Dive into your creative stream
Earth’s 2015 surface temperatures were the warmest since modern record keeping began in 1880, according to independent analyses by NASA and the National Oceanic and Atmospheric Administration (NOAA).
Globally-averaged temperatures in 2015 shattered the previous mark set in 2014 by 0.23 degrees Fahrenheit (0.13 Celsius). Only once before, in 1998, has the new record been greater than the old record by this much.
The 2015 temperatures continue a long-term warming trend, according to analyses by scientists at NASA’s Goddard Institute for Space Studies (GISS) in New York. NOAA scientists concur with the finding that 2015 was the warmest year on record based on separate, independent analyses of the data.
Since the late-19th century, the planet’s average surface temperature has risen about 1.8 degrees Fahrenheit. This change is largely driven by increased carbon dioxide and other human-made emissions into the atmosphere.
An important thing to remember when reading this information is that it reflects global temperature average. That means that specific regions or areas could have experienced colder weather than usual, but overall the global temperature has risen.
How do we know? Our analyses incorporate surface temperature measurements from 6,300 weather stations, ship-and buoy-based observations of sea surface temperatures, and temperature measurements from Antarctic research stations.
What about El Niño? Phenomena such as El Niño or La Niña, which warm or cool the tropical Pacific Ocean, can contribute to short-term variations in global average temperature. Last year’s temperatures had an assist from a warming El Niño, but it is the cumulative effect of the long-term trend that has resulted in the record warming that we’re seeing.
The full 2015 surface temperature data set and the complete methodology used to make the temperature calculation are available HERE.
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We’re committed to exploration and discovery, journeying to the Moon, Mars, and beyond. But how do we guide our missions on their voyage among the stars? Navigation engineers lead the way!
Using complex mathematical formulas, navigation experts calculate where our spacecraft are and where they’re headed. No matter the destination, navigating the stars is a complicated challenge that faces all our missions. But, we think you’re up to the task!
Our space navigation workbook lets you explore the techniques and mathematical concepts used by navigation engineers. The book delves into groundbreaking navigation innovations like miniaturized atomic clocks, autonomous navigation technologies, using GPS signals at the Moon, and guiding missions through the solar system with X-ray emissions from pulsars — a type of neutron star. It also introduces you to experts working with NASA’s Space Communications and Navigation program at Goddard Space Flight Center in Greenbelt, Maryland.
If you’re a high schooler who dreams of guiding a rover across the rocky surface of Mars or planning the trajectory of an observer swinging around Venus en route to the Sun, this workbook is for you! Download it today and start your adventure with NASA: https://go.nasa.gov/3i7Pzqr
What's your main source of motivation?
First, I love what I do, and what has motivated me is the love that I have for science and learning new things. Then there are people who support you and keep you motivated. My mother was a source of motivation, as well as my family. My advisor Dr. Chopra was also a big supporter through graduate school.
We sent the first humans to land on the Moon in 1969. Since then, only of 12 men have stepped foot on the lunar surface – but we left robotic explorers behind to continue gathering science data. And now, we’re preparing to return. Establishing a sustained presence on and near the Moon will help us learn to live off of our home planet and prepare for travel to Mars.
To help establish ourselves on and near the Moon, we are working with a few select American companies. We will buy space on commercial robotic landers, along with other customers, to deliver our payloads to the lunar surface. We’re even developing lunar instruments and tools that will fly on missions as early as 2019!
Through partnerships with American companies, we are leading a flexible and sustainable approach to deep space missions. These early commercial delivery missions will also help inform new space systems we build to send humans to the Moon in the next decade. Involving American companies and stimulating the space market with these new opportunities to send science instruments and new technologies to deep space will be similar to how we use companies like Northrop Grumman and SpaceX to send cargo to the International Space Station now. These selected companies will provide a rocket and cargo space on their robotic landers for us (and others!) to send science and technology to our nearest neighbor.
So who are these companies that will get to ferry science instruments and new technologies to the Moon?
Here’s a digital “catalogue” of the organizations and their spacecraft that will be available for lunar services over the next decade:
Pittsburg, PA
Littleton, CO
Cedar Park, TX
Houston, TX
Littleton, CO
Mojave, CA
Cape Canaveral, FL
Edison, NJ
Cambridge, MA
We are thrilled to be working with these companies to enable us to investigate the Moon in new ways. In order to expand humanity’s presence beyond Earth, we need to return to the Moon before we go to Mars.
