This month you can catch a rare sight in the pre-dawn sky: five planets at once! If you look to the south (or to the north if you’re in the southern hemisphere) between about 5:30 and 6 a.m. local time you’ll see Mercury, Venus, Saturn, Mars and Jupiter lined up like jewels on a necklace. They’re beautiful in the sky, and even more fascinating when you look closely.
This week we’re taking a tour of the planets with recent information about each:
1. Artistic License
Craters on Mercury are named for writers and artists of all kinds. There are Tolstoy, Thoreau and Tolkien craters, for example, as well as those that bear the names of the Brontës, photographer Dorothea Lange and dancer Margot Fonteyn. See the complete roster of crater names HERE.
2. Lifting the Veil of Venus
A thick covering of clouds made Venus a mystery for most of human history. In recent decades, though, a fleet of robotic spacecraft has helped us peer past the veil and learn more about this world that is so like the Earth in some ways — and in some ways it’s near opposite.
3. Curious?
Have you ever wanted to drive the Mars Curiosity rover? You can take the controls using our Experience Curiosity simulation. Command a virtual rover as you explore the terrain in Gale Crater, all using real data and images from Mars. Try it out HERE.
4. Now That’s a Super Storm
Winter weather often makes headlines on Earth — but on Jupiter there’s a storm large enough to swallow our entire planet several times over. It’s been raging for at least three hundred years! Learn about the Great Red Spot HERE.
5. Ring Watcher
This week, the Cassini spacecraft will be making high-resolution observations of Saturn’s entrancing rings. This is a simulated look at Saturn, along with actual photos of the rings from the Cassini mission.
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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It’s the 1970s, and we’re about to send two spacecraft (Voyager 1 & 2) into space. These two spacecraft will eventually leave our solar system and become the most distant man-made objects…ever. How can we leave our mark on them in the case that other spacefarers find them in the distant future?
The Golden Record.
We placed an ambitious message aboard Voyager 1 and 2, a kind of time capsule, intended to communicate a story of our world to extraterrestrials. The Voyager message is carried by a phonograph record, a 12-inch gold-plated copper disk containing sounds and images selected to portray the diversity of life and culture on Earth.
The Golden Record Cover
The outward facing cover of the golden record carries instructions in case it is ever found. Detailing to its discoverers how to decipher its meaning.
In the upper left-hand corner is an easily recognized drawing of the phonograph record and the stylus carried with it. The stylus is in the correct position to play the record from the beginning. Written around it in binary arithmetic is the correct time of one rotation of the record. The drawing indicates that the record should be played from the outside in.
The information in the upper right-hand portion of the cover is designed to show how the pictures contained on the record are to be constructed from the recorded signals. The top drawing shows the typical signal that occurs at the start of the picture. The picture is made from this signal, which traces the picture as a series of vertical lines, similar to ordinary television. Immediately below shows how these lines are to be drawn vertically, with staggered “interlace” to give the correct picture rendition. Below that is a drawing of an entire picture raster, showing that there are 52 vertical lines in a complete picture.
Immediately below this is a replica of the first picture on the record to permit the recipients to verify that they are decoding the signals correctly. A circle was used in this picture to ensure that the recipients use the correct ratio of horizontal to vertical height in picture reconstruction.
The drawing in the lower left-hand corner of the cover is the pulsar map previously sent as part of the plaques on Pioneers 10 and 11. It shows the location of the solar system with respect to 14 pulsars, whose precise periods are given.
The drawing containing two circles in the lower right-hand corner is a drawing of the hydrogen atom in its two lowest states, with a connecting line and digit 1 to indicate that the time interval associated with the transition from one state to the other is to be used as the fundamental time scale, both for the time given on the cover and in the decoded pictures.
The Contents
The contents of the record were selected for NASA by a committee chaired by Carl Sagan of Cornell University and his associates.
They assembled 115 images and a variety of natural sounds, such as those made by surf, wind and thunder, birds, whales and other animals. To this, they added musical selections from different cultures and eras, and spoken greetings from Earth-people in fifty-five languages, and printed messages from President Carter and U.N. Secretary General Waldheim.
