Researchers Just Found (For The First Time) An 8th Planet Orbiting A Star Far, Far Away

Researchers Just Found (For The First Time) An 8th Planet Orbiting A Star Far, Far Away

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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:

The new planet is called Kepler-90i.

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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.

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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.

Its planetary system is like a scrunched up version of our solar system.

Researchers Just Found (For The First Time) An 8th Planet Orbiting A Star Far, Far Away

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.

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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.

Kepler-90i was discovered using machine learning.

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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!

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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.

This is just the beginning of a new way of planet hunting.

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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.

In the meantime, we’ll be doing more searching with telescopes.

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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.

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7 years ago

Finalists for a Future Mission to Explore the Solar System

We’ve selected two finalists for a robotic mission that is planned to launch in the mid-2020s! Following a competitive peer review process, these two concepts were chosen from 12 proposals that were submitted in April under a New Frontiers program announcement opportunity.

What are they?

In no particular order…

CAESAR

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CAESAR, or the Comet Astrobiology Exploration Sample Return mission seeks to return a sample from 67P/Churyumov-Gerasimenko – the comet that was successfully explored by the European Space Agency’s Rosetta spacecraft – to determine its origin and history.

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This mission would acquire a sample from the nucleus of comet Churyumov-Gerasimenko and return it safely to Earth. 

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Comets are made up of materials from ancient stars, interstellar clouds and the birth of our solar system, so the CAESAR sample could reveal how these materials contributed to the early Earth, including the origins of the Earth's oceans, and of life.

Dragonfly

A drone-like rotorcraft would be sent to explore the prebiotic chemistry and habitability of dozens of sites on Saturn’s moon Titan – one of the so-called ocean worlds in our solar system.

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Unique among these Ocean Worlds, Titan has a surface rich in organic compounds and diverse environments, including those where carbon and nitrogen have interacted with water and energy.

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Dragonfly would be a dual-quadcopter lander that would take advantage of the environment on Titan to fly to multiple locations, some hundreds of miles apart, to sample materials and determine surface composition to investigate Titan's organic chemistry and habitability, monitor atmospheric and surface conditions, image landforms to investigate geological processes, and perform seismic studies.

What’s Next?

The CAESAR and Dragonfly missions will receive funding through the end of 2018 to further develop and mature the concepts. It is planned that from these, one investigation will be chosen in the spring of 2019 to continue into subsequent mission phases.

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That mission would be the fourth mission in the New Frontiers portfolio, which conducts principal investigator (PI)-led planetary science missions under a development cost cap of approximately $850 million. Its predecessors are the New Horizons mission to Pluto and a Kuiper Belt object, the Juno mission to Jupiter and OSIRIS-REx, which will rendezvous with and return a sample of the asteroid Bennu. 

Key Technologies

We also announced that two mission concepts were chosen to receive technology development funds to prepare them for future mission opportunities.

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The Enceladus Life Signatures and Habitability (ELSAH) mission concept will receive funds to enable life detection measurements by developing cost-effective techniques to limit spacecraft contamination on cost-capped missions.

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The Venus In situ Composition Investigations (VICI) mission concept will further develop the VEMCam instrument to operate under harsh conditions on Venus. The instrument uses lasers on a lander to measure the mineralogy and elemental composition of rocks on the surface of Venus.

The call for these mission concepts occurred in April and was limited to six mission themes: comet surface sample return, lunar south pole-Aitken Basin sample return, ocean worlds, Saturn probe, Trojan asteroid tour and rendezvous and Venus insitu explorer.

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2 years ago

12 Great Gifts from Astronomy

This is a season where our thoughts turn to others and many exchange gifts with friends and family. For astronomers, our universe is the gift that keeps on giving. We’ve learned so much about it, but every question we answer leads to new things we want to know. Stars, galaxies, planets, black holes … there are endless wonders to study.

In honor of this time of year, let’s count our way through some of our favorite gifts from astronomy.

Our first astronomical gift is … one planet Earth

So far, there is only one planet that we’ve found that has everything needed to support life as we know it — Earth. Even though we’ve discovered over 5,200 planets outside our solar system, none are quite like home. But the search continues with the help of missions like our Transiting Exoplanet Survey Satellite (TESS). And even you (yes, you!) can help in the search with citizen science programs like Planet Hunters TESS and Backyard Worlds.

