Mission Possible: Redirecting An Asteroid

And that’s a wrap! Thank you for all the great questions. We hope you learned a little bit about what it takes to work in mission control as a flight director.

If you’re hungry for more, you can read the latest installment of our First Woman graphic novel series, where fictional character Commander Callie Rodriguez embarks on the next phase of her trailblazing journey and leaves the Moon to take the helm at Mission Control.

Keep up with the flight directors, the Space Station, and the Artemis missions at the links below.

Flight directors: X

Artemis: Facebook: Facebook, Instagram, X

Space Station: Facebook, Instagram, X (@Space_Station), X( @ISS_Research)

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

The ranks of America’s Astronaut Corps grew by 11 today!

After completing more than two years of basic training, our graduating class of astronauts is eligible for spaceflight. Assignments include the International Space Station, Artemis missions to the Moon, and ultimately, missions to Mars.

The class includes 11 astronauts, selected in 2017 from a record-setting pool of more than 18,000 applicants. This was more than double the previous record of 8,000 applicants set in 1978.

Meet the graduates:

Kayla Barron

“If you don’t love what you’re doing, you’re not going to be good at it. I think it’s a combination of finding things that you really love that will also be really challenging and will force you to grow along the way.”

This Washington native graduated from the U.S. Naval Academy with a bachelor’s degree in systems engineering. As a Gates Cambridge Scholar, which offers students an opportunity to pursue graduate study in the field of their choice at the University of Cambridge. Barron earned a master’s degree in nuclear engineering.

As a Submarine Warfare Officer, Barron was part of the first class of women commissioned into the submarine community, completing three strategic deterrent patrols aboard the USS Maine.

Zena Cardman

“Every STEM opportunity that I have ever gone down is because of some mentor who inspired me or some student who was ahead of me in school who inspired me.”

Zena Cardman is a native of Virginia and completed a bachelor’s degree in biology and master’s degree in marine sciences at The University of North Carolina, Chapel Hill. Her research has focused on microorganisms in subsurface environments, ranging from caves to deep sea sediments.

An intrepid explorer, Cardman’s field experience includes multiple Antarctic expeditions, work aboard research vessels as both scientist and crew, and NASA analog missions in British Columbia, Idaho, and Hawaii.

Raja Chari

“I grew up with the mentality that education is truly a gift not to be taken for granted.”

This Iowa native graduated from the U.S. Air Force Academy in 1999 with bachelor’s degrees in astronautical engineering and engineering science. He continued on to earn a master’s degree in aeronautics and astronautics from Massachusetts Institute of Technology (MIT) and graduated from the U.S. Naval Test Pilot School.

Chari served as the Commander of the 461st Flight Test Squadron and the Director of the F-35 Integrated Test Force. He has accumulated more than 2,000 hours of flight time in the F-35, F-15, F-16 and F-18 including F-15E combat missions in Operation Iraqi Freedom.

Matthew Dominick

“I get to work with incredible people that want to solve problems and are passionate about it. I really want to contribute to the world and this is how I want to do it.”

This Colorado native earned a bachelor’s degree in electrical engineering from the University of San Diego and a master’s degree in systems engineering from the Naval Postgraduate School. He also graduated from U.S. Naval Test Pilot School.

Dominick served on the USS Ronald Reagan as department head for Strike Fighter Squadron 115. He has more than 1,600 hours of flight time in 28 aircraft, 400 carrier-arrested landings and 61 combat missions.

Bob Hines

“As you get older, other things become important to you, like being a part of something that’s bigger than yourself. This human endeavor of exploration is something that’s really exciting.”

Bob Hines is a Pennsylvania native and earned a bachelor’s degree in aerospace engineering from Boston University. He is a graduate of the U.S. Air Force Test Pilot School, where he earned a master’s degree in flight test engineering. He continued on to earn a master’s degree in aerospace engineering from the University of Alabama.

Hines served in the U.S. Air Force and Air Force Reserves for 18 years. He also served as a research pilot at our Johnson Space Center. He has accumulated more than 3,500 hours of flight time in 41 different types of aircraft and has flown 76 combat missions in support of contingency operations around the world.

Warren Hoburg

“It was back in high school that I realized that I was really interested in engineering. I always liked taking things apart and understanding how things work and then I also really enjoy solving problems.”

Nicknamed “Woody”, this Pennsylvania native earned a bachelor’s degree in aeronautics and astronautics from MIT and a doctorate in electrical engineering and computer science from the University of California, Berkeley.