Listen to some of the sounds of the Golden Record on our Soundcloud page:
Golden Record: Greetings to the Universe
Golden Record: Sounds of Earth
Songs from Chuck Berry’s “Johnny B. Goode,” to Beethoven’s Fifth Symphony are included on the golden record. For a complete list of songs, visit: https://voyager.jpl.nasa.gov/golden-record/whats-on-the-record/music/
The 115 images included on the record, encoded in analog form, range from mathematical definitions to humans from around the globe. See the images here: https://voyager.jpl.nasa.gov/golden-record/whats-on-the-record/images/
Making the Golden Record
Many people were instrumental in the design, development and manufacturing of the golden record.
Blank records were provided by the Pyral S.A. of Creteil, France. CBS Records contracted the JVC Cutting Center in Boulder, CO to cut the lacquer masters which were then sent to the James G. Lee Record Processing center in Gardena, CA to cut and gold plate eight Voyager records.
The record is constructed of gold-plated copper and is 12 inches in diameter. The record’s cover is aluminum and electroplated upon it is an ultra-pure sample of the isotope uranium-238. Uranium-238 has a half-life of 4.468 billion years.
Learn more about the golden record HERE.
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Join the Mission Juno virtual imaging team by helping us to determine the best locations in Jupiter's atmosphere that JunoCam will capture. Voting is open January 19-23, 2017. Visit www.missionjuno.swri.edu/junocam for more information about JunoCam voting.
Our Hubble Space Telescope is providing a road map for the two Voyager spacecraft as they hurtle through unexplored territory on their trip beyond our solar system. Along the way, the Voyager craft are measuring the interstellar medium, the mysterious environment between stars. Hubble is measuring the material along the probes' future trajectories and even after the Voyagers run out of electrical power and are unable to send back new data, which may happen in about a decade, astronomers can use Hubble observations to characterize the environment of through which these silent ambassadors will glide.
Mars needs YOU! In the future, Mars will need all kinds of explorers, farmers, surveyors, teachers . . . but most of all YOU! Join us on the Journey to Mars as we explore with robots and send humans there one day. Download a Mars poster that speaks to you. Be an explorer!
Each sol, or Martian day, the Mars Curiosity Team tracks the rover’s progress. And you can track them too at: http://mars.nasa.gov/msl/mission/mars-rover-curiosity-mission-updates/.
January 22 is the 425th birthday of Pierre Gassendi, French philosopher, priest, scientist, astronomer, mathematician and an active observational scientist. He was the first to publish data on the 1631 transit of Mercury. The Lunar Crater Gassendi is named for him.
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How did your launch abort affect your future space flights?
Brandon Rodriguez is an education specialist at our Jet Propulsion Laboratory (JPL) in Pasadena, California where he provides resources and training to K-12 schools across the Southwest. Working with a team at JPL, he develops content for classroom teachers, visits schools and speaks with students and trains future teachers to bring NASA into their classroom. When he’s not in the classroom, Brandon’s job takes him on research expeditions all around the world, studying our planet’s extreme environments.
Fun fact: Brandon wakes up every morning to teach an 8 a.m. physics class at a charter school before heading to JPL and clocking in at his full time job. When asked why? He shared, “The truth is that I really feel so much better about my role knowing that we’re not ‘telling’ teachers what to do from our ivory tower. Instead, I can “share” with teachers what I know works not just in theory, but because I’m still there in the classroom doing it myself.” - Brandon Rodriguez
Brandon took time from exciting the next generation of explorers to answer some questions about his life and his career:
I was over the moon when I got a call from NASA Education. I began my career as a research scientist, doing alternative energy work as a chemist. After seven years in the field, I began to feel as if I had a moral responsibility to bring access to science to a the next generation. To do so, I quit my job in science and became a high school science teacher. When NASA called, they asked me if I wanted a way to be both a scientist and an educator- how could I resist?
