As Neil Armstrong became the first human to step foot onto another world on July 20, 1969, lunar dust collected on the boots of his spacesuit. He peered through the gold coating of his visor and looked out across the surface of the Moon, an entirely different landscape than he was used to.
Now, just in time for the 50th anniversary of the Moon landing, you can experience the boots that stepped in Moon dust and the visor that saw the moonscape up close. Neil Armstrong’s spacesuit from the historic Apollo 11 Moon landing is on display for the first time in 13 years in its new display case in the Wright Brothers & the Invention of the Aerial Age Gallery of the National Air and Space Museum.
This week, you can also watch us salute our Apollo 50th heroes and look forward to our next giant leap for future missions to the Moon and Mars. Tune in to a special two-hour live NASA Television broadcast at 1 p.m. ET on Friday, July 19. Watch the program at www.nasa.gov/live.
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Hi!! I’m a high school sophomore and I love the work NASA does! I’ve always wondered, what’s an astronaut’s first thought when leaving earth? What kind of experiences do you leave the expedition with? Thanks! :) - Lauren
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:
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!
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.
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.
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.
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.
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What do you hope to find using this new technology? When you were a kid, did you ever dream of landing on Mars? Even if you may not be visiting, tech that you have sway over is.
“When you wer a kid, did you ever dream of landing on Mars?”
I was looking at the GLOBE Observer experiments for citizens and was wondering how the eclipse affects the cloud type? Or, I guess, why is that an important thing to measure? Thank you for answering our questions!
As my dad likes to say, I went to college to take up space, so I’m not sure what happens in the atmosphere. However, I think that the atmospheric scientists are interested in the types of waves that will be set up by the temperature gradients generated by the eclipse. So as totality occurs you get a very fast temperature drop in a localized area. I believe this can set up strong winds which may affect the type of clouds and/or their shapes. This is going to be the best-observed eclipse! And one thing I’ve learned as a scientist is that you never know what you’ll find in your data so collect as much of it as possible even if you aren’t sure what you’ll find. That is sometimes when you get the most exciting results! Thanks for downloading the app and helping to collect the data!
Our Spitzer Space Telescope has revealed the first known system of seven Earth-size planets around a single star. Three of these planets are firmly located in an area called the habitable zone, where liquid water is most likely to exist on a rocky planet.
This exoplanet system is called TRAPPIST-1, named for The Transiting Planets and Planetesimals Small Telescope (TRAPPIST) in Chile. In May 2016, researchers using TRAPPIST announced they had discovered three planets in the system.
Assisted by several ground-based telescopes, Spitzer confirmed the existence of two of these planets and discovered five additional ones, increasing the number of known planets in the system to seven.
This is the FIRST time three terrestrial planets have been found in the habitable zone of a star, and this is the FIRST time we have been able to measure both the masses and the radius for habitable zone Earth-sized planets.
All of these seven planets could have liquid water, key to life as we know it, under the right atmospheric conditions, but the chances are highest with the three in the habitable zone.
At about 40 light-years (235 trillion miles) from Earth, the system of planets is relatively close to us, in the constellation Aquarius. Because they are located outside of our solar system, these planets are scientifically known as exoplanets. To clarify, exoplanets are planets outside our solar system that orbit a sun-like star.
In this animation, you can see the planets orbiting the star, with the green area representing the famous habitable zone, defined as the range of distance to the star for which an Earth-like planet is the most likely to harbor abundant liquid water on its surface. Planets e, f and g fall in the habitable zone of the star.
Using Spitzer data, the team precisely measured the sizes of the seven planets and developed first estimates of the masses of six of them. The mass of the seventh and farthest exoplanet has not yet been estimated.
For comparison…if our sun was the size of a basketball, the TRAPPIST-1 star would be the size of a golf ball.
Based on their densities, all of the TRAPPIST-1 planets are likely to be rocky. Further observations will not only help determine whether they are rich in water, but also possibly reveal whether any could have liquid water on their surfaces.
The sun at the center of this system is classified as an ultra-cool dwarf and is so cool that liquid water could survive on planets orbiting very close to it, closer than is possible on planets in our solar system. All seven of the TRAPPIST-1 planetary orbits are closer to their host star than Mercury is to our sun.
The planets also are very close to each other. How close? Well, if a person was standing on one of the planet’s surface, they could gaze up and potentially see geological features or clouds of neighboring worlds, which would sometimes appear larger than the moon in Earth’s sky.