This animated visualization depicts Earth rotating in front of a black background. Land in shades of tan and green lay among vast blue oceans, with white clouds swirling in the atmosphere. The image is watermarked with the text “Credit: NASA/Goddard Space Flight Center Scientific Visualization Studio” and “visualization.”

Our second astronomical gift is … two giant bubbles

Astronomers found out that our Milky Way galaxy is blowing bubbles — two of them! Each bubble is about 25,000 light-years tall and glows in gamma rays. Scientists using data from our Fermi Gamma-ray Space Telescope discovered these structures in 2010, and we're still learning about them.

This image captures the majestic “Fermi bubbles” that extend above and below our Milky Way galaxy, set against the black background of space. A glowing blue line horizontally crosses the center of the image, showing our perspective from Earth of our galaxy’s spiral arms and the wispy clouds of material above and below it. Cloudy bubbles, colored deep magenta to represent Fermi’s gamma-ray vision, extend above and below the galactic plane. These bubbles are enormous, extending roughly half of the Milky Way's diameter and filling much of the top and bottom of the image. The image is watermarked “Credit: NASA/DOE/Fermi LAT Collaboration.”

Our third astronomical gift is … three types of black holes

Most black holes fit into two size categories: stellar-mass goes up to hundreds of Suns, and supermassive starts at hundreds of thousands of Suns. But what happens between those two? Where are the midsize ones? With the help of NASA’s Hubble Space Telescope, scientists found the best evidence yet for that third, in between type that we call intermediate-mass black holes. The masses of these black holes should range from around a hundred to hundreds of thousands of times the Sun’s mass. The hunt continues for these elusive black holes.

This cartoon depicts two black holes as birds, with a small one representing a stellar-mass black hole on the left and an enormous one representing a supermassive black hole on the right. These two birds appear on a tan background and flap their wings, and then a circle with three question marks pops up between them to represent the intermediate-mass black holes that scientists are hunting for. The image is watermarked “Credit: NASA’s Goddard Space Flight Center.”

Our fourth and fifth astronomical gifts are … Stephan’s Quintet

When looking at this stunning image of Stephan’s Quintet from our James Webb Space Telescope, it seems like five galaxies are hanging around one another — but did you know that one of the galaxies is much closer than the others? Four of the five galaxies are hanging out together about 290 million light-years away, but the fifth and leftmost galaxy in the image below — called NGC 7320 — is actually closer to Earth at just 40 million light-years away.

A group of five galaxies that appear close to each other in the sky: two in the middle, one toward the top, one to the upper left, and one toward the bottom. Four of the five appear to be touching. One is somewhat separated. In the image, the galaxies are large relative to the hundreds of much smaller (more distant) galaxies in the background. All five galaxies have bright white cores. Each has a slightly different size, shape, structure, and coloring. Scattered across the image, in front of the galaxies are a number of foreground stars with diffraction spikes: bright white points, each with eight bright lines radiating out from the center. The image is watermarked with the text “Credits: NASA, ESA, CSA, and STScI.”

Our sixth astronomical gift is … an eclipsing six-star system

Astronomers found a six-star system where all of the stars undergo eclipses, using data from our TESS mission, a supercomputer, and automated eclipse-identifying software. The system, called TYC 7037-89-1, is located 1,900 light-years away in the constellation Eridanus and the first of its kind we’ve found.

This diagram shows the sextuple star system TYC 7037-89-1, a group of six stars that interact with each other in complex orbits. The stars are arranged in pairs: System A, System B, and System C, each of which is shown as having one larger white star and one smaller yellow star. The two stars of System A, in the upper left, are connected by a red oval and labeled "1.3-day orbit." The two stars of System C, just below System A, are connected by a turquoise oval and labeled "1.6-day orbit." Additionally, these two systems orbit each other, shown as a larger blue oval connecting the two and labeled "A and C orbit every 4 years." On the other side of the image, in the bottom right, the two stars of System B are connected by a green oval and labeled "8.2-day orbit." Lastly, Systems A, B and C all interact with System B orbiting the combined A-C system, shown as a very large lilac oval labeled "AC and B orbit every 2,000 years." A caption at the bottom of the image notes, "Star sizes are to scale, orbits are not." The image is watermarked with the text “Illustration” and “Credit: NASA's Goddard Space Flight Center.”

