Studying Sediments In Space

Incoming! We’ve Got Science from Jupiter!

Our Juno spacecraft has just released some exciting new science from its first close flyby of Jupiter! 

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.

So what did this first science flyby tell us? Let’s break it down...

1. Tumultuous Cyclones

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.

2. Jupiter’s Atmosphere

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.

3. Stronger-Than-Expected Magnetic Field

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. 

4. Sounds of Jupiter

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.

5. Jovian “Southern Lights”

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.

Stay updated on all things Juno and Jupiter by following along on social media: Twitter | Facebook | YouTube | Tumblr

Learn more about the Juno spacecraft and its mission at Jupiter HERE.

Orion’s top images of 2020

The Orion program showed its resilience this year during an unprecedented time, racking up several success stories building and testing the spacecraft in preparation for upcoming Artemis missions to the Moon. From hot fire and structural testing, to crew and service module assembly activities, progress on Orion brought the agency closer to sending the first woman and next man to the Moon by 2024, and sustainable lunar exploration by 2028.

Ensuring crew safety, a hot fire test was conducted on the Northrop Grumman-built attitude control motor – which provides steering for Orion’s  launch abort system in the event of an emergency during ascent – at the company’s facility in Elkton, Maryland. The 30-second hot fire was the third and final test to qualify the motor for human missions, beginning with Artemis II.

During a three-month testing campaign at NASA’s Plum Brook Station in Sandusky, Ohio, the Orion spacecraft was subjected to the extreme temperatures and electromagnetic environment it will experience on Artemis I – Orion’s first uncrewed test flight to the Moon atop the agency’s  Space Launch System (SLS) rocket. Testing wrapped up early and the vehicle was readied for its journey back to NASA’s Kennedy Space Center aboard the agency’s one-of-a-kind Super Guppy.

Before NASA astronauts fly Orion on missions to the Moon and back, testing is necessary to verify the spacecraft’s ability to withstand the stresses of launch, climb to orbit, the harsh conditions of deep space transit, and return to Earth. Engineers from NASA and its prime contractor, Lockheed Martin, completed testing on Orion’s Structural Test Article (STA) for Artemis I. The STA is structurally identical to Orion’s main spacecraft elements: the crew module, service module and launch abort system.

The first element machined for the Artemis III Orion crew module – a cone panel with openings for windows, which will provide a spectacular view – was designed by Lockheed Martin, and manufactured by AMRO Fabricating Corp., of South El Monte, California. The completed panel made its way to NASA’s Michoud Assembly Facility near New Orleans, where engineers will weld it with other elements as part of Orion’s pressure vessel.

Orion’s European Service Module primary structure for the Artemis for the Artemis III mission arrived at the Airbus facility in Bremen, Germany, from its Thales Alenia Space manufacturing site in Turin, Italy. The service module will be equipped with components to power Orion and provide life support to astronauts – such as air, water, heat and cooling – during the mission that will land the first woman and next man on the Moon.

Three spacecraft adapter jettison fairing panels were fitted onto Orion’s service module inside the Neil Armstrong Operations and Checkout Building at Kennedy. Once secured, the panels encapsulate the service module to protect it from harsh environments such as heat, wind, and acoustics as the spacecraft is propelled out of Earth’s atmosphere atop the SLS rocket during NASA’s Artemis I mission.

Curious about NASA’s next mission to the Red Planet – the Mars 2020 Perseverance rover? Here’s your chance to ask an expert!

Targeted for launch to the Red Planet in July 2020, our Mars 2020 Perseverance rover will search for signs of ancient life. Mission engineer Lauren DuCharme and astrobiologist Sarah Stewart Johnson will be taking your questions in an Answer Time session on Friday, July 17 from noon to 1pm ET here on our Tumblr! Make sure to ask your question now by visiting http://nasa.tumblr.com/ask

Lauren DuCharme is a systems engineer at NASA’s Jet Propulsion Laboratory (JPL) in Southern California, where she’s working on the launch and cruise of the Perseverance rover. Lauren got her start at JPL as an intern. Professor Sarah Stewart Johnson is an astrobiologist at Georgetown University in Washington. Her research focuses on detecting biosignatures, or traces of life, in planetary environments.

Fun Facts:

The name Perseverance was chosen from among the 28,000 essays submitted during the "Name the Rover" contest. Seventh-grader Alex Mather wrote in his winning essay, "We are a species of explorers, and we will meet many setbacks on the way to Mars. However, we can persevere. We, not as a nation but as humans, will not give up."

Perseverance will land in Jezero Crater, a 28-mile-wide (45-kilometer-wide) crater that scientists believe was once filled with water.

Perseverance carries instruments and technology that will pave the way for future human missions to the Moon and Mars. It is also carrying 23 cameras and two microphones to the Red Planet — the most ever flown in the history of deep-space exploration.