I haven't been back to Venezuela since I was very young, which has been very difficult for me. Being an immigrant in the USA sometimes feels like you're an outsider of both sides: I'm not truly Latin, nor am I an American. When I was young, I struggled with this in ways I couldn't articulate, which manifested in a lot of anger and got me in quite a bit of trouble. Coming to California and working in schools that are not only primarily Latinx students, but also first generation Latinx has really helped me process that feeling, because it's something I can share with those kids. What was once an alienating force has become a very effective tool for my teaching practice.
I'm so fortunate that my role takes me all over the world and into environments that allow to me to continue to develop while still sharing my strengths with the education community. I visit schools all over California and the Southwest of the USA to bring professional development to teachers passionate about science. But this year, I was also able to join the Ocean Exploration Trust aboard the EV Nautilus as we explored the Pacific Remote Island National Marine Monument. We were at sea for 23 days, sailing from American Samoa to Hawaii, using submersible remotely operated vehicles to explore the ocean floor.
Image Credit: Nautilus Live
We collected coral and rock samples from places no one has ever explored before, and observed some amazing species of marine creatures along the way.
Image Credit: Nautilus Live
There's no greater motivation than seeing the product of your hard work, and I get that everyday through students. I get to bring them NASA research that is "hot off the press" in ways that their textbooks never can. They see pictures not online or on worksheets, but from earlier that day as I walked through JPL. It is clearly that much more real and tangible to them when they can access it through their teacher and their community.
As someone who struggled- especially in college- I want people to know that what they struggle with isn't science, it's science classes. The world of research doesn't have exams; it doesn't have blanks to be filled in or facts to be memorized. Science is exploring the unknown. Yes, of course we need the tools to properly explore, and that usually means building a strong academic foundation. But it helped me to differentiate the end goal from the process: I was bad at science tests, but I wanted to someday be very good at science. I could persevere through the former if it got me to the latter.
Europa, without a doubt. Imagine if we found even simple life once more in our solar system- and outside of the habitable zone, no less. What would this mean for finding life outside of our solar system as a result? We would surely need to conclude that our sky is filled with alien worlds looking back at us.
While I never worked closely with the mission, Insight was a really important project for me. It's the first time while at JPL I was able to see the construction, launch and landing of a mission.
For as long as I can remember, I've been watching and reading science fiction, and I continue to be amazed at how fiction informs reality. How long ago was it that in Star Trek, the crew would be handing around these futuristic computer tablets that decades later would become common iPads? In their honor, I would be delighted if we named a ship Enterprise.
Thanks so much Brandon!
Additional Image Credit: MLParker Media
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On June 17, our MAVEN (Mars Atmosphere and Volatile Evolution Mission) will celebrate 1,000 Earth days in orbit around the Red Planet.
Since its launch in November 2013 and its orbit insertion in September 2014, MAVEN has been exploring the upper atmosphere of Mars. MAVEN is bringing insight to how the sun stripped Mars of most of its atmosphere, turning a planet once possibly habitable to microbial life into a barren desert world.
10. Unprecedented Ultraviolet View of Mars
Revealing dynamic, previously invisible behavior, MAVEN was able to show the ultraviolet glow from the Martian atmosphere in unprecedented detail. Nightside images showed ultraviolet “nightglow” emission from nitric oxide. Nightglow is a common planetary phenomenon in which the sky faintly glows even in the complete absence of eternal light.
9. Key Features on the Loss of Atmosphere
Some particles from the solar wind are able to penetrate unexpectedly deep into the upper atmosphere, rather than being diverted around the planet by the Martian ionosphere. This penetration is allowed by chemical reactions in the ionosphere that turn the charged particles of the solar wind into neutral atoms that are then able to penetrate deeply.
8. Metal Ions
MAVEN made the first direct observations of a layer of metal ions in the Martian ionosphere, resulting from incoming interplanetary dust hitting the atmosphere. This layer is always present, but was enhanced dramatically by the close passage to Mars of Comet Siding Spring in October 2014.