Hoburg was leading a research group at MIT at the time of his selection and is a two-time recipient of the AIAA Aeronautics and Astronautics Teaching Award in recognition of outstanding teaching.

Dr. Jonny Kim

“I fundamentally believed in the NASA mission of advancing our space frontier, all while developing innovation and new technologies that would benefit all of humankind.”

This California native trained and operated as a Navy SEAL, completing more than 100 combat operations and earning a Silver Star and Bronze Star with Combat “V”. Afterward, he went on to complete a degree in mathematics at the University of San Diego and a doctorate of medicine at Harvard Medical School.

Kim was a resident physician in emergency medicine with Partners Healthcare at Massachusetts General Hospital.

Jasmin Moghbeli

“Surround yourself with good people that have the characteristics that you want to grow in yourself. I think if you surround yourself with people like that you kind of bring each other up to a higher and higher level as you go.”

Jasmin Moghbeli, a U.S. Marine Corps major, considers Baldwin, New York, her hometown. She earned a bachelor's degree in aerospace engineering with information technology at MIT, followed by a master’s degree in aerospace engineering from the Naval Postgraduate School.

She is a distinguished graduate of the U.S. Naval Test Pilot School and has accumulated more than 1,600 hours of flight time and 150 combat missions.

Loral O’Hara

“I’m one of those people who have wanted to be an astronaut since I was a little kid, and I think that came from an early obsession with flying – birds, airplanes, rockets.”

This Houston native earned a bachelor’s degree in aerospace engineering at the University of Kansas and a Master of Science degree in aeronautics and astronautics from Purdue University. As a student, she participated in multiple NASA internship programs, including the Reduced Gravity Student Flight Opportunities Program, the NASA Academy at Goddard Space Flight Center, and the internship program at the Jet Propulsion Laboratory.

O’Hara was a research engineer at Woods Hole Oceanographic Institution, where she worked on the engineering, test and operations of deep-ocean research submersibles and robots. She is also a private pilot and certified EMT and wilderness first responder.

Dr. Frank Rubio

“I just figured it was time to take the plunge and try it. And so, I did and beyond all dreams, it came true.” 

Dr. Francisco “Frank” Rubio, a U.S. Army lieutenant colonel, is originally from Miami. He earned a bachelor’s degree in international relations from the U.S. Military Academy and earned a doctorate of medicine from the Uniformed Services University of the Health Sciences. 

Rubio served as a UH-60 Blackhawk helicopter pilot and flew more than 1,100 hours, including more than 600 hours of combat and imminent danger time during deployments to Bosnia, Afghanistan, and Iraq. He is also a board certified family physician and flight surgeon.

Jessica Watkins

“I’ve always been interested in exploring space. What’s out there and how can we as humans reach those outer stars and how can we learn more information about who we are through that process.”

This Colorado native earned a bachelor’s degree in geological and environmental sciences at Stanford University, and a doctorate in geology from the University of California, Los Angeles. Watkins has worked at Ames Research Center and the Jet Propulsion Laboratory.

Watkins was a postdoctoral fellow at the California Institute of Technology, where she collaborated on the Mars Curiosity rover, participating in daily planning of rover activities and investigating the geologic history of the Red Planet.

Learn more about the new space heroes right here: https://www.nasa.gov/newastronauts

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Why We Study the Sun-Earth Connection – Explained Through Songs

We're launching a new mission to the International Space Station to continue measurements of the Sun's energy reaching Earth.

The Total and Spectral solar Irradiance Sensor (TSIS-1) will precisely measure the total amount of sunlight that falls on Earth and how that light is distributed among different wavelengths, including the ultraviolet, visible and infrared. This will give us a better understanding of Earth’s primary energy supply and help improve models simulating Earth’s climate.

1. You are my sunshine, my only sunshine. You make me happy when skies are gray.

The Sun is Earth's sunshine and it does more than make us happy; it gives us life. Our Sun's energy drives our planet's ocean currents, seasons, weather and climate. Changes in the Sun also alter our climate in at least two ways.

First, solar radiation has a direct effect where it heats regions of Earth, like our oceans, land, and atmosphere. Second, the solar radiation can cause indirect effects, such as when sunlight interacts with molecules in the upper atmosphere to produce ozone which can affect human health.  