Perseverance is the first leg of a round trip to Mars. It will be the first rover to bring a sample caching system to Mars that will package promising samples for return to Earth by a future mission.

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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.

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The Roasted Planet

Can you hear this exoplanet screaming? As the exoplanet known as HD 80606 b approaches its star from an extreme, elliptical orbit, it suffers star-grazing torture that causes howling, supersonic winds and shockwave storms across this world beyond our solar system. Its torturous journey boils its atmosphere to a hellish 2,000 degrees Fahrenheit every 111 days, roasting both its light and dark sides. HD 80606b will never escape this scorching nightmare. Download this free poster in English and Spanish and check out the full Galaxy of Horrors.

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We Just Identified More Than 200 New (Potential) Planets

The Kepler space telescope is our first mission capable of identifying Earth-size planets around other stars. On Monday, June 19, 2017, scientists from many countries gathered at our Ames Research Center to talk about the latest results from the spacecraft, which include the identification of more than 200 potential new worlds! Here’s what you need to know:

We found 219 new planet candidates.

All of these worlds were found in a patch of sky near the Cygnus constellation in our Milky Way galaxy. Between 2009 and 2013, Kepler searched more than 200,000 stars in the region for orbiting planets. The 219 new planet candidates are part of the more than 4,000 planet candidates and 2,300 confirmed planets Kepler has identified to date.

Ten of these worlds are like our own.

Out of the 219 new planet candidates, 10 are possibly rocky, terrestrial worlds and orbit their star in the habitable zone – the range of distances from a star where liquid water could pool on the surface of a rocky planet.

Small planets come in two sizes.

Kepler has opened up our eyes to the existence of many small worlds. It turns out a lot of these planets are either approximately 1.5 times the size of Earth or just smaller than Neptune. The cool names given to planets of these sizes? Super Earths and mini-Neptunes.

Some of the new planets could be habitable. 

Water is a key ingredient to life as we know it. Many of the new planet candidates are likely to have small rocky cores enveloped by a thick atmosphere of hydrogen and helium, and some are thought to be ocean worlds. That doesn’t necessarily mean the oceans of these planets are full of water, but we can dream, can’t we?

Other Earths are out there.

Kepler’s survey has made it possible for us to measure the number of Earth-size habitable zone planets in our galaxy. Determining how many planets like our own that exist is the big question we’ll explore next.

The hunt for new planets continues.

Kepler continues to search for planets in different regions of space. With the launch of our Transiting Exoplanet Survey Satellite (TESS) and the James Webb Space Telescope (JWST) in 2018, we’re going to search for planets nearest the sun and measure the composition of their atmospheres. In the mid-2020s, we have our sights on taking a picture of small planets like Earth with our Wide-Field Infrared Survey Telescope (WFIRST).

*All images of planets are artist illustrations.

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Five Record-Setting Gamma-ray Bursts!

For 10 years, our Fermi Gamma-ray Space Telescope has scanned the sky for gamma-ray bursts (GRBs), the universe’s most luminous explosions!

Most GRBs occur when some types of massive stars run out of fuel and collapse to create new black holes. Others happen when two neutron stars, superdense remnants of stellar explosions, merge. Both kinds of cataclysmic events create jets of particles that move near the speed of light.

A new catalog of the highest-energy blasts provides scientists with fresh insights into how they work. Below are five record-setting events from the catalog that have helped scientists learn more about GRBs:

1. Super-short burst in Boötes!

The short burst 081102B, which occurred in the constellation Boötes on Nov. 2, 2008, is the briefest LAT-detected GRB, lasting just one-tenth of a second!

2. Long-lived burst!

Long-lived burst 160623A, spotted on June 23, 2016, in the constellation Cygnus, kept shining for almost 10 hours at LAT energies — the longest burst in the catalog.

For both long and short bursts, the high-energy gamma-ray emission lasts longer than the low-energy emission and happens later.

3. Highest energy gamma-rays!

The highest-energy individual gamma ray detected by Fermi’s LAT reached 94 billion electron volts (GeV) and traveled 3.8 billion light-years from the constellation Leo. It was emitted by 130427A, which also holds the record for the most gamma rays — 17 — with energies above 10 GeV.

4. In a constellation far, far away!

The farthest known GRB occurred 12.2 billion light-years away in the constellation Carina. Called 080916C, researchers calculate the explosion contained the power of 9,000 supernovae.

5. Probing the physics of our cosmos!

The known distance to 090510 helped test Einstein’s theory that the fabric of space-time is smooth and continuous. Fermi detected both a high-energy and a low-energy gamma ray at nearly the same instant. Having traveled the same distance in the same amount of time, they showed that all light, no matter its energy, moves at the same speed through the vacuum of space.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.  