Our seventh astronomical gift is … seven Earth-sized planets

In 2017, our now-retired Spitzer Space Telescope helped find seven Earth-size planets around TRAPPIST-1. It remains the largest batch of Earth-size worlds found around a single star and the most rocky planets found in one star’s habitable zone, the range of distances where conditions may be just right to allow the presence of liquid water on a planet’s surface.

Further research has helped us understand the planets’ densities, atmospheres, and more!

his animated image shows an artist's concept of the star TRAPPIST-1, an ultra-cool dwarf, and the seven Earth-size planets orbiting it. TRAPPIST-1 is large and glows bright orange, while the planets are smaller and in shades of cool gray-blue. The image is highly stylized to look like glowing balls sitting on a shiny surface, and neither the sizes nor distances are to scale. The planets closer to TRAPPIST-1 have droplets of water standing on the surface around them, indicating that they may have liquid water. Planets further away have frost around them, indicating that those are more likely to have significant amounts of ice, especially on the side that faces away from the star. Our view pans across the system, from the center outward, and faint tan rings depict the orbits of each planet. The image is watermarked with the text “Illustration” and “Credit: NASA/JPL-Caltech/R. Hurt (IPAC).”

Our eighth astronomical gift is … an (almost) eight-foot mirror

The primary mirror on our Nancy Grace Roman Space Telescope is approximately eight feet in diameter, similar to our Hubble Space Telescope. But Roman can survey large regions of the sky over 1,000 times faster, allowing it to hunt for thousands of exoplanets and measure light from a billion galaxies.

Side profile of a man standing in front of the Nancy Grace Roman Space Telescope Primary mirror. The man wears a long white coat, hair net, facemask, and glasses. The man is standing to the left of the mirror, and looking at it. The mirror faces the man, so it appears to be looking back at him. The mirror is a flat, smooth, silver disk with a black cylinder protruding from its center. Behind the mirror, a black square houses hardware for the mirror. The image is watermarked “Credit: NASA/Chris Gunn.”

Our ninth astronomical gift is … a kilonova nine days later

In 2017, the National Science Foundation (NSF)’s Laser Interferometer Gravitational-Wave Observatory (LIGO) and European Gravitational Observatory’s Virgo detected gravitational waves from a pair of colliding neutron stars. Less than two seconds later, our telescopes detected a burst of gamma rays from the same event. It was the first time light and gravitational waves were seen from the same cosmic source. But then nine days later, astronomers saw X-ray light produced in jets in the collision’s aftermath. This later emission is called a kilonova, and it helped astronomers understand what the slower-moving material is made of.

This animated illustration shows what happened in the nine days following a neutron star merger known as GW170817, detected on Aug. 17, 2017. In the first part of the animation, a pair of glowing blue neutron stars spiral quickly towards each other and merge with a bright flash. The merger creates gravitational waves (shown as pale arcs rippling out from the center), a near-light-speed jet that produced gamma rays (shown as brown cones and a rapidly-traveling magenta glow erupting from the center of the collision), and a donut-shaped ring of expanding blue debris around the center of the explosion. A variety of colors represent the many wavelengths of light produced by the kilonova, creating violet to blue-white to red bursts at the top and bottom of the collision. In the second part of the animation, we see the collision as it would appear from Earth, looking like a burst of red light in the lower left and a huge umbrella-shaped cascade of blue light in the upper right, representing X-rays.  The image is watermarked with the text “Credit: NASA's Goddard Space Flight Center/CI Lab” and “Illustration.”

Our tenth astronomical gift is … NuSTAR’s ten-meter-long mast

Our NuSTAR X-ray observatory is the first space telescope able to focus on high-energy X-rays. Its ten-meter-long (33 foot) mast, which deployed shortly after launch, puts NuSTAR’s detectors at the perfect distance from its reflective optics to focus X-rays. NuSTAR recently celebrated 10 years since its launch in 2012.

