Our Nancy Grace Roman Space Telescope recently passed a major review of the ground system, which will make data from the spacecraft available to scientists and the public.
Since the telescope has a gigantic field of view, it will be able to send us tons of data really quickly — about 500 times faster than our Hubble Space Telescope! That means Roman will send back a flood of new information about the cosmos.
Let’s put it into perspective — if we printed out all of Roman’s data as text, the paper would have to hurtle out of the printer at 40,000 miles per hour (64,000 kilometers per hour) to keep up! At that rate, the stack of papers would tower 330 miles (530 kilometers) high after a single day. By the end of Roman’s five-year primary mission, the stack would extend even farther than the Moon! With all this data, Roman will bring all kinds of cosmic treasures to light, from dark matter and dark energy to distant planets and more!
Learn more about the Roman Space Telescope.
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In case you don’t know, the Juno spacecraft entered orbit around the gas giant on July 4, 2016…about a year ago. Since then, it has been collecting data and images from this unique vantage point.
Juno is in a polar orbit around Jupiter, which means that the majority of each orbit is spent well away from the gas giant. But once every 53 days its trajectory approaches Jupiter from above its north pole, where it begins a close two-hour transit flying north to south with its eight science instruments collecting data and its JunoCam camera snapping pictures.
Space Fact: The download of six megabytes of data collected during the two-hour transit can take one-and-a-half days!
Juno and her cloud-piercing science instruments are helping us get a better understanding of the processes happening on Jupiter. These new results portray the planet as a complex, gigantic, turbulent world that we still need to study and unravel its mysteries.
Juno’s imager, JunoCam, has showed us that both of Jupiter’s poles are covered in tumultuous cyclones and anticyclone storms, densely clustered and rubbing together. Some of these storms as large as Earth!
These storms are still puzzling. We’re still not exactly sure how they formed or how they interact with each other. Future close flybys will help us better understand these mysterious cyclones.
Seen above, waves of clouds (at 37.8 degrees latitude) dominate this three-dimensional Jovian cloudscape. JunoCam obtained this enhanced-color picture on May 19, 2017, at 5:50 UTC from an altitude of 5,500 miles (8,900 kilometers). Details as small as 4 miles (6 kilometers) across can be identified in this image.
An even closer view of the same image shows small bright high clouds that are about 16 miles (25 kilometers) across and in some areas appear to form “squall lines” (a narrow band of high winds and storms associated with a cold front). On Jupiter, clouds this high are almost certainly comprised of water and/or ammonia ice.
Juno’s Microwave Radiometer is an instrument that samples the thermal microwave radiation from Jupiter’s atmosphere from the tops of the ammonia clouds to deep within its atmosphere.
Data from this instrument suggest that the ammonia is quite variable and continues to increase as far down as we can see with MWR, which is a few hundred kilometers. In the cut-out image below, orange signifies high ammonia abundance and blue signifies low ammonia abundance. Jupiter appears to have a band around its equator high in ammonia abundance, with a column shown in orange.
Why does this ammonia matter? Well, ammonia is a good tracer of other relatively rare gases and fluids in the atmosphere...like water. Understanding the relative abundances of these materials helps us have a better idea of how and when Jupiter formed in the early solar system.
This instrument has also given us more information about Jupiter’s iconic belts and zones. Data suggest that the belt near Jupiter’s equator penetrates all the way down, while the belts and zones at other latitudes seem to evolve to other structures.
Prior to Juno, it was known that Jupiter had the most intense magnetic field in the solar system…but measurements from Juno’s magnetometer investigation (MAG) indicate that the gas giant’s magnetic field is even stronger than models expected, and more irregular in shape.
At 7.766 Gauss, it is about 10 times stronger than the strongest magnetic field found on Earth! What is Gauss? Magnetic field strengths are measured in units called Gauss or Teslas. A magnetic field with a strength of 10,000 Gauss also has a strength of 1 Tesla.
Juno is giving us a unique view of the magnetic field close to Jupiter that we’ve never had before. For example, data from the spacecraft (displayed in the graphic above) suggests that the planet’s magnetic field is “lumpy”, meaning its stronger in some places and weaker in others. This uneven distribution suggests that the field might be generated by dynamo action (where the motion of electrically conducting fluid creates a self-sustaining magnetic field) closer to the surface, above the layer of metallic hydrogen. Juno's orbital track is illustrated with the black curve.