Hello there 👋

Welcome back to Mindful Mondays! 🧘

Mondays are, famously, most people’s seventh favorite day of the week. And Mondays where everything is darker, longer, and colder than normal? Thanks, but no thanks.

But don’t panic; we’ve got something to help. It might be small, but it can make a big difference. Just ten minutes of mindfulness can go a long way, and taking some time out to sit down, slow down, and breathe can help center your thoughts and balance your mood. Sometimes, the best things in life really are free.

This year, we have teamed up with the good folks at @nasa. They want you to tune in and space out to relaxing music and ultra-high-definition visuals of the cosmos—from the surface of Mars.  

Sounds good, right? Well, it gets better. Watch more Space Out episodes on NASA+, a new no-cost, ad-free streaming service.

Why not give it a try? Just a few minutes this Monday morning can make all the difference, and we are bringing mindfulness straight to you. 

🧘WATCH: Space Out with NASA: Martian Landscapes, 11/27 at 1pm EST🧘

YouTube

Space Out with NASA: Martian Landscapes

Explore the surface of Mars as you turn on, tune in, and space out to relaxing music and stunning ultra-high-definition visuals of our cosmi

We are going to the Moon!

At 1:47 a.m. EST on Nov. 16, 2022, our Orion spacecraft launched aboard the Space Launch System (SLS) rocket from historic Launch Complex 39B at NASA’s Kennedy Space Center in Florida on a path to the Moon, officially beginning the Artemis I mission.

This mission is the first integrated test of NASA’s deep space exploration systems: the Orion spacecraft, the SLS rocket, and Kennedy ground systems. This is the very first time this rocket and spacecraft have flown together, and it’s the first of many Artemis missions to the Moon. Artemis I is uncrewed, but it lays the groundwork for increasingly complex missions that will land humans on the lunar surface, including the first woman and the first person of color to do so.

With Artemis, we will build a long-term human presence on the Moon and prepare humanity for future exploration plans to Mars and beyond.

See more photos of Artemis I on our Flickr.

Make sure to follow us on Tumblr for your regular dose of space!

From Apollo to Commercial Crew: Get To Know Historic Launch Pad 39A

Originally built for the massive Saturn V rockets that sent astronauts on Apollo missions to the Moon, Launch Complex 39A also served as one of the two launch pads used by the space shuttle. Between Apollo, Skylab, Apollo-Soyuz and the space shuttle, this launch pad has been the starting point for many of the nation’s most challenging and inspiring missions.

In 2014, SpaceX signed a property agreement with NASA for use and operation of the launch complex for 20 years, and the company modified the facility to prepare for the processing and launch of its Falcon 9 and Falcon Heavy rockets.

The SpaceX Falcon 9 rocket carrying the company’s Crew Dragon on its Demo-2 flight test to the International Space Station with NASA astronauts Robert Behnken and Douglas Hurley will lift off from the same historic site where astronauts first launched to the moon. Launch Complex 39A at NASA’s Kennedy Space Center in Florida is also the site of dozens of space shuttle launches that helped build the orbital laboratory.

Launch Complexes 39A and B were constructed in the 1960s. Both launch pads have a long history of supporting launches for the Apollo and Space Shuttle Programs. Launch Pad 39A was the launch site for 11 Saturn V Apollo missions, including Apollo 11, the first Moon landing. The pad also was the launch site for 82 space shuttle missions, including STS-1, the first shuttle launch, the STS-125 final servicing mission for the Hubble Space Telescope, and STS-135, the final shuttle mission.

After the space shuttle was retired in 2011, we began the process to transform Kennedy Space Center from a historically government-only launch facility into a multi-user spaceport for both government and commercial use. On April 14, 2014, the agency signed a property agreement with SpaceX for use of the launch site for the next 20 years.

SpaceX upgraded and modified the launch pad to support its Falcon 9 and Falcon Heavy rockets. The company also built a horizontal processing hangar at the base of the pad to perform final vehicle integration prior to flight. The first SpaceX launch from the pad was the company’s 10th commercial resupply services (CRS-10) mission for us. A SpaceX Falcon 9 launched a Dragon cargo spacecraft on CRS-10 on Feb. 19, 2017. The Dragon delivered about 5,500 pounds of supplies to the space station, including the Stratospheric Aerosol and Gas Experiment (SAGE) III instrument to further study ozone in the Earth’s atmosphere. Combined with SpaceX, we’ve launched more than 100 missions from Pad 39A.

Because of our partnership with SpaceX within our agency’s Commercial Crew Program, Launch Complex 39A will once again be the site of crewed missions to the space station.

🚀 TUNE IN starting at 12:15 p.m. EDT on Wednesday, May 27 as NASA and SpaceX launch astronauts Robert Behnken and Douglas Hurley to the International Space Station aboard the Crew Dragon spacecraft: www.nasa.gov.live.

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