This animation shows an artist’s concept of the NuSTAR X-ray observatory orbiting above the blue marble of Earth and deploying its 10-meter-long (33 foot) mast shortly after launch in 2012. NuSTAR is roughly cylindrical, with a shiny silver covering and a pair of blue solar panels on each of its sides. As we pan around the spacecraft, silver scaffolding extends from inside, separating the ends of the telescope to the right distance to begin observing the universe in X-rays. The image is watermarked with the text “Illustration” and “Credit: Credit: NASA/JPL-Caltech.”

Our eleventh astronomical gift is … eleven days of observations

How long did our Hubble Space Telescope stare at a seemingly empty patch of sky to discover it was full of thousands of faint galaxies? More than 11 days of observations came together to capture this amazing image — that’s about 1 million seconds spread over 400 orbits around Earth!

This animated image zooms into the Hubble Ultra Deep Field, showing how a tiny patch of “empty” sky turned out to contain about 10,000 galaxies. The sequence begins with a starry backdrop, then we begin to zoom into the center of this image. As we travel, larger and brighter objects come into view, including dazzling spiral and elliptical galaxies in reds, oranges, blues, and purples. The image is watermarked with the text “Credit: NASA, G. Bacon and Z. Levay (STScI).”

Our twelfth astronomical gift is … a twelve-kilometer radius

Pulsars are collapsed stellar cores that pack the mass of our Sun into a whirling city-sized ball, compressing matter to its limits. Our NICER telescope aboard the International Space Station helped us precisely measure one called J0030 and found it had a radius of about twelve kilometers — roughly the size of Chicago! This discovery has expanded our understanding of pulsars with the most precise and reliable size measurements of any to date.

In this simulation of a pulsar’s magnetic fields, dozens of thin lines dance around a central gray sphere, which is the collapsed core of a dead massive star. Some of these lines, colored orange, form loops on the surface of the sphere. Others, colored blue, arc away from two spots on the lower half of the sphere and vanish into the black background. The image is watermarked with the text “Simulation” and “Credit: NASA's Goddard Space Flight Center.”

Stay tuned to NASA Universe on Twitter and Facebook to keep up with what’s going on in the cosmos every day. You can learn more about the universe here.

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8 years ago

Want to Send Your Art to the International Space Station?!

For children ages 4-12, we’re hosting an art contest! Get the details:

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We are working with Boeing and SpaceX to build human spaceflight systems, like rockets and spacecraft, to take astronauts to the International Space Station. These companies will fly astronauts to orbit around Earth while we focus on plans to explore deeper into our solar system. 

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Get out your art supplies and use your creative imagination to show us the present and future of traveling in space!

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There are no grocery stores in space, but there may soon be farms. Very small farms that are important to a crew conducting a mission to deep space. That’s because our astronauts will need to grow some of their own food. Researchers on Earth and astronauts on the International Space Station are already showing what is needed to grow robust plants in orbit.

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What would you take to space? Astronaut Suni Williams took a cutout of her dog, Gorbie, on her first mission to the International Space Station. 

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Kids 4 to 12, draw what you would take and enter it in our Children’s Artwork Calendar contest! Your entry could be beamed to the space station!

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Go to http://go.nasa.gov/2fvRLNf for more information about the competition’s themes, rules and deadlines plus the entry form. 

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Get your parent's permission, of course!

Email your entry form and drawing to us at: ksc-connect2ccp@mail.nasa.gov

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6 years ago
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The year is 1965, and thanks to telecommunication engineers at our Jet Propulsions Laboratory, the first color version of one of our first Martian images had been created. Brought to life by hand coloring numbered strips, this image is a true blast to the past.

Fast forward to the 21st century and our Mars InSight mission now enables us to gawk at the Martian horizon as if we were there. InSight captured this panorama of its landing site on Dec. 9, 2018, the 14th Martian day, or sol, of its mission. The 290-degree perspective surveys the rim of the degraded crater InSight landed in and was made up of 30 photos stitched together.

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8 years ago

Solar System: Things to Know This Week

Be a scientist for a day, solstice on the Red Planet, historic launches and more!