The Moon helps us to learn how to live and work on another planetary body while being only three days away from home – instead of several months. The Moon also holds enormous potential for testing new technologies, like prospecting for water ice and turning it into drinking water, oxygen and rocket fuel. Plus, there’s so much science to be done!
The Moon can help us understand the early history of the solar system, how planets migrated to their current formation and much more. Understanding how the Earth-Moon system formed is difficult because those ancient rocks no longer exist here on Earth. They have been recycled by plate tectonics, but the Moon still has rocks that date back to the time of its formation! It’s like traveling to a cosmic time machine!
Join us on this exciting journey as we expand humanity’s presence beyond Earth.
Learn more about the Moon and all the surprises it may hold: https://moon.nasa.gov
Find out more about today’s announcement HERE.
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Weather permitting, you can observe the Moon most nights, unless it's a new moon, when the lighted side of the Moon faces away from Earth. The Moon is by far the brightest object in the night sky and there's plenty to see. But this week is special...
...October 28 is International Observe the Moon Night (also known as InOMN).
Everyone on Earth is invited to join the celebration by hosting or attending an InOMN event and uniting on one day each year to look at and learn about the Moon together.
October's night skies are full of sights, from the first quarter Moon on InOMN to Saturn making a cameo appearance above the Moon October 23 and 24. Watch our What's Up video for details.
Hundreds of events are planned around the globe. Click the top link on this page for a handy map. You can also register your own event.
Here are some activities for enhanced Moon watching.
Download InOMN flyers and handouts, Moon maps and even some pre-made presentations. There's even a certificate to mark your participation.
Almost dead center on the Earth-facing side of the Moon is the Surveyor 6 robotic spacecraft impact side. Apollo 12 and 14 are a bit to the left. And Apollo 11 - the first steps on the moon - are to the right. This retro graphic tells the whole story.
NASA photographers have done some exceptional work capturing views of the Moon from Earth. Here are a few galleries:
You can't have a solar eclipse without the Moon.
The 2016 "Supermoon" was pretty spectacular.
The Moon gets eclipsed, too.
That IS a Moon - AND the International Space Station.
The Moon is always a great photo subject.
Some spooky shots of the 2014 "Supermoon."
And 2013.
Tips from a NASA pro for photographing the Moon.
Twelve human beings walked on the face of the Moon. Here are some of the best shots from the Apollo program.
Our Lunar Reconnaissance Orbiter is up there right now, mapping the moon and capturing some spectacular high-resolution shots.
Make our Moon portal your base for further lunar exploration.
Check out the full version of ‘Ten Things to Know This Week’ HERE.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
What made you want to become a pilot for NASA? What’s your favorite part of this job?
And luckily, our Hubble Space Telescope is there to be our window to the unimaginable! Hubble recently ran into an issue with its payload computer which controls and coordinates science instruments onboard the spacecraft. On July 16, teams successfully switched to backup hardware to compensate for the problem! A day later, the telescope resumed normal science operations. To celebrate, we’re taking you back to 2016 when our dear Hubble captured perhaps one of the most intriguing objects in our Milky Way galaxy: a massive star trapped inside a bubble! The star inside this Bubble Nebula burns a million times brighter than our Sun and produces powerful gaseous outflows that howl at more than four million miles per hour. Based on the rate the star is expending energy, scientists estimate in 10 to 20 million years it will explode as a supernova. And the bubble will succumb to a common fate: It’ll pop.
Did you know our Milky Way galaxy is blowing bubbles? Two of them, each 25,000 light-years tall! They extend above and below the disk of the galaxy, like the two halves of an hourglass. We can’t see them with our own eyes because they’re only apparent in gamma-ray light, the highest-energy light in the universe.
We didn’t even know these humongous structures were smack in the middle of our galaxy until 2010. Scientists found them when they analyzed the first two years of data from NASA’s Fermi Gamma-ray Space Telescope. They dubbed them the “Fermi bubbles” and found that in addition to being really big and spread out, they seem to have well-defined edges. The bubbles’ shape and the light they give off led scientists to think they were created by a rapid release of energy. But by what? And when?
One possible explanation is that they could be leftovers from the last big meal eaten by the supermassive black hole at the center of our galaxy. This monster is more than 4 million times the mass of our own Sun. Scientists think it may have slurped up a big cloud of hydrogen between 6 and 9 million years ago and then burped jets of hot gas that we see in gamma rays and X-rays.
