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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When the sun goes down, the lights on Earth shine bright. A new look using our satellite data captures the lights coming from our neighborhoods, vehicles, buildings, factories, fishing vessels and other human activity brightening the night.
Our scientists have just released the first new global map of Earth at night since 2012. This nighttime view of our home planet, dubbed the Black Marble, provides researchers with a unique perspective of human activities around the globe.
By studying Earth at night, researchers can investigate how and why cities expand, monitor light intensity to estimate energy use and economic activity, and aid in disaster response in near-real time.
The data on Earth at night comes from the Visible Infrared Imaging Radiometer Suite (VIIRS) instrument on the Suomi National Polar-orbiting Partnership satellite, jointly managed by NASA and the National Oceanic and Atmospheric Administration (NOAA).
VIIRS captures visible and infrared light, allowing researchers to glimpse the Earth as it looks to astronauts peering out of the International Space Station. The new map is a composite of data collected in 2016, and it took several months of processing to filter out clouds, moonlight, airglow, and other interfering features to create the global image. In the coming months our scientists will release daily nighttime lights data at even finer resolutions for the first time.
The East Coast sparkles with population hubs, suburbs circling cities and major roadways. The I-95 corridor includes the most densely populated region of the United States – the stretch from Washington, DC to Boston.
To get images like these from the satellite data, our scientists had to filter out moonlight, aerosols and other sources of extraneous light – the goal is to eventually be able to detect the lights from a single building or fishing boat.
Daytime satellite images, like this one from Landsat 8, can show us the forests, deserts, mountains, waterways and built-up cities. Add a nighttime view, and scientists can study when and how people are using these limited resources – like the lights tracing the Nile River leading to the metropolis of Cairo, Egypt.
Lights aren’t confined to land. With the global nighttime view, the ocean is dotted with fishing fleets, including boats that try to attract their catch with bright lights.
What lights illuminate your neighborhood? Download a high-resolution version of the Black Marble HERE, and find out more about our new night lights data HERE.
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One year ago, on Sept. 15, 2017, NASA’s Cassini spacecraft ended its epic exploration of Saturn with a planned dive into the planet’s atmosphere--sending back new science to the last second. The spacecraft is gone, but the science continues. Here are 10 reasons why Cassini mattered...
Cassini and ESA (European Space Agency)’s Huygens probe expanded our understanding of the kinds of worlds where life might exist.
At Saturn’s largest moon, Titan, Cassini and Huygens showed us one of the most Earth-like worlds we’ve ever encountered, with weather, climate and geology that provide new ways to understand our home planet.
Cassini gave us a portal to see the physical processes that likely shaped the development of our solar system, as well as planetary systems around other stars.
The length of Cassini’s mission enabled us to observe weather and seasonal changes over nearly half of a Saturn year, improving our understanding of similar processes at Earth, and potentially those at planets around other stars.
Cassini revealed Saturn’s moons to be unique worlds with their own stories to tell.
Cassini showed us the complexity of Saturn’s rings and the dramatic processes operating within them.
Some of Cassini’s best discoveries were serendipitous. What Cassini found at Saturn prompted scientists to rethink their understanding of the solar system.
Cassini represented a staggering achievement of human and technical complexity, finding innovative ways to use the spacecraft and its instruments, and paving the way for future missions to explore our solar system.
Cassini revealed the beauty of Saturn, its rings and moons, inspiring our sense of wonder and enriching our sense of place in the cosmos.
The data returned by Cassini during its 13 years at Saturn will continue to be studied for decades, and many new discoveries are undoubtedly waiting to be revealed. To keep pace with what’s to come, we’ve created a new home for the mission--and its spectacular images--at https://solarsystem.nasa.gov/cassini.
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Our Milky Way galaxy is full of hundreds of billions of worlds just waiting to be found. In 2014, scientists using data from our planet-hunting Kepler space telescope discovered seven planets orbiting Kepler-90, a Sun-like star located 2,500 light-years away. Now, an eighth planet has been identified in this planetary system, making it tied with our own solar system in having the highest number of known planets. Here’s what you need to know:
Kepler-90i is a sizzling hot, rocky planet. It’s the smallest of eight planets in the Kepler-90 system. It orbits so close to its star that a “year” passes in just 14 days.
Average surface temperatures on Kepler-90i are estimated to hover around 800 degrees Fahrenheit, making it an unlikely place for life as we know it.
The Kepler-90 system is set up like our solar system, with the small planets located close to their star and the big planets farther away. This pattern is evidence that the system’s outer gas planets—which are about the size of Saturn and Jupiter—formed in a way similar to our own.
But the orbits are much more compact. The orbits of all eight planets could fit within the distance of Earth’s orbit around our Sun! Sounds crowded, but think of it this way: It would make for some great planet-hopping.