Solar System: Things To Know This Week

1. Scientist for a Day!

This year's Scientist for a Day essay contest was announced last week. Write an essay on one of the three images above. Essays are due in Feb. 2017. Students in grades 5-12 in U.S. schools, after-school and home-school programs, scout troops and museum programs are eligible to participate.

+ Learn more

Solar System: Things To Know This Week

2. Tuesday is Winter Solstice on Mars' Northern Hemisphere

Mars' orbit is much more eccentric than Earth's. The winters in the northern hemisphere are warm and short, as Mars is near perihelion—closer to the sun. This means that the winters in the southern hemisphere are long and cold.

+ Read Mars: The Other Terrestrial Planet

+ Seasons on Mars (Malin Space Science Systems) 

Solar System: Things To Know This Week

3. Launch-iversaries!

We’re celebrating two launch anniversaries. Before Curiosity. Before Spirit and Opportunity, there was Pathfinder and the hardy Sojourner rover, launched on Dec. 4, 1996. Pathfinder was a demonstration of the technology necessary to deliver a lander and a free-ranging robotic rover to the surface of Mars in a cost-effective and efficient manner. The lander, formally named the Carl Sagan Memorial Station following its successful touchdown, and the rover, named Sojourner after American civil rights crusader Sojourner Truth, both outlived their design lives — the lander by nearly three times, and the rover by 12 times! We continued the tradition with Spirit and Opportunity. Now there is the Mars Science Laboratory (with the Curiosity rover in stowage), which was launched on Nov. 26, 2011. It landed successfully in Gale Crater at 1:31 am EDT on Aug. 6, 2012. 

+ Go Back in Time

+ Video: Where Were You When Curiosity Landed on Mars? 

Solar System: Things To Know This Week

4. Mars Ice Deposit Holds as Much Water as Lake Superior

Water ice makes up half or more of an underground layer in a large region of Mars, about halfway from the equator to the north pole. The amount of water in this deposit—assessed using a radar aboard NASA's Mars Reconnaissance Orbiter—is about as much as in Lake Superior.

+ Read More

Solar System: Things To Know This Week

5. A Little Bit of History

Finally, it’s been seven years since Cassini caught one of its most stunning views of the plume on Saturn's moon Enceladus.

+ Read More

Discover the full list of 10 things to know about our solar system this week HERE.

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5 years ago

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

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

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

Meet the graduates:

Kayla Barron

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

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

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

Zena Cardman

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

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

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

Raja Chari

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

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

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

Matthew Dominick

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

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

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

Bob Hines

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

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

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

Warren Hoburg

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

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

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

Dr. Jonny Kim

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

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

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

Jasmin Moghbeli

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

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

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

Loral O’Hara

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

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

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

Dr. Frank Rubio

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

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

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

Jessica Watkins

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

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

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

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

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2 years ago

See the Universe in a New Way with the Webb Space Telescope's First Images

Are you ready to see unprecedented, detailed views of the universe from the James Webb Space Telescope, the largest and most powerful space observatory ever made? Scroll down to see the first full-color images and data from Webb. Unfold the universe with us. ✨

Carina Nebula

See The Universe In A New Way With The Webb Space Telescope's First Images

This landscape of “mountains” and “valleys” speckled with glittering stars, called the Cosmic Cliffs, is the edge of the star-birthing Carina Nebula. Usually, the early phases of star formation are difficult to capture, but Webb can peer through cosmic dust—thanks to its extreme sensitivity, spatial resolution, and imaging capability. Protostellar jets clearly shoot out from some of these young stars in this new image.

Southern Ring Nebula

See The Universe In A New Way With The Webb Space Telescope's First Images

The Southern Ring Nebula is a planetary nebula: it’s an expanding cloud of gas and dust surrounding a dying star. In this new image, the nebula’s second, dimmer star is brought into full view, as well as the gas and dust it’s throwing out around it. (The brighter star is in its own stage of stellar evolution and will probably eject its own planetary nebula in the future.) These kinds of details will help us better understand how stars evolve and transform their environments. Finally, you might notice points of light in the background. Those aren’t stars—they’re distant galaxies.