The planets may also be tidally-locked to their star, which means the same side of the planet is always facing the star, therefore each side is either perpetual day or night. This could mean they have weather patterns totally unlike those on Earth, such as strong wind blowing from the day side to the night side, and extreme temperature changes.
Because most TRAPPIST-1 planets are likely to be rocky, and they are very close to one another, scientists view the Galilean moons of Jupiter – lo, Europa, Callisto, Ganymede – as good comparisons in our solar system. All of these moons are also tidally locked to Jupiter. The TRAPPIST-1 star is only slightly wider than Jupiter, yet much warmer.
How Did the Spitzer Space Telescope Detect this System?
Spitzer, an infrared telescope that trails Earth as it orbits the sun, was well-suited for studying TRAPPIST-1 because the star glows brightest in infrared light, whose wavelengths are longer than the eye can see. Spitzer is uniquely positioned in its orbit to observe enough crossing (aka transits) of the planets in front of the host star to reveal the complex architecture of the system.
Every time a planet passes by, or transits, a star, it blocks out some light. Spitzer measured the dips in light and based on how big the dip, you can determine the size of the planet. The timing of the transits tells you how long it takes for the planet to orbit the star.
The TRAPPIST-1 system provides one of the best opportunities in the next decade to study the atmospheres around Earth-size planets. Spitzer, Hubble and Kepler will help astronomers plan for follow-up studies using our upcoming James Webb Space Telescope, launching in 2018. With much greater sensitivity, Webb will be able to detect the chemical fingerprints of water, methane, oxygen, ozone and other components of a planet’s atmosphere.
At 40 light-years away, humans won’t be visiting this system in person anytime soon...that said...this poster can help us imagine what it would be like:
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For the first time in almost a decade, we're going back to Jupiter. Our Juno spacecraft arrives at the king of planets on the fourth of July. From a unique polar orbit, Juno will repeatedly dive between the planet and its intense belts of charged particle radiation. Juno's primary goal is to improve our understanding of Jupiter's formation and evolution, which will help us understand the history of our own solar system and provide new insight into how other planetary systems form.
In anticipation, here are a few things you need to know about the Juno mission and the mysterious world it will explore:
1. This is the Big One
The most massive planet in our solar system, with dozens of moons and an enormous magnetic field, Jupiter rules over a kind of miniature solar system.
2. Origin Story
Why study Jupiter in the first place? How does the planet fit into the solar system as a whole? What is it hiding? How will Juno unlock its secrets? A series of brief videos tells the stories of Jupiter and Juno. Watch them HERE.
3. Eyes on Juno
If you really want a hands-on understanding of Juno's flight through the Jupiter system, there's no better tool than the "Eyes on Juno" online simulation. It uses data from the mission to let you realistically see and interact with the spacecraft and its trajectory—in 3D and across both time and space.
4. You’re on JunoCam!
Did you know that you don't have to work for NASA to contribute to the Juno mission? Amateur astronomers and space enthusiasts everywhere are invited to help with JunoCam, the mission's color camera. You can upload your own images of Jupiter, comment on others' images, and vote on which pictures JunoCam will take when it reaches the Jovian system.
5. Ride Along
It's easy to follow events from the Juno mission as they unfold. Here are several ways to follow along online:
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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A rocket is launching to the International Space Station next week, carrying tons of science and supplies to the orbiting laboratory. It’s Northrop Grumman’s 14th (NG-14) commercial resupply cargo mission, and includes plant research, a new space toilet, and a special virtual reality camera designed to immerse you in a spacewalk. Let’s take a closer look at what’s on board, and how you can ask some of the scientists anything.
A new space toilet is heading to the space station. It’s smaller than the current toilets aboard the station, and includes a 3D printed titanium cover for its dual fan separator. These are just some of the upgrades that make it better suited for our deep space exploration missions. Engineers also gathered feedback from astronauts and set out to design more comfortable attachments that would make “boldly going” in space a more enjoyable experience. The toilet is being tested on the space station, and will also be used on a future Artemis mission. The new design will allow us to increase how much water we recover for use, because yep … yesterday’s coffee becomes tomorrow’s drinking water. See below for an opportunity to speak with the folks who made the new space toilet happen.
Astronauts traveling to the Moon and Mars will need to grow food to supplement their diets. The latest in plant studies aboard the space station hopes to pack a crunch in that research. We’ll be growing radishes in a special plant chamber, and learning how light, water, atmosphere, and soil conditions affect the bulbous vegetables. Radishes are nutritious, grow quickly (roughly four weeks from sowing to harvest), and are genetically similar to Arabidopsis, a plant frequently studied in microgravity. What we learn could help optimize growth of the plants in space as well as provide an assessment of their nutrition and taste. See below for an opportunity to ask anything of the scientist and engineer behind this new crop.