Earth’s energy system is in a constant dance to maintain a balance between incoming energy from the Sun and outgoing energy from Earth to space, which scientists call Earth’s energy budget. If you have more energy absorbed by the Earth than leaving it, its temperature increases and vice versa. Because the Sun is Earth's fundamental energy source and only sunshine, we need a quantitative record of the Sun's solar energy output. TSIS-1 will provide the most accurate measurements ever made of sunlight as seen from above Earth’s atmosphere.

2. You're hot then you're cold…You're in then you're out. You're up then you're down.

The energy flow between the Earth and Sun's connection is not a constant thing. The Sun can be fickle, sometimes it puts out slightly more energy and some years less. Earth is no better. The Earth absorbs different amounts of the Sun's energy depending on many factors, such as the presence of clouds and tiny particles in the atmosphere called aerosols.  

What we do know is that the Sun's cycle is about 11 years rolling through periods of quiet to times of intense activity. When the Sun is super-intense it releases explosions of light and solar material. This time is a solar maximum.

When the Sun is in a quiet state this period is called the solar minimum.

Over the course of one solar cycle (one 11-year period), the Sun’s total emitted energy varies on average at about 0.1 percent. That may not sound like a lot, but the Sun emits a large amount of energy – 1,361 watts per square meter. Even fluctuations at just a tenth of a percent can affect Earth. That's why TSIS-1 is launching: to help scientists understand and anticipate how changes in the Sun will affect us on Earth.

3. You're so vain. You probably think this climate model is about you.

Scientists use computer models to interpret changes in the Sun’s energy input. If less solar energy is available, scientists can gauge how that affects Earth’s atmosphere, oceans, weather and seasons by using computer simulations. But the Sun is just one of many factors scientists use to model Earth’s climate. A lot of other factors come into play in addition to the energy from the Sun. Factors like greenhouse gases, clouds scattering light and small particles in the atmosphere called aerosols all can affect Earth’s climate so they all need to be included in climate models. So, while we need to measure the total amount of energy from the Sun, we also need to understand how these other factors alter the amount of energy reaching Earth's surface and affect our climate.

4. Someday we'll find it, the rainbow connection. The lovers, the dreamers and me.

We receive the Sun's energy in many different wavelengths, including visible light (rainbows!) as well as light we can't see like infrared and ultraviolet wavelengths. Each color or wavelength of light from the Sun affects Earth’s atmosphere differently.

For instance, ultraviolet light from the Sun can affect Earth's ozone. High in the atmosphere is a layer of protective ozone gas. Ozone is Earth’s natural sunscreen, absorbing the Sun’s most harmful ultraviolet radiation and protecting living things below. But ozone is vulnerable to certain gases made by humans that reach the upper atmosphere. Once there, they react in the presence of sunlight to destroy ozone molecules. Currently, several satellites from us and the National Oceanic and Atmospheric Administration (NOAA) track the ozone in the upper atmosphere and the solar energy that drives the photochemistry that creates and destroys ozone. Our new instrument, TSIS-1, will join that fleet with even better accuracy.

TSIS-1 will see different types of ultraviolet (UV) light, including UV-B and UV-C. Each plays a different role in the ozone layer. UV-C rays are essential in creating ozone. UV-B rays and some naturally occurring chemicals regulate the abundance of ozone in the upper atmosphere. The amount of ozone is a balance between these natural production and loss processes.

TSIS-1 data of the Sun's UV energy will help improve computer models of the atmosphere that need accurate measurements of sunlight across the ultraviolet spectrum to model the ozone layer correctly. While UV light represents a tiny fraction of the total sunlight that reaches the top of Earth's atmosphere, it fluctuates from 3 to 10 percent, a change that, in turn causes small changes in the chemical composition and thermal structure of the upper atmosphere.

This is just one of the important applications of TSIS-1 measurements. TSIS-1 will measure how the Sun's energy is distributed over 1,000 different wavelengths.

5. Every move you make…every step you take, I'll be watching you.

TSIS-1 will continue our nearly 40 years of closely studying the total amount of energy the Sun sends to Earth from space. We've previously studied this 'total solar irradiance' with nine previous satellites, currently with Solar Radiation and Climate Experiment, (SORCE).

NASA’s SORCE collected this data on the total amount of the Sun’s radiant energy throughout Sept. 2017. The satellite actually detected a dip in total irradiance – or the total amount of energy from the Sun- during the month’s intense solar activity.