Juno also observed plasma wave signals from Jupiter’s ionosphere. This movie shows results from Juno's radio wave detector that were recorded while it passed close to Jupiter. Waves in the plasma (the charged gas) in the upper atmosphere of Jupiter have different frequencies that depend on the types of ions present, and their densities.
Mapping out these ions in the jovian system helps us understand how the upper atmosphere works including the aurora. Beyond the visual representation of the data, the data have been made into sounds where the frequencies and playback speed have been shifted to be audible to human ears.
The complexity and richness of Jupiter’s “southern lights” (also known as auroras) are on display in this animation of false-color maps from our Juno spacecraft. Auroras result when energetic electrons from the magnetosphere crash into the molecular hydrogen in the Jovian upper atmosphere. The data for this animation were obtained by Juno’s Ultraviolet Spectrograph.
During Juno’s next flyby on July 11, the spacecraft will fly directly over one of the most iconic features in the entire solar system – one that every school kid knows – Jupiter’s Great Red Spot! If anybody is going to get to the bottom of what is going on below those mammoth swirling crimson cloud tops, it’s Juno.
Learn more about the Juno spacecraft and its mission at Jupiter HERE.
On Jan. 25, we’re going for GOLD!
We’re launching an instrument called Global-scale Observations of the Limb and Disk, GOLD for short. It’s a new mission that will study a complicated — and not yet fully understood — region of near-Earth space, called the ionosphere.
Space is not completely empty: It’s teeming with fast-moving energized particles and electric and magnetic fields that guide their motion. At the boundary between Earth’s atmosphere and space, these particles and fields — the ionosphere — co-exist with the upper reaches of the neutral atmosphere.
That makes this a complicated place. Big events in the lower atmosphere, like hurricanes or tsunamis, can create waves that travel all the way up to that interface to space, changing the wind patterns and causing disruptions.
It’s also affected by space weather. The Sun is a dynamic star, and it releases spurts of energized particles and blasts of solar material carrying electric and magnetic fields that travel out through the solar system. Depending on their direction, these bursts have the potential to disrupt space near Earth.
This combination of factors makes it hard to predict changes in the ionosphere — and that can have a big impact. Communications signals, like radio waves and signals that make our GPS systems work, travel through this region, and sudden changes can distort them or even cut them off completely.
Low-Earth orbiting satellites — including the International Space Station — also fly through the ionosphere, so understanding how it fluctuates is important for protecting these satellites and astronauts.
GOLD is a spectrograph, an instrument that breaks light down into its component wavelengths, measuring their intensities. Breaking light up like this helps scientists see the behavior of individual chemical elements — for instance, separating the amount of oxygen versus nitrogen. GOLD sees in far ultraviolet light, a type of light that’s invisible to our eyes.
GOLD is a hosted payload. The instrument is hitching a ride aboard SES-14, a commercial communications satellite built by Airbus for SES Government Solutions, which owns and operates the satellite.
Also launching this year is the Ionospheric Connection Explorer, or ICON, which will also study the ionosphere and neutral upper atmosphere. But while GOLD will fly in geostationary orbit some 22,000 miles above the Western Hemisphere, ICON will fly just 350 miles above Earth, able to gather close up images of this region.
Together, these missions give us an unprecedented look at the ionosphere and upper atmosphere, helping us understand the very nature of how our planet interacts with space.
To learn more about this region of space and the GOLD mission, visit: nasa.gov/gold.
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On Aug. 30, 1983, Guion Bluford, better known as Guy, became the first African American to fly to space. An accomplished jet pilot and aerospace engineer, Bluford became part of NASA’s 1978 astronaut class that included the first African American, the first Asian American, and the first women astronauts.
He and the other crew members of mission STS-8 were aboard the orbiter Challenger as it lifted off from Kennedy Space Center in Florida; it was the first nighttime launch and landing of the Space Shuttle program. While aboard, he and the other crew members deployed the Indian National Satellite (INSAT-1B), operated a Canadian-built robot arm, conducted experiments with live cell samples, and participated in studies measuring the effects of spaceflight on humans.
Guy Bluford chased his childhood dream of becoming an aerospace engineer, and in doing so, changed history and encouraged other Black astronauts to follow in his footsteps.