Most planets beyond our solar system are too far away to be imaged directly. The Kepler space telescope searches for these exoplanets—those planets orbiting stars beyond our solar system—by measuring how the brightness of a star changes when a planet transits, or crosses in front of its disk. Generally speaking, for a given star, the greater the dip in brightness, the bigger the planet!
Researchers trained a computer to learn how to identify the faint signal of transiting exoplanets in Kepler’s vast archive of deep-space data. A search for new worlds around 670 known multiple-planet systems using this machine-learning technique yielded not one, but two discoveries: Kepler-90i and Kepler-80g. The latter is part of a six-planet star system located 1,000 light-years away.
Kepler-90 is the first known star system besides our own that has eight planets, but scientists say it won’t be the last. Other planets may lurk around stars surveyed by Kepler. Next, researchers are using machine learning with sophisticated computer algorithms to search for more planets around 150,000 stars in the Kepler database.
Kepler is the most successful planet-hunting spacecraft to date, with more than 2,500 confirmed exoplanets and many more awaiting verification. Future space missions, like the Transiting Exoplanet Survey Satellite (TESS), the James Webb Space Telescope and Wide-Field Infrared Survey Telescope (WFIRST) will continue the search for new worlds and even tell us which ones might offer promising homes for extraterrestrial life.
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*All images of exoplanets are artist illustrations.
Crab Nebula in technicolor! This new composite view combines data from five different telescopes, showing the celestial object in multiple kinds of light.
The video starts with a composite image of the Crab Nebula, a supernova remnant that was assembled by combining data from five telescopes spanning nearly the entire breadth of the electromagnetic spectrum: the Very Large Array, the Spitzer Space Telescope, the Hubble Space Telescope, the XMM-Newton Observatory, and the Chandra X-ray Observatory.
It then dissolves to the red-colored radio-light view that shows how a neutron star’s fierce “wind” of charged particles from the central neutron star energized the nebula, causing it to emit the radio waves.
The yellow-colored infrared image includes the glow of dust particles absorbing ultraviolet and visible light.
The green-colored Hubble visible-light image offers a very sharp view of hot filamentary structures that permeate this nebula.
The blue-colored ultraviolet image and the purple-colored X-ray image shows the effect of an energetic cloud of electrons driven by a rapidly rotating neutron star at the center of the nebula.
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Out of all the theories and fantasies created around blackholes, which of them, in your opinion, do you think could come closest to reality?
Happy New Year! And happy supermoon! Tonight, the Moon will appear extra big and bright to welcome us into 2018 – about 6% bigger and 14% brighter than the average full Moon. And how do we know that? Well, each fall, our science visualizer Ernie Wright uses data from the Lunar Reconnaissance Orbiter (LRO) to render over a quarter of a million images of the Moon. He combines these images into an interactive visualization, Moon Phase and Libration, which depicts the Moon at every day and hour for the coming year.
Want to see what the Moon will look like on your birthday this year? Just put in the date, and even the hour (in Universal Time) you were born to see your birthday Moon.
Our Moon is quite dynamic. In addition to Moon phases, our Moon appears to get bigger and smaller throughout the year, and it wobbles! Or at least it looks that way to us on Earth. This wobbling is called libration, from the Latin for ‘balance scale’ (libra). Wright relies on LRO maps of the Moon and NASA orbit calculations to create the most accurate depiction of the 6 ways our Moon moves from our perspective.
The Moon phases we see on Earth are caused by the changing positions of the Earth and Moon relative to the Sun. The Sun always illuminates half of the Moon, but we see changing shapes as the Moon revolves around the Earth. Wright uses a software library called SPICE to calculate the position and orientation of the Moon and Earth at every moment of the year. With his visualization, you can input any day and time of the year and see what the Moon will look like!
Check out that crater detail! The Moon is not a smooth sphere. It’s covered in mountains and valleys and thanks to LRO, we know the shape of the Moon better than any other celestial body in the universe. To get the most accurate depiction possible of where the sunlight falls on the lunar surface throughout the month, Wright uses the same graphics software used by Hollywood design studios, including Pixar, and a method called ‘raytracing’ to calculate the intricate patterns of light and shadow on the Moon’s surface, and he checks the accuracy of his renders against photographs of the Moon he takes through his own telescope.
The Moon Phase and Libration visualization shows you the apparent size of the Moon. The Moon’s orbit is elliptical, instead of circular - so sometimes it is closer to the Earth and sometimes it is farther. You’ve probably heard the term “supermoon.” This describes a full Moon at or near perigee (the point when the Moon is closest to the Earth in its orbit). A supermoon can appear up to 14% bigger and brighter than a full Moon at apogee (the point when the Moon is farthest from the Earth in its orbit).