Another possible explanation is that the bubbles could be the remains of star formation. There are massive clusters of stars at very the center of the Milky Way — sometimes the stars are so closely packed they’re a million times more dense than in the outer suburb of the galaxy where we live. If there was a burst of star formation in this area a few million years ago, it could have created the surge of gas needed to in turn create the Fermi bubbles.
It took us until 2010 to see these Fermi bubbles because the sky is filled with a fog of other gamma rays that can obscure our view. This fog is created when particles moving near light speed bump into gas, dust, and light in the Milky Way. These collisions produce gamma rays, and scientists had to factor out the fog to unveil the bubbles.
Scientists continue to study the possible causes of these massive bubbles using the 10 years of data Fermi has collected so far. Fermi has also made many other exciting discoveries — like the the collision of superdense neutron stars and the nature of space-time. Learn more about Fermi and how we’ve been celebrating its first decade in space.
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Coming in to a post office near you: new “Views of Our Planets: Forever stamps featuring iconic images of the planets in our solar system, including the well-known “Blue Marble” photo of Earth.
New “Pluto Explored” Forever stamps commemorating the July 2015 flyby of Pluto by our New Horizons spacecraft are also being issued for online purchase.
The May 31 first-day-of-issue dedication ceremony for the Pluto and planetary stamps will be in New York City at the World Stamp Show. This international gathering of stamp collectors occurs only once each decade in the United States, and – with more than 250,000 visitors expected to attend – is the largest stamp show in the world.
The Pluto stamps are of special significance to the New Horizons team, which placed a 20-cent 1991 “Pluto: Not Yet Explored” stamp on board the spacecraft. On July 14, 2015, New Horizons carried the stamp on its history-making journey to Pluto and beyond, as jubilant members of the mission team celebrated with a large print, striking the words “not yet.”
The above pane of 16 Forever stamps, the Postal Service showcases some of the more visually compelling historic, full-disk images of the planets obtained during the last half-centruy of our space exploration. Eight new colorful Forever stamps – each shown twice – feature Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune.
This isn’t the first time that space has been featured on postal stamps. In the past, many different space images and missions have been highlighted on the tiny pieces of paper you stick on the corner of your mail.
Nebulae
Stamps depicting multiple nebulae seen by the Hubble Space Telescope were released in 2000.
Pioneer 10
Launched in 1972, Pioneer 10 was the first spacecraft to travel through the asteroid belt and obtain close-ups of Jupiter
U.S. Launches Satellites
This stamp, released in 1999, depicts the post World War II race in space exploration.
Alan Shepard: First American in Space
This stamp, released in 2011, featured Alan Shepard, the first American in space. Flying on the Mercury spacecraft, Shepard launched, flew 116 miles high and came back to Earth. His flight lasted about 15 and a half minutes.
MESSENGER Mission
MESSENGER, launching in 2004, was the first spacecraft to orbit Mercury. This stamp, released in 2011, highlighted this mission and its importance. Understanding Mercury and how it formed is critical to better understanding the conditions on and evolution of the inner planets.
The new “Views of our Planets” stamps will be widely available across the U.S. at post offices and for online purchase beginning May 31. The Pluto – Explored Forever stamps will only be sold online or by calling 800-782-6724.
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From space, we can see a swirling brown mass making its way across the Atlantic – dust from the Sahara Desert – the largest hot desert in the world. It’s a normal phenomenon. Every year, winds carry millions of tons of dust from North Africa, usually during spring and summer in the Northern Hemisphere.
June 2020 has seen a massive plume of dust crossing the ocean. It’s so large it’s visible from one million miles away in space.
Dust clouds this large can affect air quality in regions where the dust arrives. The particles can also scatter the Sun’s light, making sunrises and sunsets more vibrant.
Dust particles in the air are also known as aerosols. We can measure aerosols, including dust, sea salt and smoke, from satellites and also use computer models to study how they move with the wind.
Following the transport of dust from space shows us how one of the driest places on Earth plays a role in fertilizing the Amazon rainforest. There are minerals in Saharan dust, like phosphorous, that exist in commercial fertilizers, helping seed the rainforest.