7. Two New Types of Aurora
MAVEN has identified two new types of aurora, termed “diffuse” and “proton” aurora. Unlike how we think of most aurorae on Earth, these aurorae are unrelated to either a global or local magnetic field.
6. Cause of the Aurorae
These aurorae are caused by an influx of particles from the sun ejected by different types of solar storms. When particles from these storms hit the Martian atmosphere, they can also increase the rate of loss of gas to space, by a factor of ten or more.
5. Complex Interactions with Solar Wind
The interactions between the solar wind and the planet are unexpectedly complex. This results due to the lack of an intrinsic Martian magnetic field and the occurrence of small regions of magnetized crust that can affect the incoming solar wind on local and regional scales. The magnetosphere that results from the interactions varies on short timescales and is remarkably “lumpy” as a result.
4. Seasonal Hydrogen
After investigating the upper atmosphere of the Red Planet for a full Martian year, MAVEN determined that the escaping water does not always go gently into space. The spacecraft observed the full seasonal variation of hydrogen in the upper atmosphere, confirming that it varies by a factor of 10 throughout the year. The escape rate peaked when Mars was at its closest point to the sun and dropped off when the planet was farthest from the sun.
3. Gas Lost to Space
MAVEN has used measurements of the isotopes in the upper atmosphere (atoms of the same composition but having different mass) to determine how much gas has been lost through time. These measurements suggest that 2/3 or more of the gas has been lost to space.
2. Speed of Solar Wind Stripping Martian Atmosphere
MAVEN has measured the rate at which the sun and the solar wind are stripping gas from the top of the atmosphere to space today, along with details of the removal process. Extrapolation of the loss rates into the ancient past – when the solar ultraviolet light and the solar wind were more intense – indicates that large amounts of gas have been lost to space through time.
1. Martian Atmosphere Lost to Space
The Mars atmosphere has been stripped away by the sun and the solar wind over time, changing the climate from a warmer and wetter environment early in history to the cold, dry climate that we see today.
Maven will continue its observations and is now observing a second Martian year, looking at the ways that the seasonal cycles and the solar cycle affect the system.
For more information about MAVEN, visit: www.nasa.gov/maven
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When NASA began operations on Oct. 1, 1958, we consisted mainly of the four laboratories of our predecessor, the National Advisory Committee for Aeronautics (NACA). Hot on the heels of NASA’s first day of business, we opened the Goddard Space Flight Center. Chartered May 1, 1959, and located in Greenbelt, Maryland, Goddard is home to one of the largest groups of scientists and engineers in the world. These people are building, testing and experimenting their way toward answering some of the universe’s most intriguing questions.
Goddard instruments were crucial in tracking the hole in the ozone layer over Antarctica as it grew and eventually began to show signs of healing. Satellites and field campaigns track the changing height and extent of ice around the globe. Precipitation missions give us a global, near-real-time look at rain and snow everywhere on Earth. Researchers keep a record of the planet’s temperature, and Goddard supercomputer models consider how Earth will change with rising temperatures. From satellites in Earth’s orbit to field campaigns in the air and on the ground, Goddard is helping us understand our planet.
We’re piecing together the story of our cosmos, from now all the way back to its start 13.7 billion years ago. Goddard missions have contributed to our understanding of the big bang and have shown us nurseries where stars are born and what happens when galaxies collide. Our ongoing census of planets far beyond our own solar system (several thousand known and counting!) is helping us hone in on which ones might be potentially habitable.
Our Sun is an active star, with occasional storms and a constant outflow of particles, radiation and magnetic fields that fill the solar system out far past the orbit of Neptune. Goddard scientists study the Sun and its activity with a host of satellites to understand how our star affects Earth, planets throughout the solar system and the nature of the very space our astronauts travel through.
Goddard instruments (well over 100 in total!) have visited every planet in the solar system and continue on to new frontiers. What we’ve learned about the history of our solar system helps us piece together the mysteries of life: How did life in our solar system form and evolve? Can we find life elsewhere?