If going to space is on your bucket list, you might be closer than you think to checking that box. Felix & Paul Studios is creating an immersive 360 virtual reality film of a spacewalk that will put you right next to the astronauts as they go about their work on the outside of the space station … at 17,500 miles per hour. The new camera, specially designed to withstand the incredibly harsh environment of space, will be mounted on the station’s robotic arm so it can be maneuvered around the outside of the space station. Félix Lajeunesse and Paul Raphaël are the co-founders of the immersive entertainment studio, and have been producing a film aboard the space station – from Earth – for more than a year already. See below for a chance to ask them anything about what filming in space takes.
You can join in the NG-14 Reddit Ask Me Anything on Friday, Sept. 25 to ask anything of these folks and their projects. Here’s the schedule:
Space toilet (a.k.a the Universal Waste Management System): Melissa McKinley with NASA’s Advanced Exploration Systems and Jim Fuller of Collins Aerospace, and program manager for UWMS at 12 p.m. EDT at https://www.reddit.com/r/space.
Radishes in space (a.k.a. Plant Habitat-02): Dr. Karl Hasenstein is the scientist behind the Plant Habitat-02, and Dave Reed knows the ins and outs of the Advanced Plant Habitat of the space station. Their Reddit AMA begins at 3 p.m. EDT at https://www.reddit.com/r/gardening.
Virtual reality spacewalk camera: Félix Lajeunesse and Paul Raphaël co-founders and creative directors of Felix & Paul Studios will be taking questions at 5 p.m. EDT on https://www.reddit.com/r/filmmakers.
These are just a few of the payloads launching aboard the NG-14 Cygnus cargo vehicle to the space station next week. Read about the cancer research, and new commercial products also heading to space and watch the video above to learn more. Launch is targeted for Tuesday, Sept. 29, with a five-minute launch window opening at approximately 10:26 p.m. EDT. Live coverage begins on NASA TV at 10 p.m. EDT.
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Each month, we highlight a different research topic on the International Space Station. In August, our focus is biological research. Learning how spaceflight affects living organisms will help us understand potential health risks related to humans on long duration missions, including our journey to Mars.
Cells, microbes, animals and plants are affected by microgravity, and studying the processes involved in adaptation to spaceflight increases our fundamental understanding of biological processes on Earth. Results on Earth from biological research in space include the development of new medications, improved agriculture, advancements in tissue engineering and regeneration, and more.
Take a look at a few of the biological research experiments performed on space station:
Biomolecule Sequencer
Living organisms contain DNA, and sequencing DNA is a powerful way to understand how they respond to changing environments. The Biomolecule Sequencer experiment hopes to demonstrate (for the first time) that DNA sequencing is feasible in an orbiting spacecraft. Why? A space-based DNA sequencer could identify microbes, diagnose diseases and understand crew member health, and potentially help detect DNA- based life elsewhere in the solar system.
Ant-stronauts
Yes, ant-stronauts…as in ants in space. These types of studies provide insights into how ants answer collective search problems. Watching how the colony adapts as a unit in the quest for resources in extreme environments, like space, provides data that can be used to build algorithms with varied applications. Understanding how ants search in different conditions could have applications for robotics.
TAGES
The TAGES experiment (Transgenic Arabidopsis Gene Expression System) looks to see how microgravity impacts the growth of plant roots. Fluorescent markers placed on the plant’s genes allow scientists to study root development of Arabidopsis (a cress plant) grown on the space station. Evidence shows that directional light in microgravity skews root growth to the right, rather than straight down from the light source. Root growth patters on station mimic that of plants grown at at 45% degree angle on Earth. Space flight appears to slow the rate of the plant’s early growth as well.
Heart Cells
Spaceflight can cause a suite of negative health effects, which become more problematic as crew members stay in orbit for long periods of time. Effects of Microgravity on Stem Cell-Derived Cardiomycytes (Heart Cells) studies the human heart, specifically how heart muscle tissue contracts, grows and changes in microgravity. Understanding how heart muscle cells change in space improves efforts for studying disease, screening drugs and conducting cell replacement therapy for future space missions.
Medaka Fish
Chew on these results…Jaw bones of Japanese Medaka fish in microgravity show decreased mineral density and increased volume of osteoclasts, cells that break down bone tissue. Results from this study improve our understanding of the mechanisms behind bone density and organ tissue changes in space.