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New science is headed to the International Space Station aboard the SpaceX Dragon.
Investigations on this flight include a test of robotic technology for refueling spacecraft, a project to map the world’s forests and two student studies inspired by Marvel’s “Guardians of the Galaxy” series.
Learn more about the science heading into low-Earth orbit:
The Global Ecosystem Dynamics Investigation (GEDI) is an instrument to measure and map Earth’s tropical and temperate forests in 3D.
The Jedi knights may help protect a galaxy far, far away, but our GEDI will help us study and understand forest changes right here on Earth.
What’s cooler than cool? Cryogenic propellants, or ice-cold spacecraft fuel! Our Robotic Refueling Mission 3 (RRM3) will demonstrate technologies for storing and transferring these special liquids. By establishing ways to replenish this fuel supply in space, RRM3 could help spacecraft live longer and journey farther.
The mission’s techniques could even be applied to potential lunar gas stations at the Moon, or refueling rockets departing from Mars.
The Molecular Muscle investigation examines the molecular causes of muscle abnormalities from spaceflight in C. elgans, a roundworm and model organism.
This study could give researchers a better understanding of why muscles deteriorate in microgravity so they can improve methods to help crew members maintain their strength in space.
Perfect Crystals is a study to learn more about an antioxidant protein called manganese superoxide dismutase that protects the body from the effects of radiation and some harmful chemicals.
The station’s microgravity environment allows researchers to grow more perfectly ordered crystals of the proteins. These crystals are brought back to Earth and studied in detail to learn more about how the manganese superoxide dismutase works. Understanding how this protein functions may aid researchers in developing techniques to reduce the threat of radiation exposure to astronauts as well as prevent and treat some kinds of cancers on Earth.
SlingShot is a new, cost-effective commercial satellite deployment system that will be tested for the first time.
SlingShot hardware, two small CubeSats, and a hosted payload will be carried to the station inside SpaceX’s Dragon capsule and installed on a Cygnus spacecraft already docked to the orbiting laboratory. Later, Cygnus will depart station and fly to a pre-determined altitude to release the satellites and interact with the hosted payload.
Spaceflight appears to accelerate aging in both humans and mice. Rodent Research-8 (RR-8) is a study to understand the physiology of aging and the role it plays on the progression of disease in humans. This investigation could provide a better understanding of how aging changes the body, which may lead to new therapies for related conditions experienced by astronauts in space and people on Earth.
The MARVEL ‘Guardians of the Galaxy’ Space Station Challenge is a joint project between the U.S. National Laboratory and Marvel Entertainment featuring two winning experiments from a contest for American teenage students. For the contest, students were asked to submit microgravity experiment concepts that related to the Rocket and Groot characters from Marvel’s “Guardians of the Galaxy” comic book series.
Team Rocket: Staying Healthy in Space
If an astronaut suffers a broken tooth or lost filling in space, they need a reliable and easy way to fix it. This experiment investigates how well a dental glue activated by ultraviolet light would work in microgravity. Researchers will evaluate the use of the glue by treating simulated broken teeth and testing them aboard the station.
Team Groot: Aeroponic Farming in Microgravity
This experiment explores an alternative method for watering plants in the absence of gravity using a misting device to deliver water to the plant roots and an air pump to blow excess water away. Results from this experiment may enable humans to grow fruits and vegetables in microgravity, and eliminate a major obstacle for long-term spaceflight.
These investigation join hundreds of others currently happening aboard the station. For more info, follow @ISS_Research!
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On April 7, Jupiter--the king of planets--reaches opposition, when it shines brightest and appears largest.
Jupiter will be almost directly overhead at midnight.
This is also a great time to observe the planet’s Galilean moons--Io, Ganymeade, Europa and Callisto. They can be easily seen through binoculars.
With binoculars, you can even see the Great Red Spot as the storm transits the planet every ten hours.
Looking east on April 22, look to the skies for the Summer Triangle, consisting of Deneb, in Cygnus, the Swan; Altair in Aquila, the Eagle; and Vega, in Lyre(the Harp).
Get ready for the Lyrids, the year’s second major meteor shower, as it pierces the Summer Triangle in the early morning hours of April 22. Since the shower begins close to the new moon, expect excellent almost moonless viewing conditions.