Today, Goddard communications networks bring down 98 percent of our spacecraft data – nearly 30 terabytes per day! This includes not only science data, but also key information related to spacecraft operations and astronaut health. Goddard is also leading the way in creating cutting-edge solutions like laser communications that will enable exploration – faster, better, safer – for generations to come. Pew pew!
Goddard’s technologists and engineers must often invent tools, mechanisms and sensors to return information about our universe that we may not have even known to look for when the center was first commissioned.
Behind every discovery is an amazing team of people, pushing the boundaries of humanity’s knowledge. Here’s to the ones who ask questions, find answers and ask questions some more!
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1. Earth's Changing Cryosphere
This year, we will launch two satellite missions that will increase our understanding of Earth's frozen reaches. Snow, ice sheets, glaciers, sea ice and permafrost, known as the cryosphere, act as Earth's thermostat and deep freeze, regulating temperatures by reflecting heat from the Sun and storing most of our fresh water.
2. GRACE-FO: Building on a Legacy and Forging Ahead
The next Earth science satellites set to launch are twins! The identical satellites of the GRACE Follow-On mission will build on the legacy of their predecessor GRACE by also tracking the ever-changing movement of water around our planet, including Earth's frozen regions. GRACE-FO, a partnership between us and the German Research Center for Geosciences (GFZ), will provide critical information about how the Greenland and Antarctic ice sheets are changing. GRACE-FO, working together, will measure the distance between the two satellites to within 1 micron (much less than the width of a human hair) to determine the mass below.
Greenland has been losing about 280 gigatons of ice per year on average, and Antarctica has lost almost 120 gigatons a year with indications that both melt rates are increasing. A single gigaton of water would fill about 400,000 Olympic-sized swimming pools; each gigaton represents a billion tons of water.
3. ICESat-2: 10,000 Laser Pulses a Second
In September, we will launch ICESat-2, which uses a laser instrument to precisely measure the changing elevation of ice around the world, allowing scientists to see whether ice sheets and glaciers are accumulating snow and ice or getting thinner over time. ICESat-2 will also make critical measurements of the thickness of sea ice from space. Its laser instrument sends 10,000 pulses per second to the surface and will measure the photons' return trip to satellite. The trip from ICESat-2 to Earth and back takes about 3.3 milliseconds.
4. Seeing Less Sea Ice
Summertime sea ice in the Arctic Ocean now routinely covers about 40% less area than it did in the late 1970s, when continuous satellite observations began. This kind of significant change could increase the rate of warming already in progress and affect global weather patterns.
5. The Snow We Drink
In the western United States, 1 in 6 people rely on snowpack for water. Our field campaigns such as the Airborne Snow Observatory and SnowEx seek to better understand how much water is held in Earth's snow cover, and how we could ultimately measure this comprehensively from space.
6. Hidden in the Ground
Permafrost - permanently frozen ground in the Arctic that contains stores of heat-trapping gases such as methane and carbon dioxide - is thawing at faster rates than previously observed. Recent studies suggest that within three to four decades, this thawing could be releasing enough greenhouse gases to make Arctic permafrost a net source of carbon dioxide rather than a sink. Through airborne and field research on missions such as CARVE and ABoVE - the latter of which will put scientists back in the field in Alaska and Canada this summer - our scientists are trying to improve measurements of this trend in order to better predict global impact.
7. Breaking Records Over Cracking Ice
Last year was a record-breaking one for Operation IceBridge, our aerial survey of polar ice. For the first time in its nine-year history, the mission carried out seven field campaigns in the Arctic and Antarctic in a single year. In total, the IceBridge scientists and instruments flew over 214,000 miles, the equivalent of orbiting the Earth 8.6 times at the equator.
On March 22, we completed the first IceBridge flight of its spring Arctic campaign with a survey of sea ice north of Greenland. This year marks the 10th Arctic spring campaign for IceBridge. The flights continue until April 27 extending the mission's decade-long mapping of the fastest-changing areas of the Greenland Ice Sheet and measuring sea ice thickness across the western Arctic basin.