Our supermoon tonight is a full Moon very close to perigee, and will appear to be about 14% bigger than the July 27 full Moon, the smallest full Moon of 2018, occurring at apogee. Input those dates into the Moon Phase and Libration visualization to see this difference in apparent size!
Over a month, the Moon appears to nod, twist, and roll. The east-west motion, called ‘libration in longitude’, is another effect of the Moon’s elliptical orbital path. As the Moon travels around the Earth, it goes faster or slower, depending on how close it is to the Earth. When the Moon gets close to the Earth, it speeds up thanks to an additional pull from Earth’s gravity. Then it slows down, when it’s farther from the Earth. While this speed in orbital motion changes, the rotational speed of the Moon stays constant.
This means that when the Moon moves faster around the Earth, the Moon itself doesn’t rotate quite enough to keep the same exact side facing us and we get to see a little more of the eastern side of the Moon. When the Moon moves more slowly around the Earth, its rotation gets a little ahead, and we see a bit more of its western side.
The Moon also appears to nod, as if it were saying “yes,” a motion called ‘libration in latitude’. This is caused by the 5 degree tilt of the Moon’s orbit around the Earth. Sometimes the Moon is above the Earth’s northern hemisphere and sometimes it’s below the Earth’s southern hemisphere, and this lets us occasionally see slightly more of the northern or southern hemispheres of the Moon!
Finally, the Moon appears to tilt back and forth like a metronome. The tilt of the Moon’s orbit contributes to this, but it’s mostly because of the 23.5 degree tilt of our own observing platform, the Earth. Imagine standing sideways on a ramp. Look left, and the ramp slopes up. Look right and the ramp slopes down.
Now look in front of you. The horizon will look higher on the right, lower on the left (try this by tilting your head left). But if you turn around, the horizon appears to tilt the opposite way (tilt your head to the right). The tilted platform of the Earth works the same way as we watch the Moon. Every two weeks we have to look in the opposite direction to see the Moon, and the ground beneath our feet is then tilted the opposite way as well.
So put this all together, and you get this:
Beautiful isn’t it? See if you can notice these phenomena when you observe the Moon. And keep coming back all year to check on the Moon’s changing appearance and help plan your observing sessions.
Follow @NASAMoon on Twitter to keep up with the latest lunar updates.
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Did you have a favorite astronaut as a kid? If not, who were your inspirations? :)
Of course Mae Jemison was an inspiration, but I didn’t have a favorite. Because how do you pick out of such a great group?
In September 2023, students at HBCUs participated in a hackathon at the National HBCU Week Conference, where they used NASA’s technologies to create solutions to problems that affect Black communities. The winning team, Team Airtek, proposed a nano-sensor array for medical diagnoses that would give students on HBCU campuses a non-invasive, non-intensive way to test themselves for precursors for diseases and illnesses like diabetes and COVID.
The hackathon they participated in is a modified version of the full NASA Minority University Research and Education Project Innovation and Tech Transfer Idea Competition (MITTIC) that takes place each fall and spring semester at NASA’s Johnson Space Center in Houston.
No matter what you’re studying, you can join the MITTIC competition and come up with new and innovative tech to help your community and the world.
MITTIC could be the beginning of your career pathway: Teams can go on exclusive NASA tours and network with industry experts. Show off your entrepreneurial skills and your team could earn money—and bragging rights.
Don’t wait too long to apply or to share with someone who should apply! The deadline for proposals is Oct. 16, 2023. Apply here: https://microgravityuniversity.jsc.nasa.gov/nasamittic.
Here are a few things you should know about our solar system this week:
1. Gearing Up for a Grand Finale
There’s just a year left until the Cassini mission begins its Grand Finale – the final phase of its mission, during which the spacecraft will dive repeatedly between the planet and the rings. To get ready, the Cassini team has launched an enhanced, mobile device-friendly version of the mission website. The site includes information about Cassini, Saturn, the moons and the rings – but it also tells the human stories behind one of the most ambitions expeditions of all time.
2.Caught in Transit
On Monday, May 9, the planet Mercury will cross directly in front of the sun, an event that hasn’t occurred since 2006 and won’t happen again until 2019. Find out how to watch HERE.
3. A Moon for Makemake
Our Hubble Space Telescope has spotted a small, dark moon orbiting Makemake (pronounced “MAH-kay MAH-kay). Make make is the second brightest icy dwarf planet – after Pluto – in the faraway Kuiper Belt.
4. The Age of the Aquarids
The Eta Aquarid meteor shower is the first of two showers that occur each year as a result of Earth passing through dust released by Halley’s Comet. This year, it should peak on the night of May 5/6. Get tips for watching HERE.