You can catch up on solar system and all of our missions at www.nasa.gov
Watch the full “What’s Up for April 2017″ video:
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Our view from space shows our planet is changing, but to really understand the details of these changes and what they mean for our future, scientists need a closer look. Over the next six months, we’re taking you on a world tour as we kick off major new field research campaigns to study regions of critical change from land, sea and air.
You can follow the Earth Expeditions on Facebook, Twitter and their Blog.
CORAL (Coral Reef Airborne Laboratory)
This three-year CORAL mission will use advanced airborne instruments and in-water measurements to survey a portion of the world’s coral reefs. The mission will assess the conditions of these threatened ecosystems to better understand their relation to the environment, including physical, chemical and human factors. With a new understanding of reef condition, the future of this global ecosystem can be predicted.
OMG (Oceans Melting Greenland)
Oceans Melting Greenland (OMG) mission will pave the way for improved estimates of sea level rise by addressing the question: To what extent are the oceans melting Greenland’s ice from below? This mission will observe changing water temperatures and glaciers that reach the ocean around all of Greenland from 2015 to 2020. This year, the OMG mission will fly over the periphery of Greenland to take measurements of the heights and extents of Greenland’s coastal glaciers that reach the ocean and release expendable sensors to measure the temperature and salinity of coastal waters. The OMG field campaign will gather data that will help scientists both understand how the oceans are joining with the atmosphere in melting the vast ice sheet and to predict the extent and timing of the resulting sea level rise.
NAAMES (North Atlantic Aerosols and Marine Ecosystems Study)
About half the carbon dioxide emitted into Earth’s atmosphere each year ends up in the ocean, and plankton absorb a lot of it. The NAAMES mission studies the world’s largest plankton bloom and how it gives rise to small organic particles that leave the ocean and end up in the atmosphere, ultimately influencing clouds and climate. This mission will be taking measurements from both ship and aircraft in the North Atlantic.
KORUS-AQ (Korea U.S.-Air Quality)
Air quality is a significant environmental concern around the world. Scientists are developing new ways to untangle the different factors that contribute to poor air quality. KORUS-AQ is a joint field study between NASA and the Republic of Korea to advance the ability to monitor air pollution from space. The campaign will assess air quality across urban, rural and coastal South Korea using observations from aircraft, ground sites, ships and satellites to test air quality models and remote sensing methods. Findings from this study will help develop observing systems using models and data to improve air quality assessments for decision makers.
ABoVE (Arctic Boreal Vulnerability Experiment)
The ABoVE mission covers 2.5 million square miles of tundra, forests, permafrost and lakes in Alaska and Northwestern Canada. Scientists from the mission are using satellites and aircraft to study this formidable terrain as it changes in a warming climate. Teams of researchers will also go out into the field to gather additional data. The mission will investigate questions about the role of climate in wildfires, thawing permafrost, wildlife migration habits, insect outbreaks and more.
ATom (Atmospheric Tomography)
The ATom mission takes flight through Earth’s atmosphere to understand how short-lived greenhouse gases like ozone and methane contribute to climate change. In late July through August 2016, a suite of instruments aboard our DC-8 flying laboratory will be hopping down the Pacific Ocean from Alaska to the southern tip of South America. It will then travel north up the Atlantic to Greenland to measure more than 200 gases and particles in the air and their interactions all around the world.
ORACLES (Observations of Clouds above Aerosols and their Interactions)
Southern Africa produces almost a third of the world’s vegetative burning, which sends smoke particles up into the atmosphere, where they eventually mix with stratocumulus clouds over the southeastern Atlantic Ocean. Little is known about how these particles impact the clouds, which play a key role in both regional and global surface temperatures and precipitation. The ORACLES mission is a five-year ground and air campaign aimed at better understanding their interactions and improve on current climate models.
ACT-America (Atmospheric Carbon and Transport – America)
The ACT-America mission will conduct five airborne campaigns across three regions in the eastern United States to study the transport of atmospheric carbon. This region serves as an ideal study area for its productive biosphere, agricultural activity, gas and oil extraction and consumption, dynamic seasonally varying weather patterns and the most extensive carbon cycle and meteorological observing networks on Earth. Using space borne, airborne and ground-based measurements, this mission will enable more accurate and precise estimates for climate management and prediction by studying sources and sinks of greenhouse gases, which act as a thermal blanket for Earth.