8. OMG
Researchers were back in the field this month in Greenland with our Oceans Melting Greenland survey. The airborne and ship-based mission studies the ocean's role in melting Greenland's ice. Researchers examine temperatures, salinity and other properties of North Atlantic waters along the more than 27,000 miles (44,000 km) of jagged coastline.
9. DIY Glacier Modeling
Computer models are critical tools for understanding the future of a changing planet, including melting ice and rising seas. Our new sea level simulator lets you bury Alaska's Columbia glacier in snow, and, year by year, watch how it responds. Or you can melt the Greenland and Antarctic ice sheets and trace rising seas as they inundate the Florida coast.
10. Ice Beyond Earth
Ice is common in our solar system. From ice packed into comets that cruise the solar system to polar ice caps on Mars to Europa and Enceladus-the icy ocean moons of Jupiter and Saturn-water ice is a crucial ingredient in the search for life was we know it beyond Earth.
Read the full version of this week’s 10 Things to Know HERE.
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On Nov. 16, 2022, the Artemis I mission officially began with the launch of the Orion spacecraft atop the Space Launch System rocket. The rocket and spacecraft lifted off from historic Launch Complex 39B at NASA’s Kennedy Space Center in Florida.
Now, the Orion spacecraft is about halfway through its journey around the Moon. Although the spacecraft is uncrewed, the Artemis I mission prepares us for future missions with astronauts, starting with Artemis II.
Stay up-to-date with the mission with the latest full-resolution images, mission updates, on-demand and live video.
Find full-resolution images from the Orion spacecraft as they are released here.
Launch imagery can be found here. When Orion splashes down in the Pacific Ocean on Dec. 11, the images will be available here, as well!
This playlist contains informational videos, as well as upcoming and past live events, about Artemis I.
You can watch a livestream of the Artemis I mission here. (Just a note: the livestream may cut off during moments when the Orion team needs higher bandwidth for activities.)
Keep yourself updated on the upcoming broadcasts of Artemis milestones with the NASA TV schedule.
Our Artemis I Tracker uses live telemetry data streamed directly from Mission Control Center in Houston to show Orion position, attitude, solar array positions, and thruster firings throughout the mission.
“Eyes on the Solar System” shows Orion's position along the Artemis I trajectory and in relation to other NASA spacecraft and objects in the solar system.
“DSN Now” shows which antenna on Earth’s Deep Space Network is communicating with Orion.
Read up on where Orion is and what’s next in the Artemis I mission with the Mission Blog.
Thank you so much for following with us on this historic mission. Go Artemis!
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Michael S. Hopkins was selected by NASA as an astronaut in 2009. The Missouri native is currently the Crew-1 mission commander for NASA’s next SpaceX launch to the International Space Station on Nov. 14, 2020. Hopkin’s Crew-1 mission will mark the first-ever crew rotation flight of a U.S. commercial spacecraft with astronauts on board, and it secures the U.S.’s ability to launch humans into space from American soil once again. Previously, Hopkins was member of the Expedition 37/38 crew and has logged 166 days in space. During his stay aboard the station, he conducted two spacewalks totaling 12 hours and 58 minutes to change out a degraded pump module. He holds a Bachelor of Science in Aerospace Engineering from the University of Illinois and a Master of Science in Aerospace Engineering.
He took some time from being a NASA astronaut to answer questions about his life and career! Enjoy:
I hope people are thinking about the fact that we’re starting a new era in human spaceflight. We’re re-opening human launch capability to U.S. soil again, but it’s not just that. We’re opening low-Earth orbit and the International Space Station with commercial companies. It’s a lot different than what we’ve done in the past. I hope people realize this isn’t just another launch – this is something a lot bigger. Hopefully it’s setting the stage, one of those first steps to getting us to the Moon and on to Mars.
First off, just like being an astronaut, it involves a lot of training when you first get started. I went to the U.S. Air Force Test Pilot School and spent a year in training and just learning how to be a flight test engineer. It was one of the most challenging years I’ve ever had, but also one of the more rewarding years. What it means afterwards is, you are basically testing new vehicles or new systems that are going on aircraft. You are testing them before they get handed over to the operational fleet and squadrons. You want to make sure that these capabilities are safe, and that they meet requirements. As a flight test engineer, I would help design the test. I would then get the opportunity to go and fly and execute the test and collect the data, then do the analysis, then write the final reports and give those conclusions on whether this particular vehicle or system was ready to go.
