes over Greenland and Antarctica to study the ice and snow at our planet’s poles.
In this case, the crater is near Hiawatha Glacier, covered by a sheet of ice more than half a mile thick. We're pretty sure that the crater was caused by a meteor because it has characteristics traditionally associated with those kinds of impacts, like a bowl shape and central peaks.
It’s also one of the 25 largest impact craters in the world, large enough to hold the cities of Paris or Washington, D.C. The meteor that created it was likely half a mile wide.
Currently, there’s still lots to learn about the crater – and the meteor that created it – but it’s likely relatively young in geologic timescales. The meteor hit Earth within the last 3 million years, but the impact could have been as recent as 13,000 years ago.
While it was likely smaller than the meteor credited with knocking out the dinosaurs, this impact could have potentially caused a large influx of fresh water into the northern Atlantic Ocean, which would have had profound impacts for life in the region at the time.
Go here to learn more about this discovery: https://www.nasa.gov/press-release/international-team-nasa-make-unexpected-discovery-under-greenland-ice
Operation IceBridge continues to uncover the hidden secrets under Earth's ice. IceBridge has been flying for 10 years, providing a data bridge between ICESat, which flew from 2003 to 2009, and ICESat-2, which launched in September. IceBridge uses a suite of instruments to help track the changing height and thickness of the ice and the snow cover above it. IceBridge also measures the bedrock below the ice, which allows for discoveries like this crater.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Hello there 👋
Welcome back to the third week of Mindful Mondays. It’s very good to see you 🧘
Here is another installment of mindfulness to get the first day of your week well underway, and underway well. Experience the phases of the Moon as you turn on, tune in, and space out to relaxing music and stunning ultra-high-definition visuals of our cosmic neighborhood… 🌌
Sounds good, right? Of course it does. Mysterious, even. You can watch even more Space Out episodes on NASA+, a new no-cost, ad-free streaming service.
Why not give it a try? There is nothing to lose, everything to gain. Because just a few minutes this Monday morning can make all the difference to your entire week, as @nasa helps to bring mindfulness from the stars and straight to you.
🧘WATCH: Space Out with NASA: Moon Phase 12/11 at 1pm EST🧘
This galactic ghoul, captured by our Hubble Space Telescope, is actually a titanic head-on collision between two galaxies. Each "eye" is the bright core of a galaxy, one of which slammed into another. The outline of the face is a ring of young blue stars. Other clumps of new stars form a nose and mouth.
Although galaxy collisions are common most of them are not head-on smashups like this Arp-Madore system. Get spooked & find out what lies inside this ghostly apparition, here.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Morning Jeanette. My 10 year son old recently told me his dream job that he would love to do is to become an Astronaut or be apart of a team that builds a spaceship. What is your best suggestion for me as his parent to help expose him to know what life is like for an astronaut and how much work did you put in your education to help you solidify your career that I can use as encouragement for him? Thanks again and you're AWESOME.
I spent 11 and a half years in school after high school, so I tell this to students because it takes a lot of investment in educating yourself. Then even beyond that, gaining experiences that are meaningful. After graduate school, working at Ford Motor Company and the CIA really taught me how to be a detailed scientist as well as working operationally in the field. I also did internships to help hone and sharpen skills as an engineer. I was happy with my career, and then I applied.
This natural-color image shows smoke from fires in the Amazon rainforest spreading across several states within Brazil, including Amazonas, Mato Grosso, and Rondônia. The image was collected by our VIIRS (Visible Infrared Imaging Radiometer Suite) instrument aboard the Suomi NPP satellite (a joint-partnership between NASA and the National Oceanic and Atmospheric Administration) on August 20, 2019. It’s not unusual to see fires in Brazil at this time of year, but activity in the country’s largest state, Amazonas, has been above average. Many people use fire to maintain farmland and pastures or to clear land for other purposes.
Credits: NASA Worldview, Earth Observing System Data and Information System (EOSDIS).
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It’s Friday, Sept. 15 and our Cassini mission has officially come to a spectacular end. The final signal from the spacecraft was received here on Earth at 7:55 a.m. EDT after a fateful plunge into Saturn’s atmosphere.
After losing contact with Earth, the spacecraft burned up like a meteor, becoming part of the planet itself.
Although bittersweet, Cassini’s triumphant end is the culmination of a nearly 20-year mission that overflowed with discoveries.
Mission Team and Data
Now that the spacecraft is gone, most of the team’s engineers are migrating to other planetary missions, where they will continue to contribute to the work we’re doing to explore our solar system and beyond.
Mission scientists will keep working for the coming years to ensure that we fully understand all of the data acquired during the mission’s Grand Finale. They will carefully calibrate and study all of this data so that it can be entered into the Planetary Data System. From there, it will be accessible to future scientists for years to come.
Even beyond that, the science data will continue to be worked on for decades, possibly more, depending on the research grants that are acquired.
Other team members, some who have spent most of their career working on the Cassini mission, will use this as an opportunity to retire.
Future Missions
In revealing that Enceladus has essentially all the ingredients needed for life, the mission energized a pivot to the exploration of “ocean worlds” that has been sweeping planetary science over the past couple of decades.
Jupiter’s moon Europa has been a prime target for future exploration, and many lessons during Cassini’s mission are being applied in planning our Europa Clipper mission, planned for launch in the 2020s.
The mission will orbit the giant planet, Jupiter, using gravitational assists from large moons to maneuver the spacecraft into repeated close encounters, much as Cassini has used the gravity of Titan to continually shape the spacecraft’s course.
In addition, many engineers and scientists from Cassini are serving on the new Europa Clipper mission and helping to shape its science investigations. For example, several members of the Cassini Ion and Neutral Mass Spectrometer team are developing an extremely sensitive, next-generation version of their instrument for flight on Europa Clipper. What Cassini has learned about flying through the plume of material spraying from Enceladus will be invaluable to Europa Clipper, should plume activity be confirmed on Europa.
In the decades following Cassini, scientists hope to return to the Saturn system to follow up on the mission's many discoveries. Mission concepts under consideration include robotic explorers to drift on the methane seas of Titan and fly through the Enceladus plume to collect and analyze samples for signs of biology.
Atmospheric probes to all four of the outer planets have long been a priority for the science community, and the most recent recommendations from a group of planetary scientists shows interest in sending such a mission to Saturn. By directly sampling Saturn's upper atmosphere during its last orbits and final plunge, Cassini is laying the groundwork for an potential Saturn atmospheric probe.
A variety of potential mission concepts are discussed in a recently completed study — including orbiters, flybys and probes that would dive into Uranus' atmosphere to study its composition. Future missions to the ice giants might explore those worlds using an approach similar to Cassini's mission.
Learn more about the Cassini mission and its Grand Finale HERE.
Follow the mission on Facebook and Twitter for the latest updates.
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