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Labor Day reflections: the Nancy Grace Roman Space Telescope’s primary mirror reflects an American flag hanging overhead. The mirror, which will collect and focus light from cosmic objects near and far, has been completed. Renamed after our first chief astronomer and "Mother of Hubble," the Roman Space Telescope will capture stunning space vistas with a field of view 100 times greater than Hubble Space Telescope images. The spacecraft will study the universe using infrared light, which human eyes can’t detect without assistance. This Labor Day, we thank all the people who work to advance the future for humanity. Credit: L3Harris Technologies Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Orbital ATK will launch its Cygnus cargo spacecraft to the International Space Station on November 11, 2017 from Wallops Flight Facility in Virginia. It will be packed with cargo and scientific experiments for the six humans currently living and working on the orbiting laboratory.
The cargo spacecraft is named the S.S. Gene Cernan after former NASA astronaut Eugene Cernan, who is the last man to have walked on the moon.
What’s Microgravity Got to do with Bacterial Antibiotics?
Antibiotic resistance could pose a danger to astronauts, especially since microgravity has been shown to weaken human immune response. E. coli AntiMicrobial Satellite (EcAMSat) will study microgravity’s effect on bacterial antibiotic resistance.
Results from this experiment could help us determine appropriate antibiotic dosages to protect astronaut health during long-duration human spaceflight and help us understand how antibiotic effectiveness may change as a function of stress on Earth.
Laser Beams…Not on Sharks…But on a CubeSat
Traditional laser communication systems use transmitters that are far too large for small spacecraft. The Optical Communication Sensor Demonstration (OCSD) tests the functionality of laser-based communications using CubeSats that provide a compact version of the technology.
Results from OCSD could lead to improved GPS and other satellite networks on Earth and a better understanding of laser communication between small satellites in low-Earth orbit.
This Hybrid Solar Antenna Could Make Space Communication Even Better
As space exploration increases, so will the need for improved power and communication technologies. The Integrated Solar Array and Reflectarray Antenna (ISARA), a hybrid power and communication solar antenna that can send and receive messages, tests the use of this technology in CubeSat-based environmental monitoring.
ISARA may provide a solution for sending and receiving information to and from faraway destinations, both on Earth and in space.
More Plants in Space!
Ready for a mouthful…The Biological Nitrogen Fixation in Microgravity via Rhizobium-Legume Symbiosis…aka the Biological Nitrogen Fixation experiment, will examine how low-gravity conditions affect the nitrogen fixation process of the Microclover legume (a plant in the pea family). Nitrogen fixation is a process where nitrogen in the atmosphere is converted into ammonia. This crucial element of any ecosystem is also a natural fertilizer that is necessary for most types of plant growth.
This experiment could tell us about the space viability of the legume’s ability to use and recycle nutrients and give researchers a better understanding of this plant’s potential uses on Earth.
What Happens When Mealworms Live in Space?
Mealworms are high in nutrients and one of the most popular sources of alternative protein in developing countries. The Effects of Microgravity on the Life Cycle of Tenebrio Molitor (Tenebrio Molitor) investigation studies how the microgravity environment affects the mealworm life cycle.
In addition to alternative protein research, this investigation will provide information about animal growth under unique conditions.
Mustard Seeds in Microgravity
The Life Cycle of Arabidopsis thaliana in Microgravity experiment studies the formation and functionality of the Arabidopsis thaliana, a mustard plant with a genome that is fully mapped, in microgravity conditions.
The results from this investigation could contribute to an understanding of plant and crop growth in space.
Follow @ISS_Research on Twitter for more information about the science happening on space station.
Watch the launch live HERE on Nov. 11, liftoff is scheduled for 7:37 a.m. EDT!
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What led you to this job? (what’s your degree in/what are your passions)
NASA’s Space Launch System (SLS) rocket is on the launch pad at NASA’s Kennedy Space Center in Florida and in final preparations for the Artemis I mission to the Moon. Now that our Moon rocket is almost ready for its debut flight, we wanted to take a look back at some of the most liked photographs of our SLS rocket coming together over the years.