Remember to follow the Earth Expeditions on Facebook, Twitter and their Blog.
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Currently, six humans are living and working on the International Space Station, which orbits 250 miles above our planet at 17,500mph. Below you will find a real journal entry, written in space, by NASA astronaut Scott Tingle.
To read more entires from this series, visit our Space Blogs on Tumblr.
This is my last entry into the Captain’s Log. Drew Feustel, Ricky Arnold and Oleg Artymyev are now in charge after an excellent change of command ceremony where Drew took command of the International Space Station (ISS). We, the crew of the Soyuz MS-07 spacecraft, will undock from the International Space Station on Sunday morning (3 June), reenter the earth’s atmosphere and land on the steppe of Kazakhstan. I will be reunited with my family 24 hours later in Houston, and then begin recovery for living on Earth….with gravity….ugh.
I would like to thank all of you for following along on this incredible adventure, an adventure that started for me many years ago, and a journey that you have supported each step of the way.
To our Lead Flight Director, Gary Horlacher (Houston) and our Lead Payload Operations Director Patricia Patterson (Huntsville) – what an amazing job. Endless hours, minimal sleep, and herding a cast of thousands to establish the priorities that would define success for our Expedition. Thank you for your service, and for your outstanding leadership.
To our incredibly talented team supporting from Mission Control at all of our centers – Houston, Huntsville, Tsukuba, Cologne, and Moscow – you are incredible professionals without which our human spaceflight program could not exist. Thank you for your dedication, service and professionalism.
My life has been driven by dreams and goals. One of my concerns has always been that following my heart to achieve my dreams would have a deep impact on my family and friends. In the Navy, we endured multiple extended deployments onboard aircraft carriers, constant training cycles in locations away from home, and long days and weekends of training and work when we finally had some time at home.
In the space program, operational requirements demand the same attention and focus. I have moved my family 12 times in 30 years to make myself available for opportunities to serve that I would have otherwise not been afforded. I have always asked myself – is this worth it? I always assumed “yes”, but could not say definitively in the midst of the journey. My journey has brought my family to several new communities where we needed to learn, adjust, adapt and thrive. We are good at it. My family knows what it is like to live on the East Coast, the West Coast, the desert, the Midwest and the South. My family does not consider varying locations or diverse cultures as barriers to their success, but as opportunities to grow and excel. My children are embarking on their own dreams now, with an energy and focus even greater than I had at their age. My family maintains relationships with lifelong friends all over the country, and now the world. My family believes that dreams are attainable, and that the journey towards their dreams is where the value is found.
I am very lucky that I have lifelong friends that understand what it was that took me away from my childhood home. I am very lucky to have a family that “gets it”. My wife, Raynette, is amazing at being patient, and at making things work amidst unimaginable chaos. I am very proud of my military family for enduring all that they have over the years. Throughout the sacrifice and endurance, they decided to thrive – typical of our country’s incredible military families. My son, Sean Tingle, wrote and produced the song “To Touch the Stars” in honor of our journey that reached another level of success during ISS Expeditions 54 and 55. After hearing this song, I can definitively say, “Yes, it was worth it”.
To my family, friends and colleagues - THANK YOU for a LIFETIME OF INSPIRATION!
Now, it’s time to get busy again - chop chop hubba bubba!
Find more ‘Captain’s Log’ entries HERE.
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What’s your favorite geological feature to view from space? Alternatively, what’s the biggest “duh” moment you’ve had during your career where you had an incorrect, preconceived notion about something. Thanks!
Vice President Mike Pence visited our Kennedy Space Center in Florida today. While there, he delivered remarks to the workforce and toured our complex to see progress toward sending humans deeper into space, and eventually to Mars. He also had the opportunity to see our work with commercial companies to launch humans from U.S. soil to the International Space Station.
Do you spend a lot of time online? Would you like to see our next crew of astronauts lift off to the International Space Station?
We're looking for digital content creators of all backgrounds to join us at Kennedy Space Center in Florida for our Crew-6 mission to the space station, set to lift off no earlier than Sunday, Feb. 26. Applications close Friday, Jan. 27 at 3 p.m. EST (2000 UTC)—we'd love to see you there! Apply now.
Can't make this one? Click here to stay updated about future opportunities.
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