But there's still very much we don't know about total solar irradiance. We do not know how it varies over longer timescales. Longer term observations are especially important because scientists have observed unusually quiet magnetic activity from the Sun for the past two decades with previous satellites. During the last prolonged solar minimum in 2008-2009, our Sun was the quietest it has ever been since we started observations in 1978. Scientists expect the Sun to enter a solar minimum within the next three years, and TSIS-1 will be primed to take measurements of the next minimum and see if this is part of a larger trend.

For all the latest Earth updates, follow us on Twitter @NASAEarth or Facebook. 

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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.

Put to the Test: Orion Service Module

Blasted with sound, shaken for hours and pyro detonated, the Orion Service Module Completes Ground Tests at our Glenn Research Center

We recently completed a structural integrity evaluation on the test version of the Orion service module at our Plum Brook Station in Sandusky, Ohio. Designed to ensure the module can withstand launch atop the Space Launch System (SLS) rocket, the battery of tests was conducted in stages over a 16-month period.

The 13-ton European service module will power, propel and cool Orion, while supplying vital oxygen and water to its crew during future missions.

The Powerhouse: Space Launch System and Orion

Our Space Launch System is an advanced launch vehicle that will usher in a new era of human exploration beyond Earth’s orbit. SLS, with its unparalleled power and capabilities, will launch missions to explore deep-space destinations aboard our Orion spacecraft.

What is Orion? Named after one of the largest constellations in the night sky and drawing from more than 50 years of spaceflight research and development, the Orion spacecraft will be the safest, most advanced spacecraft ever built. It will be flexible and capable enough to take astronauts to a variety of deep destinations, including Mars.

Welcome to the Buckeye State

In November 2015, the full-sized test version of the Orion service module arrived at Cleveland Hopkins Airport aboard an Antonov AN-124. After being unloaded from one of the world’s largest transport aircraft, the module was shipped more than 50 miles by truck to Plum Brook for testing.

Spread Your Wings

The first step of the service module’s ground test journey at Plum Brook’s Space Power Facility, saw one of its 24-foot solar array wings deployed to verify operation of the power system. The test confirmed the array extended and locked into place, and all of the wing mechanisms functioned properly.

Can You Hear SLS Now?

The SLS will produce a tremendous amount of noise as it launches and climbs through our atmosphere. In fact, we’re projecting the rocket could produce up to 180 decibels, which is louder than 20 jet engines operating at the same time.

While at the Reverberant Acoustic Test Facility, the service module was hit with more than 150 decibels and 20-10,000 hertz of sound pressure. Microphones were placed inside the test environment to confirm it matched the expected acoustic environment during launch.

After being blasted by sound, it was time to rock the service module, literally.

Shake Without the Bake 

Launching atop the most powerful rocket ever built – we’re talking more than eight million pounds of thrust – will subject Orion to stresses never before experienced in spaceflight.

To ensure the launch doesn’t damage any vital equipment, the engineering team utilized the world’s most powerful vibration table to perform nearly 100 different tests, ranging from 2.5 Hz to 100 Hz, on the module in the summer of 2016. 

Gotta Keep ‘Em Separated

The team then moved the Orion test article from the vibration table into the high bay for pyroshock tests, which simulated the shock the service module will experience as it separates from the SLS during launch.

Following the sound, vibration and separation tests, a second solar array wing deployment was conducted to ensure the wing continued to properly unfurl and function.

Headed South for the Summer

The ground test phase was another crucial step toward the eventual launch of Exploration Mission-1, as it validated extensive design prep and computer modeling, and verified the spacecraft met our safety and flight requirements.

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Any advice for young girls going into the sciences?

Astronaut Journal Entry - Alarms

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.

The smoke detectors have been setting off alarms. This happens routinely due to dust circulating in the modules, but every alarm is taken seriously. This is the third time that the alarm has sounded while I was using the Waste & Hygiene Compartment (toilet). I am starting to think that my actions are causing the alarms…. maybe I should change my diet?

Find more ‘Captain’s Log’ entries HERE.

Follow NASA astronaut Scott Tingle on Instagram and Twitter.

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

NASA Spotlight: Carbon Cycle and Ecosystems Earth Scientist Erika Podest 

Dr. Erika Podest is a scientist with the Carbon Cycle and Ecosystems Group in our Jet Propulsion Laboratory’s Earth Science Division and Visiting Associate Researcher in the Joint Institute for Regional Earth System Science and Engineering (JIFRESSE) at UCLA. Her research entails using satellite images to study Earth’s ecosystems specifically related to wetlands and boreal forests and how they are being affected by climate change. 