We asked NASA photographers to share their favorite photos of the SLS rocket for Artemis I at different phases of testing, manufacturing, and assembly. Here are their stories behind the photos:
“On this day in March 2018, crews at NASA’s Marshall Space Flight Center in Huntsville, Alabama, transported the intertank structural test article off NASA’s Pegasus barge to the Load Test Annex test facility for qualification testing.” —Emmett Given, photographer, NASA’s Marshall Space Flight Center
“This is the liquid oxygen tank structural test article as it was moved from the Pegasus barge to the West Test Area at our Marshall Space Flight Center on July 9, 2019. The tank, which is structurally identical to its flight version, was subsequently placed in the test stand for structural testing several days later. I remember it being a blazing hot day!” —Fred Deaton, photographer, NASA’s Marshall Space Flight Center
“The large components of the SLS rocket’s core stage can make you forget that there are many hands-on tasks required to assemble a rocket, too. During the mating of the liquid hydrogen tank to the forward section of the rocket’s 212-foot-tall core stage in May 2019, technicians fastened 360 bolts to the circumference of the rocket. Images like this remind me of all the small parts that have to be installed with care, expertise, and precision to create one huge Moon rocket. Getting in close to capture the teammates that work tirelessly to make Artemis a success is one of the best parts of my job.” —Eric Bordelon, photographer, NASA’s Michoud Assembly Facility
“An incredible amount of precision goes into building a rocket, including making sure that each of our SLS rocket’s four RS-25 engines is aligned and integrated into the core stage correctly. In this image from October 2019, I attempted to illustrate the teamwork and communication happening as technicians at NASA’s Michoud Assembly Facility in New Orleans do their part to help land the first woman and the first person of color on the Moon through the Artemis missions. It’s rare to see the inside of a rocket – not as much for the NASA and Boeing engineers who manufacture and assemble a rocket stage!” —Jared Lyons, photographer, NASA’s Michoud Assembly Facility
“When the fully assembled and completed core stage left the Michoud factory in January 2020, employees took a “family photo” to mark the moment. Crews transported the flight hardware to NASA’s Pegasus barge on Jan. 8 in preparation for the core stage Green Run test series at NASA’s Stennis Space Center near Bay St. Louis, Mississippi. When I look at this photo, I am reminded of all of the hard work and countless hours the Michoud team put forth to build this next-generation Moon rocket. I am honored to be part of this family and to photograph historic moments like this for the Artemis program.” —Steven Seipel, MAF multimedia team lead, NASA’s Michoud Assembly Facility
“This photo shows workers at Stennis prepare to lift the SLS core stage into the B-2 Test Stand for the SLS Green Run test series in the early morning hours of Jan. 22, 2020. I started shooting the lift operation around midnight. During a break in the action at about 5:30 a.m., I was driving my government vehicle to the SSC gas station to fuel up, when I saw the first light breaking in the East and knew it was going to be a nice sunrise. I turned around and hurried back to the test stand, sweating that I might run out of gas. Luckily, I didn’t run out and was lucky enough to catch a beautiful Mississippi sunrise in the background, too.” —Danny Nowlin, photographer, NASA’s Stennis Space Center
“I like the symmetry in the video as it pushes toward the launch vehicle stage adapter. Teams at NASA’s Marshall Space Flight Center in Huntsville, Alabama, loaded the cone-shaped piece of flight hardware onto our Pegasus barge in July 2020 for delivery to NASA’s Kennedy Space Center in Florida. The one-point perspective puts the launch vehicle stage adapter at the center of attention, but, if you pay attention to the edges, you can see people working. It gives a sense of scale. This was the first time I got to walk around Pegasus and meet the crew that transport the deep space rocket hardware, too.” —Sam Lott, videographer, SLS Program at Marshall Space Flight Center
“This was my first time photographing a test at our Stennis Space Center, and I wasn't sure what to expect. I have photographed big events like professional football games, but I wasn't prepared for the awesome power unleashed by the Space Launch System’s core stage and four RS-25 engines during the Green Run hot fire test. Watching the sound wave ripple across the tall grass toward us, feeling the shock wave of ignition throughout my whole body, seeing the smoke curling up into the blue sky with rainbows hanging from the plume; all of it was as unforgettable as watching a football player hoist a trophy into the air.” —Michael DeMocker, photographer, NASA’s Michoud Assembly Facility
“When our SLS Moon rocket launches the agency’s Artemis I mission to the Moon, 10 CubeSats, or small satellites, are hitching a ride inside the rocket’s Orion stage adapter (OSA). BioSentinel is one of those CubeSats. BioSentinel’s microfluidics card, designed at NASA’s Ames Research Center in California’s Silicon Valley, will be used to study the impact of interplanetary space radiation on yeast. To me, this photo is a great combination of the scientific importance of Artemis I and the human touch of more than 100 engineers and scientists who have dedicated themselves to the mission over the years.” —Dominic Hart, photographer, NASA’s Ames Research Center