A common theme for me is to just have patience. Enjoy the ride along the way. I think I tend to be pretty high intensity on things and looking back, I think things happen when they’re supposed to happen, and sometimes that doesn’t necessarily agree with when you think it should happen. So for me, someone saying, “Just be patient Mike, it’s all going to happen when it’s supposed to,” would be really good advice.
There’s a lot of experiments I had the opportunity to participate in, but the ones in particular I liked were ones where I got to interact directly with the folks that designed the experiment. One thing I enjoyed was a fluid experiment called Capillary Flow Experiment, or CFE. I got to work directly with the principal investigators on the ground as I executed that experiment. What made it nice was getting to hear their excitement as you were letting them know what was happening in real time and getting to hear their voices as they got excited about the results. It’s just a lot of fun.
I think most of us when we think about whatever it is we do, we don’t think of it in those terms. Space is risky, yes, but there’s a lot of other risky jobs out there. Whether it’s in the military, farming, jobs that involve heavy machinery or dangerous equipment… there’s all kinds of jobs that entail risk. Why do it? You do it because it appeals to you. You do it because it’s what gets you excited. It just feels right. We all have to go through a point in our lives where we figure out what we want to do and what we want to be. Sometimes we have to make decisions based on factors that maybe wouldn’t lead you down that choice if you had everything that you wanted, but in this particular case for me, it’s exactly where I want to be. From a risk standpoint, I don’t think of it in those terms.
There are many facets to Soichi Noguchi. I’m thinking about the movie Shrek. He has many layers! He’s very talented. He’s very well-thought. He’s very funny. He’s very caring. He’s very sensitive to other people’s needs and desires. He’s a dedicated family man. I could go on and on and on… so maybe like an onion – full of layers!
I love them both. But can I say Firefly? There’s a TV series out there called Firefly. It lasted one season – kind of a space cowboy-type show. They did have a movie, Serenity, that was made as well. But anyway, I love both Star Wars and Star Trek. We’ve really enjoyed The Mandalorian. I mean who doesn’t love Baby Yoda right? It’s all fun.
I tried four times over the course of 13 years. My first three attempts, I didn’t even have references checked or interviews or anything. Remember what we talked about earlier, about patience? For my fourth attempt, the fact is, it happened when it was supposed to happen. I didn’t realize it at the time. I would have loved to have been picked on my first attempt like anybody would think, but at the same time, because I didn’t get picked right away, my family had some amazing experiences throughout my Air Force career. That includes living in Canada, living overseas in Italy, and having an opportunity to work at the Pentagon. All of those helped shape me and grow my experience in ways that I think helped me be a better astronaut.
One of my favorite pictures was a picture inside the station at night when all of the lights were out. You can see the glow of all of the little LEDs and computers and things that stay on even when you turn off the overhead lights. You see this glow on station. It’s really one of my favorite times because the picture doesn’t capture it all. I wish you could hear it as well. I like to think of the station in some sense as being alive. It’s at that time of night when everybody else is in their crew quarters in bed and the lights are out that you feel it. You feel the rhythm, you feel the heartbeat of the station, you see it in the glow of those lights – that heartbeat is what’s keeping you alive while you’re up there. That picture goes a small way of trying to capture that, but I think it’s a special time from up there.
My wedding bands. I’m also taking up pilot wings for my son. He wants to be a pilot so if he succeeds with that, I’ll be able to give him his pilot wings. Last time, I took one of the Purple Hearts of a very close friend. He was a Marine in World War II who earned it after his service in the Pacific.
Thank you for your time, Mike, and good luck on your historic mission! Get to know a bit more about Mike and his Crew-1 crew mates Victor Glover, Soichi Noguchi, and Shannon Walker in the video above.
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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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