Stephan’s Quintet

See The Universe In A New Way With The Webb Space Telescope's First Images

Stephan’s Quintet, a visual grouping of five galaxies near each other, was discovered in 1877 and is best known for being prominently featured in the holiday classic, “It’s a Wonderful Life.” This new image brings the galaxy group from the silver screen to your screen in an enormous mosaic that is Webb’s largest image to date. The mosaic covers about one-fifth of the Moon’s diameter; it contains over 150 million pixels and is constructed from almost 1,000 separate image files. Never-before-seen details are on display: sparkling clusters of millions of young stars, fresh star births, sweeping tails of gas, dust and stars, and huge shock waves paint a dramatic picture of galactic interactions.

WASP-96 b

See The Universe In A New Way With The Webb Space Telescope's First Images

WASP-96 b is a giant, mostly gas planet outside our solar system, discovered in 2014. Webb’s Near-Infrared Imager and Slitless Spectrograph (NIRISS) measured light from the WASP-96 system as the planet moved across the star. The light curve confirmed previous observations, but the transmission spectrum revealed new properties of the planet: an unambiguous signature of water, indications of haze, and evidence of clouds in the atmosphere. This discovery marks a giant leap forward in the quest to find potentially habitable planets beyond Earth.

Webb's First Deep Field

See The Universe In A New Way With The Webb Space Telescope's First Images

This image of galaxy cluster SMACS 0723, known as Webb’s First Deep Field, looks 4.6 billion years into the past. Looking at infrared wavelengths beyond Hubble’s deepest fields, Webb’s sharp near-infrared view reveals thousands of galaxies—including the faintest objects ever observed in the infrared—in the most detailed view of the early universe to date. We can now see tiny, faint structures we’ve never seen before, like star clusters and diffuse features and soon, we’ll begin to learn more about the galaxies’ masses, ages, histories, and compositions.

These images and data are just the beginning of what the observatory will find. It will study every phase in the history of our Universe, ranging from the first luminous glows after the Big Bang, to the formation of solar systems capable of supporting life on planets like Earth, to the evolution of our own Solar System.

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Credits: NASA, ESA, CSA, and STScI


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9 years ago

Space Station Research: Cardiovascular Health

Each month, we highlight a different research topic on the International Space Station. In February, our focus is cardiovascular health, which coincides with the American Hearth Month.

Like bones and muscle, the cardiovascular system deconditions (gets weaker) in microgravity. Long-duration spaceflight may increase the risk of damage and inflammation in the cardiovascular system primarily from radiation, but also from psychological stress, reduced physical activity, diminished nutritional standards and, in the case of extravehicular activity, increased oxygen exposure.

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Even brief periods of exposure to reduced-gravity environments can result in cardiovascular changes such as fluid shifts, changes in total blood volume, heartbeat and heart rhythm irregularities and diminished aerobic capacity.

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The weightless environment of space also causes fluid shifts to occur in the body. This normal shift of fluids to the upper body in space causes increased inter-cranial pressure which could be reducing visual capacity in astronauts. We are currently testing how this can be counteracted by returning fluids to the lower body using a “lower body negative pressure” suit, also known as Chibis.

Spaceflight also accelerates the aging process, and it is important to understand this process to develop specific countermeasures. Developing countermeasures to keep astronauts’ hearts healthy in space is applicable to heart health on Earth, too!

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On the space station, one of the tools we have to study heart health is the ultrasound device, which uses harmless sound waves to take detailed images of the inside of the body. These images are then viewed by researchers and doctors inside Mission Control. So with minimal training on ultrasound, remote guidance techniques allow astronauts to take images of their own heart while in space. These remote medicine techniques can also be beneficial on Earth.

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


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9 years ago

7 Sports Astronauts Love Without Gravity (Including Football)

Astronauts onboard the International Space Station spend most of their time doing science, exercising and maintaining the station. But they still have time to shoot hoops and toss around a football.

From chess to soccer, there’s a zero-gravity spin to everything.

1. Baseball

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Baseball: America’s favorite pastime. JAXA astronaut, Satoshi Furukawa shows us how microgravity makes it possible to be a one-man team. It would be a lot harder to hit home runs if the players could jump that high to catch the ball.