Erika took time from studying our home planet to answer questions about her life and career! Get to know our Earth Scientist: 

What inspires/motivates you?

I am inspired by the beauty of nature, its perfection and by the peace it brings me. My motivation is to make a positive impact on our planet by better understanding it and caring for it.

What first sparked your interest in Earth science?

I was born and raised in Panama, which is a country with an exuberant nature. Since I can remember, I was always surrounded by nature because my father was an adventurer who loved the outdoors and always took me with him to go exploring or simply to enjoy a nice relaxing day outside. This led me to develop a deep sense of appreciation, respect, and curiosity for nature, which sparked my interest to learn about it and pursue a career in Earth Science.

What got you interested in the study of Earth from space?

Early in my college years I was training for my private pilot’s license and during my solo flights I would take pictures of features on the surface from the plane. I was always amazed at the details the pictures showed of the landscape that were not obvious from the ground. This was the first step towards discovering that there was a field for studying Earth from above, called remote sensing and consequently my Masters and Ph.D. were focused in this field.

What technology, discovery, or policy do you think has the most potential to decrease humans’ environmental impact (e.g. wind turbines, carbon taxes, clean meat)?

I don’t think it is a matter of any one technology, discovery or policy. It is a combination of everything. Having an impact on climate change involves every level and direction, from the bottom up at the individual, grassroots and community level to the top down at the policy level. As individuals, I think it is important to educate ourselves about climate change (I suggest climate.nasa.gov). We all have the power to make a positive change by speaking up and making informed decisions about our consumptive habits.

What’s a fact about the role of wetlands and boreal forests in the global ecosystem that you think would surprise people?

Wetlands provide a vital role in carbon storage. Even though they cover about 5-8% of the Earth’s land surface, studies indicate that they contain a disproportionate amount of our planet’s total soil carbon, about 20-30%. In addition, they are like the arteries and veins of the landscape, acting as water sources and purifiers and helping in flood control. They also protect our shores and harbor large amounts of biodiversity.

Boreal forests are found in the uppermost northern hemisphere (Alaska, most of Canada, Russia, Scandinavia and northern Asia) and account for about 30% of the world’s forest cover. These forests lock up enormous amounts of carbon and help slow the increasing buildup of carbon dioxide in our atmosphere. In their peak growth phase during the northern spring and summer, the worldwide levels of carbon dioxide fall and the worldwide levels of oxygen rise. 

Can you describe a typical day on a research trip?

It depends on the research trip. For example, one of my more recent ones was to the Peruvian Amazon where we went upriver on a boat for three weeks on a major tributary of the Amazon River called the Ucuyali River. I was with a team of eight researchers and we were studying the wetland ecosystems of the Pacaya-Samiria Natural Reserve, which entailed making vegetation measurements and assessing inundation extent to validate our scientific findings from satellite observations. We camped for most of the trip and a typical day entailed waking up at around 5:00 am with a symphony of sounds that emerged from the forest, including monkeys. We had breakfast and set off from base camp into the forest (~1 hour walk) to work an 8-9 hour day with a short lunch break (we had packed lunches) at noon. At the end of the day I’d be drenched in sweat, sunscreen, insect repellent, and dust and I’d bathe with water from the river, which was as brown as a milk chocolate bar. It was the most refreshing and cleansing feeling! The day would close with dinner followed with a discussion of the measurements to be collected the following day. Lights were out by 7:30 pm (which seemed like midnight) and I’d re-emerge myself into my tent in the dark tropical night surrounded by the sounds of the forest, until the next morning.

What are some of the most important lessons you’ve learned in life?

That it is important to be patient, humble and thankful.

Do you have any secret skills, talents, or hobbies?

Great question! I do not have any secrete skills or talents but I do have a couple of hobbies. I play the piano, though I am still a novice. I love windsurfing. It is an amazing feeling to skim over the water at fast speeds (I’m also an adrenaline junkie). Finally, I am fascinated by magic card tricks and whenever I have some free time I like to learn a new trick.

What do you enjoy the most about your job?

I enjoy constantly learning about our natural world and how it works. I also really enjoy communicating my work to students and to the general public. I find it especially rewarding when I can educate people and motivate students to consider careers in science.

Erika, thank you for your time and everything you do to keep our home planet safe!

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The Great Conjunction of Jupiter and Saturn

Credits:  NASA/Bill Ingalls

Have you noticed two bright objects in the sky getting closer together with each passing night? It’s Jupiter and Saturn doing a planetary dance that will result in the Great Conjunction on Dec. 21. On that day, Jupiter and Saturn will be right next to each other in the sky – the closest they have appeared in nearly 400 years!