“I was in the employee viewing area at Kennedy when the integrated SLS rocket and Orion spacecraft was rolled out to the launchpad for its wet dress rehearsal in March 2022. I really like this photo because the sun is shining on Artemis I like a spotlight. The giant doors of the Vehicle Assembly Building are the red curtain that opened up the stage -- and the spotlight is striking the SLS because it’s the star of the show making its way to the launchpad. I remember thinking how cool that NASA Worm logo looked as well, so I wanted to capture that. It was so big that I had to turn my camera sideways because the lens I had wasn’t big enough to capture the whole thing.” —Brandon Hancock, videographer, SLS Program at NASA’s Marshall Space Flight Center
“I made this image while SLS and Orion atop the mobile launcher were nearing the end of their four-mile trek to the pad on crawler-transporter 2 ahead of launch. Small groups of employees were filtering in and out of the parking lot by the pad gate to take in the sight of the rocket’s arrival. The “We Are Going!” banner affixed to the gate in the foreground bears the handwritten names of agency employees and contractors who have worked to get the rocket and spacecraft ready for the Artemis I flight test. As we enter the final days before launch, I am proud to have made my small contribution to documenting the historic rollout for this launch to the Moon.” —Joel Kowsky, photographer, NASA Headquarters
NASA photographers will be on the ground covering the Artemis I launch. As they do, we’ll continue to share their photos on our official NASA channels.
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What would happen if the crew of the Starship Enterprise handed over the controls to our scientists and engineers? It turns out many are avid Star Trek fans with lengthy itineraries in mind.
1. Vulcan
What is perhaps the most famous Star Trek planet was placed by creator Gene Roddenberry in a real star system: 40 Eridani. This trinary system of three dwarf stars, about 16 light-years from Earth, could play host to exoplanets; none have been detected there so far. The most massive is 40 Eridani A, chosen as Vulcan’s sun.
2. Andoria
An icy “M-class” (Star Trek's term for “Earth-like”) moon of a much larger planet—a gas giant—that is home to soft-spoken humanoids with blue skin, white hair and stylish antennae. In our solar system, gas giants play host to icy moons, such as Jupiter’s Europa or Saturn’s Enceladus, that possess subsurface oceans locked inside shells of ice. Our missions are searching for lifeforms that might exist in these cold, dark habitats.
3. Risa
Another Trek M-class planet known for its engineered tropical climate and its welcoming humanoid population. The planet is said to orbit a binary, or double, star system—in Star Trek fan lore, Epsilon Ceti, a real star system some 79 light-years from Earth. The first discovery of a planet around a binary was Kepler-16b, which is cold, gaseous and Saturn-sized.
4. “Shore Leave” planet, Omicron Delta region
This is another amusement park of a planet, where outlandish characters are manufactured in underground factories straight from the crew members’ imaginations. In real life, astronauts aboard the International Space Station print out plastic tools and containers with their own 3-D printer.
5. Nibiru
“Star Trek: Into Darkness” finds Captain Kirk and Dr. McCoy fleeing from chalk-skinned aliens through a red jungle. Red or even black vegetation could exist on real planets that orbit cooler, redder stars, an adaptation meant to gather as much light for photosynthesis as possible. An example may be Kepler-186f, a planet only 10 percent larger than Earth in diameter. At high noon, the surface of this planet would look something like dusk on Earth.
6. Wolf 359
A star best known in the Star Trek universe as the site of a fierce battle in which a multitude of “Star Trek: Next Generation” ships are defeated by the Borg. But Wolf 359 is a real star, one of the closest to Earth at a distance of 7.8 light-years. Wolf 359 is also a likely observational target for the Kepler space telescope in the upcoming Campaign 14 of its “K2” mission.
7. Eminiar VII/Vendikar
These two planets are neighbors, sharing a star system. So, of course, they’ve been at war for centuries. While we have no signs of interplanetary war, multiple rocky worlds have been discovered orbiting single stars. A cool dwarf star called TRAPPIST-1 is orbited by three Earth-size planets; two have a chance of being the right temperature for liquid water, with possible Earth-like atmospheres.
8. Remus
The planets Romulus and Remus are home to the Romulan Empire (ancient Rome, anyone?), although Remus seemed to have gotten the raw end of the deal. Remus is tidally locked, one face always turned to its star. Tidally locked worlds might well be a real thing, with many possible candidates discovered with our Kepler space telescope. The habitable portion of the surface of such planets might be confined to a band between the day and night sides called the “terminator zone”—a.k.a. the twilight zone.