2. Chess

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Yes, it’s a sport, and one time NASA astronaut Greg Chamitoff (right) played Earth on a Velcro chess board. An elementary school chess team would pick moves that everyone could vote for online. The winning move would be Earth’s play, and then Chamitoff would respond. About every two days, a move would be made. But who won the historic Earth vs. Space match? Earth! Chamitoff resigned after Earth turned its pawn into a queen, but it was game well played.

3. Soccer

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NASA astronaut Steve Swanson put a new spin on soccer by juggling the ball upside down. However, he might not have considered himself upside down. On the space station, up and down are relative.

4. Gymnastics

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NASA astronauts usually sign off their videos with a zero-gravity somersault (either forwards or backwards). But astronauts are also proficient in handstands, flips and twists. The predecessor to the International Space Station, the Skylab, had the best space for the moves. The current space station is a bit tight in comparison.

5. Basketball

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Objects that aren’t heavy don’t move very well on the space station. They kind of just float. It’s like Earth, but exaggerated. For example, on Earth a beach ball wouldn’t go as far as a basketball. The same is true in space, which is why playing with a basketball in space is more fun than playing with a beach ball.

6. Golf

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People talk about hitting golf balls off skyscrapers, but what about off the International Space Station? While golf isn’t a normal occurrence on the station, it’s been there. One golf company even sent an experiment to the station to find out how to make better golf clubs.

7. Football

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Zero gravity doesn’t make everything easier. Astronauts need to relearn how to throw things because their brains need to relearn how to interpret sensory information. A bowling ball on the space station no longer feels as heavy as a bowling ball on Earth. When astronauts first throw things on the space station, everything keeps going too high. That would put a wrench in your spiral for a couple of months. But once you adjust, the perfect spiral will just keep spiraling!

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


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8 years ago

A Ring of Fire Eclipse in the Southern Hemisphere

On Feb. 26, a “ring of fire” will be visible in the sky above parts of the Southern Hemisphere, including Chile, Argentina and Angola. This is called an annular eclipse.

A Ring Of Fire Eclipse In The Southern Hemisphere

Credit: Dale Cruikshank

If you live within the viewing area, even though most of the sun will be obscured by the moon, it’s essential to observe eye safety. This includes using a proper solar filter or an indirect viewing method during ALL phases of this eclipse.

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See full graphic

What is an annular eclipse? During any type of solar eclipse, the sun, moon, and Earth line up, allowing the moon to cast its shadow on Earth’s surface in a partial or total solar eclipse.

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Download this animation

An annular eclipse is the product of almost the same celestial geometry as a total solar eclipse – that is, from the perspective of some place on Earth, the moon crosses in front of the sun's center. 

But an annular eclipse is different in one important way – the moon is too far from Earth to obscure the sun completely, leaving the sun’s edges exposed and producing the “ring of fire” effect for which annular eclipses are known. Because the moon’s orbit is slightly oblong, its distance from Earth – and therefore its apparent size compared to the sun’s – is constantly changing.

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An annular eclipse seen in extreme ultraviolet light – a type of light invisible to humans – by the Hinode spacecraft on Jan. 4, 2011.

Any time part, or all, of the sun’s surface is exposed – whether during an annular eclipse, a partial eclipse, or just a regular day – it’s essential to use a proper solar filter or an indirect viewing method to view the sun. You can NEVER look directly at the sun, and an annular eclipse is no exception!  

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If you live in the Southern Hemisphere or near the equator, check this interactive map for partial eclipse times.

If you live in North America, you’ll have a chance to see an eclipse later this year. On Aug. 21, 2017, a total solar eclipse will cross the US – the first total solar eclipse in the contiguous US in nearly 40 years! The path of totality for the August eclipse runs from coast to coast.

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Within this narrow path of totality, the moon will completely obscure the sun – unlike an annular eclipse – revealing the sun’s outer atmosphere. People in other parts of North America will see a partial solar eclipse, weather permitting. Find out what you can see during the Aug. 21, 2017, eclipse in your area with our maps, and explore the rest of eclipse2017.nasa.gov for more information.

For more eclipse science, visit www.nasa.gov/eclipse.

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


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