Skywatching Tips from NASA

Credits: NASA/JPL-Caltech

For those who would like to see this phenomenon for themselves, here’s what to do:

Find a spot with an unobstructed view of the sky, such as a field or park. Jupiter and Saturn are bright, so they can be seen even from most cities.

An hour after sunset, look to the southwestern sky. Jupiter will look like a bright star and be easily visible. Saturn will be slightly fainter and will appear slightly above and to the left of Jupiter until December 21, when Jupiter will overtake it and they will reverse positions in the sky.

The planets can be seen with the unaided eye, but if you have binoculars or a small telescope, you may be able to see Jupiter’s four large moons orbiting the giant planet.

How to Photograph the Conjunction

Credits: NASA/Bill Dunford

Saturn and Jupiter are easy to see without special equipment, and can be photographed easily on DSLR cameras and many cell phone cameras. Here are a few tips and tricks:

These planets are visible in the early evening, and you'll have about 1-2 hours from when they are visible, to when they set. A photo from the same location can look completely different just an hour later!

Using a tripod will help you hold your camera steady while taking longer exposures. If you don’t have a tripod, brace your camera against something – a tree, a fence, or a car can all serve as a tripod for a several-second exposure.

The crescent Moon will pass near Jupiter and Saturn a few days before the conjunction. Take advantage of it in your composition!

Get more tips HERE.

Still have questions about the Great Conjunction?

Our NASA expert answered questions from social media on an episode of NASA Science Live on Thursday, Dec. 17. Watch the recording HERE.

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Solar System: 10 Things to Know This Week

Planets Outside Our Solar System

Let the planet-hunting begin!

Our Transiting Exoplanet Survey Satellite (TESS), which will scan the skies to look for planets beyond our solar system—known as exoplanets—is now in Florida to begin preparations for launch in April. Below, 10 Things to know about the many, many unknown planets out there awaiting our discovery.

1—Exo-what?

We call planets in our solar system, well, planets, but the many planets we’re starting to discover outside of our solar system are called exoplanets. Basically, they’re planets that orbit another star.

2—All eyes on TRAPPIST-1.

Remember the major 2016 announcement that we had discovered seven planets 40 light-years away, orbiting a star called TRAPPIST-1? Those are all exoplanets. (Here’s a refresher.)

3—Add 95 new ones to that.

Just last month, our Kepler telescope discovered 95 new exoplanets beyond our solar system (on top of the thousands of exoplanets Kepler has discovered so far). The total known planet count beyond our solar system is now more than 3,700. The planets range in size from mostly rocky super-Earths and fluffy mini-Neptunes, to Jupiter-like giants. They include a new planet orbiting a very bright star—the brightest star ever discovered by Kepler to have a transiting planet.

4—Here comes TESS.

How many more exoplanets are out there waiting to be discovered? TESS will monitor more than 200,000 of the nearest and brightest stars in search of transit events—periodic dips in a star’s brightness caused by planets passing in front—and is expected to find thousands of exoplanets.

5—With a sidekick, too.

Our upcoming James Webb Space Telescope, will provide important follow-up observations of some of the most promising TESS-discovered exoplanets. It will also allow scientists to study their atmospheres and, in some special cases, search for signs that these planets could support life.

6—Prepped for launch.

TESS is scheduled to launch on a SpaceX Falcon 9 rocket from Cape Canaveral Air Force Station nearby our Kennedy Space Center in Florida, no earlier than April 16, pending range approval.

7—A groundbreaking find.

In 1995, 51 Pegasi b (also called "Dimidium") was the first exoplanet discovered orbiting a star like our Sun. This find confirmed that planets like the ones in our solar system could exist elsewhere in the universe.

8—Trillions await.

A recent statistical estimate places, on average, at least one planet around every star in the galaxy. That means there could be a trillion planets in our galaxy alone, many of them in the range of Earth’s size.

9—Signs of life.

Of course, our ultimate science goal is to find unmistakable signs of current life. How soon can that happen? It depends on two unknowns: the prevalence of life in the galaxy and a bit of luck. Read more about the search for life.

10—Want to explore the galaxy?

No need to be an astronaut. Take a trip outside our solar system with help from our Exoplanet Travel Bureau.

Read the full version of this week’s ‘10 Things to Know’ article HERE. 

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