9. Janus VI
A rocky world lacking an atmosphere, perhaps similar to Mars. While humans must maintain an artificial underground environment to survive, the innards of the planet are a comfortable home to an alien species known as the “Horta.” Their rock-like biochemistry is based on silicon, rather than carbon, inspiring us to imagine the many forms life might take in the universe.
10. Earth
In the Star Trek universe, Earth is home to Starfleet Headquarters; the real Earth is, at least so far, the only life-bearing world we know. No true Earth analogs have been discovered among the real exoplanets detected so far. But a new generation of space telescopes, designed to capture direct images of exoplanets in Earth’s size range, might one day reveal an alternative “pale blue dot.”
Learn more about exoplanets at: exoplanets.nasa.gov
Link to full article: https://exoplanets.nasa.gov/news/1378/top-10-star-trek-destinations-chosen-by-nasa-scientists/
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sorry, i don't know much about earth science (though it sounds very intriguing), but - what exactly is it that you do? does it take a lot of time? is it fun but challenging? was it hard to get your job? have you always wanted to work with earth science?
An eclipse occurs when the Moon temporarily blocks the light from the Sun. Within the narrow, 60- to 70-mile-wide band stretching from Oregon to South Carolina called the path of totality, the Moon completely blocked out the Sun’s face; elsewhere in North America, the Moon covered only a part of the star, leaving a crescent-shaped Sun visible in the sky.
During this exciting event, we were collecting your images and reactions online.
This composite image, made from 4 frames, shows the International Space Station, with a crew of six onboard, as it transits the Sun at roughly five miles per second during a partial solar eclipse from, Northern Cascades National Park in Washington. Onboard as part of Expedition 52 are: NASA astronauts Peggy Whitson, Jack Fischer, and Randy Bresnik; Russian cosmonauts Fyodor Yurchikhin and Sergey Ryazanskiy; and ESA (European Space Agency) astronaut Paolo Nespoli.
Credit: NASA/Bill Ingalls
The Bailey's Beads effect is seen as the moon makes its final move over the sun during the total solar eclipse on Monday, August 21, 2017 above Madras, Oregon.
Credit: NASA/Aubrey Gemignani
This image from one of our Twitter followers shows the eclipse through tree leaves as crescent shaped shadows from Seattle, WA.
Credit: Logan Johnson
“The eclipse in the palm of my hand”. The eclipse is seen here through an indirect method, known as a pinhole projector, by one of our followers on social media from Arlington, TX.
Credit: Mark Schnyder
Through the lens on a pair of solar filter glasses, a social media follower captures the partial eclipse from Norridgewock, ME.
Credit: Mikayla Chase
While most of us watched the eclipse from Earth, six humans had the opportunity to view the event from 250 miles above on the International Space Station. European Space Agency (ESA) astronaut Paolo Nespoli captured this image of the Moon’s shadow crossing America.
Credit: Paolo Nespoli
This composite image shows the progression of a partial solar eclipse over Ross Lake, in Northern Cascades National Park, Washington. The beautiful series of the partially eclipsed sun shows the full spectrum of the event.
Credit: NASA/Bill Ingalls
In this video captured at 1,500 frames per second with a high-speed camera, the International Space Station, with a crew of six onboard, is seen in silhouette as it transits the sun at roughly five miles per second during a partial solar eclipse, Monday, Aug. 21, 2017 near Banner, Wyoming.
Credit: NASA/Joel Kowsky
To see more images from our NASA photographers, visit: https://www.flickr.com/photos/nasahqphoto/albums/72157685363271303
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Only a few humans ever get to experience the awe-inspiring vantage point provided by the space station, but a new virtual reality (VR) experience, Space Explorers: The ISS Experience (ISS Experience), attempts to bring this perspective back to Earth for the rest of us.
Partnering with the ISS National Lab and Time, a team from Felix and Paul Studios launched a high quality 360 degree camera to space to help tell the story of science and life aboard the orbiting laboratory.
The project, currently in the process of being filmed by the station astronauts themselves, serves as an outreach project as well a technology demonstration, testing the limits of filming in the harsh environment of space.
The camera flew to the station on 16th SpaceX commercial resupply services mission in December 2018 along with a number of other scientific experiments.