5. The Southern Lights of Saturn
On May 4, Cassini will reach periapse, the closest point to Saturn in the spacecraft’s orbit. At about this time, Cassini’s cameras will monitor Saturn’s south polar aurorae, and also image the bright limb of the planet to better understand its upper haze layers.
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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Sustainable Aviation Ambassadors Alex Kehler, Bianca Legeza-Narvaez, Evan Gotchel, and Janki Patel pose in front of the NASA Pavilion at EAA AirVenture Oshkosh.
It’s that time of year again–EAA AirVenture Oshkosh is underway!
Boasting more than 650,000 visitors annually, EAA AirVenture Oshkosh, or “Oshkosh” for short, is an airshow and fly-in held by the Experimental Aircraft Association (EAA). Each year, flight enthusiasts and professionals from around the world converge on Oshkosh, Wisconsin, to engage with industry-leading organizations and businesses and celebrate past, present, and future innovation in aviation.
This year, four NASA interns with the Electrified Powertrain Flight Demonstration (EPFD) project count themselves among those 650,000+ visitors, having the unique opportunity to get firsthand experience with all things aerospace at Oshkosh.
Alex Kehler, Bianca Legeza-Narvaez, Evan Gotchel, and Janki Patel are Sustainable Aviation Ambassadors supporting the EPFD project, which conducts tests of hybrid electric aircraft that use electric aircraft propulsion technologies to enable a new generation of electric-powered aircraft. The focus of Alex, Bianca, Evan, and Janki’s internships cover everything from strategic communications to engineering, and they typically do their work using a laptop. But at Oshkosh, they have a special, more hands-on task: data collection.
“At Oshkosh, I am doing some data collection to better estimate how we can be prepared in the future,” said Janki, an Aerospace Engineering major from the University of Michigan. “Coming to Oshkosh has been an amazing experience… I can walk around and see people passionate about the work they do.”
The NASA Pavilion at EAA AirVenture Oshkosh is full of interactive exhibits and activities for visitors to engage with. NASA Interns Alex, Bianca, Evan, and Janki are collecting data in the pavilion to help improve future exhibits at Oshkosh.
In addition to gathering data to help inform future NASA exhibits and activities at Oshkosh, the interns also have the opportunity to engage with visitors and share their passion for aviation with other aero enthusiasts. For Evan, who is receiving his Master's in Aerospace Engineering from the Georgia Institute of Technology, “being able to be here and talk with people who are both young and old who are interested in what the future of flight could be has been so incredible.”
Alex, Evan, Bianca, and Janki pose in front of NASA’s Super Guppy, a specialized aircraft used to transport oversized cargo.
At Oshkosh, one memory in particular stands out for Alex, Bianca, Evan, and Janki: seeing NASA’s famous Super Guppy in person. With a unique hinged nose and a cargo area that's 25 feet in diameter and 111 feet long, the Super Guppy can carry oversized cargo that is impossible to transport with other cargo aircraft.
“We had a very lucky experience… We were able to not only see the Super Guppy, we got to get up close when it landed,” said Bianca, who is receiving her Master's in Business Administration with a specialization in Strategic Communications from Bowling Green State University. “From a learning experience, it gave me a way better basis on cargo aircraft and how they operate.”
For Alex, who is receiving his Master's in Aeronautical Engineering from the Georgia Institute of Technology, it was exciting to see the Super Guppy’s older technology integrated with newer technologies up close. “There have been a lot of good memories, but I think the best one was the Super Guppy. It was cool to see this combination of 60’s and 70’s technology with this upgraded plane.”
Evan and Janki pose for a photo while walking around EAA AirVenture Oshkosh.
With Oshkosh coming to a close this Sunday, July 30, Alex, Bianca, Evan, and Janki also reflected on advice they have for future NASA interns on how they can get the most out of their internship: be curious and explore, connect with people who work in the field you’re interested in, and don’t be afraid to ask questions.
Alex advises potential NASA interns to “dream big and shoot for your goals, and divide that up into steps… In the end it will work out.” For Bianca, being open and exploring is key: “take opportunities, even if it’s the complete opposite thing that you were intending to do.”
“Ask questions all the time,” said Evan. “Even outside the internship, always continue asking people about what they are knowledgeable on.” And Janki encourages future interns to “Follow your own path. Get the help of mentors, but still do your own thing.”
Visiting Oshkosh and want to see NASA science in action? Stop by the NASA Pavilion, located at Aviation Gateway Park, and see everything from interactive exhibits on sustainable aviation, Advanced Air Mobility, Quesst, and Artemis to STEM activities–and you may even meet NASA pilots, engineers, and astronauts! At Oshkosh, the sky’s the limit.
Interested in interning with NASA? Head over to NASA’s internship website to learn more about internship opportunities with NASA and find your place in (aero)space.
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