These experiments, and many others, emphasize the importance of biological research on the space station. Understanding the potential health effects for crew members in microgravity will help us develop preventatives and countermeasures.
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Astronomers may be closer than ever to discovering a planet that’s habitable like our own, but along the way they’ve discovered some very scary exoplanets – places where conditions are far too harsh for life as we know it to exist.
We’ve rounded up some of the most frightening, deadly exoplanets, places that make even the scariest haunted house on Earth pale in comparison. Check them out...
The exoplanets PSR B1257+12 B, C & D were among the first discovered, and also happened to be three of the weirdest! The entire system is a graveyard, remnants of what used to be a normal, functional solar system before the star blew apart in a giant explosion known as a supernova.
The massive shockwave from the supernova stripped away any atmosphere or living creatures that might have once lived on these planets, leaving behind ghostly, rocky shells, dead planets orbiting the corpse of an extinct star.
Except that the system isn’t completely dead…the remaining core from the old star has become a zombie star called a pulsar. Literally spinning in its grave, it makes a full rotation every 6.22 milliseconds and emits an intense beam of radiation that can be detected from Earth. The star’s unfortunate planets are thus bathed in deadly radiation on a regular basis, making sure that this system remains a cosmic no-man’s land.
The sound of howling wind is a must for any Earth-based haunted house, but weather conditions on HD 189733 b make it a very dangerous place to go trick-or-treating.
At first glance, this exoplanet looks like the typical “hot Jupiter” — a huge gas planet perched dangerously to a burning-hot star, with daytime temperatures around a balmy 1,770 degrees Fahrenheit. This exoplanet is also “tidally locked” in its orbit, which means that the same side of the planet always faces its star.
But when scientists measured the planet’s nighttime temperature, they were shocked to find that it was only 500 degrees cooler. How does the back side of the planet stay so warm?
The answer is wind! Insanely fast, dangerous wind that whisks heat from day-side to night-side at a speed of 4,500 mph, nearly six times the speed of sound! In fact, astronomers estimate that wind speeds might top out at 5,400 mph, conditions that make hurricanes on Earth look like a breezy day at the beach.
This exoplanet, named K2-33b, is the youngest fully formed exoplanet ever detected. This planet is a bit larger than Neptune and whips tightly around its star every five days. Since this planet sits nearly 10 times closer to its star than Mercury is to our sun, it’s HOT!
No matter how cute you think infants are, this is one baby you’d want to stay away from.
The planet HD 209458 b (aka. Osiris - the god of death) has a few things in common with Earth: water vapor, methane and carbon dioxide in its atmosphere, key ingredients for life on our planet. Don’t be fooled, though, because this planet is a rolling cauldron of almost unimaginable heat.
Even the hottest summer days on Earth don’t get as dangerous as the conditions here. A planet that orbits so close to its host star that its atmosphere is literally boiling off, ripped away from the planet as it whips around on its breakneck 3.5-day orbit.
While most of the exoplanets found so far are hellishly hot, OGLE-2005-BLG-390L b has the distinction of being extremely cold.
The planet takes about 10 Earth years to orbit its tiny dwarf star, and it’s a chilly trip; the average temperature on this exoplanet is 50 Kelvin, or minus 370 degrees Fahrenheit! A good costume for trick-or-treating on this frigid planet would be a toasty self-heating spacesuit, an oxygen supply, ice skates and plenty of hot cocoa.
Of course, don’t expect to find many houses with candy here, because despite the fact that it’s just a few times bigger than Earth, this exoplanet is an uninhabitable ice ball stuck in a perpetual winter freeze.
Kepler-10b is a scorched world, orbiting at a distance that’s more than 20 times closer to its star than Mercury is to our own sun. The daytime temperatures are expected to be more than 2,500 degrees Fahrenheit, hotter than lava flows here on Earth.
Intense radiation from the star has kept the planet from holding onto an atmosphere, but flecks of silicates and iron that have boiled off a molten surface are swept away by the stellar radiation.
Learn more about worlds beyond our solar system at: https://exoplanets.nasa.gov/
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With this new name, our Mars 2020 rover has now come to life! Chosen by middle school student Alex Mather, Perseverance helps to remind ourselves that no matter what obstacles we face, whether it's on the way to reaching our goals or on the way to Mars, we will push through. In Alex’s own words,
“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. The human race will always persevere into the future.”
Welcome to the family. ❤️
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