Since then, the team has recorded many moments, including the SPHERES robots flying around the station (see below) , the growing and harvesting of vegetables, jam session among the astronauts, crew meals and the arrival of new astronauts.
So far, the footage coming back seems to be achieving the goal of immersing audiences in science and life aboard the space station. NASA astronaut Sunita Williams got the chance to watch some of the initial footage and says it was like I was back on the station.
While most of the filming has been completed, the biggest technical challenge is yet to come: capturing a spacewalk in virtual reality. The team expects to launch a new camera for spacewalk filming and begin production of spacewalk filming in 2020.
Learn more about ISS Experience here.
For daily updates, follow @ISS_Research on Twitter, Space Station Research and Technology News or our Facebook. Follow the ISS National Lab for information on its sponsored investigations. For opportunities to see the space station pass over your town, check out Spot the Station.
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Currently, six humans are living and working on the International Space Station, which orbits 250 miles above our planet at 17,500mph. Below you will find a real journal entry, written in space, by NASA astronaut Scott Tingle.
To read more entires from this series, visit our Space Blogs on Tumblr.
Wow, time has gone by extremely fast. The mid-deployment phase will be short-lived for me this time, as the new crew (Drew Feustel, Ricky Arnold, and Oleg Artemyev) will arrive on March 23rd, and then we have at least one spacewalk on the 29th, followed by a planned SpaceX Dragon cargo craft arrival on the 4th of April. It’s a little strange being up here with only two other crewmates. We are still very busy, but the overall work effort is half of what it was just a week ago. My crewmate, Nemo (Norishige Kanai), and I are trying to use the time to prepare for the upcoming very busy schedule, and we have been having some great success getting a ton of details taken care of.
Yesterday I had a funny event, though. I was controlling a robot named “Justin” who was located in Munich. The research and demonstration events were so interesting and fun that I offered them my lunch hour to do an additional protocol and have a longer debrief session. The ground team responded happily and accepted the offer – any extra time with crew onboard the International Space Station (ISS) is valuable to our programs. Halfway through the event, the team needed a few minutes to shut down and restart the robot, and I surmised that since I was skipping my break, this would be a good time to use the toilet. And I did, use the toilet. And literally 3 minutes later I returned, waited another 2 minutes for the robot systems to connect, and we began another great session controlling Justin from ISS with no loss to science.
Later that same day, I was approached by the ground team in Houston (not the test team I was working with in Munich) and queried if something was wrong, and why did I have to take a toilet break while we were executing valuable science? They were concerned that I might have a medical issue, as taking a break in the middle of some very valuable science is not normal for us to do while on ISS. It’s nice to know that we have literally hundreds of highly-trained professionals looking out for us.
Find more ‘Captain’s Log’ entries HERE.
Follow NASA astronaut Scott Tingle on Instagram and Twitter.
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When we talk about the enormity of the cosmos, it’s easy to toss out big numbers – but far harder to wrap our minds around just how large, how far and how numerous celestial bodies like exoplanets – planets beyond our solar system – really are.
So. How big is our Milky Way Galaxy?
We use light-time to measure the vast distances of space.
It’s the distance that light travels in a specific period of time. Also: LIGHT IS FAST, nothing travels faster than light.
How far can light travel in one second? 186,000 miles. It might look even faster in metric: 300,000 kilometers in one second. See? FAST.
How far can light travel in one minute? 11,160,000 miles. We’re moving now! Light could go around the Earth a bit more than 448 times in one minute.
Speaking of Earth, how long does it take light from the Sun to reach our planet? 8.3 minutes. (It takes 43.2 minutes for sunlight to reach Jupiter, about 484 million miles away.) Light is fast, but the distances are VAST.
In an hour, light can travel 671 million miles. We’re still light-years from the nearest exoplanet, by the way. Proxima Centauri b is 4.2 light-years away. So… how far is a light-year? 5.8 TRILLION MILES.
A trip at light speed to the very edge of our solar system – the farthest reaches of the Oort Cloud, a collection of dormant comets way, WAY out there – would take about 1.87 years.
Our galaxy contains 100 to 400 billion stars and is about 100,000 light-years across!
One of the most distant exoplanets known to us in the Milky Way is Kepler-443b. Traveling at light speed, it would take 3,000 years to get there. Or 28 billion years, going 60 mph. So, you know, far.
SPACE IS BIG.
Read more here: go.nasa.gov/2FTyhgH
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