How Often Do Solar Eclipses Occur On Other Planets Like Mars Or Venus?

8 Common Questions About Our James Webb Space Telescope

You might have heard the basics about our James Webb Space Telescope, or Webb, and still have lots more questions! Here are more advanced questions we are frequently asked. (If you want to know the basics, read this Tumblr first!)

Webb is our upcoming infrared space observatory, which will launch in 2021. It will spy the first luminous objects that formed in the universe and shed light on how galaxies evolve, how stars and planetary systems are born, and how life could form on other planets.

1. Why is the mirror segmented? 

The James Webb Space Telescope has a 6.5-meter (21.3-foot) diameter mirror, made from 18 individual segments. Webb needs to have an unfolding mirror because the mirror is so large that it otherwise cannot fit in the launch shroud of currently available rockets.

The mirror has to be large in order to see the faint light from the first star-forming regions and to see very small details at infrared wavelengths. 

Designing, building, and operating a mirror that unfolds is one of the major technological developments of Webb. Unfolding mirrors will be necessary for future missions requiring even larger mirrors, and will find application in other scientific, civil, and military space missions.

2. Why are the mirrors hexagonal?

In short, the hexagonal shape allows a segmented mirror to be constructed with very small gaps, so the segments combine to form a roughly circular shape and need only three variations in prescription. If we had circular segments, there would be gaps between them.

Finally, we want a roughly circular overall mirror shape because that focuses the light into the most symmetric and compact region on the detectors. 

An oval mirror, for example, would give images that are elongated in one direction. A square mirror would send a lot of the light out of the central region.

3. Is there a danger from micrometeoroids?

A micrometeoroid is a particle smaller than a grain of sand. Most never reach Earth's surface because they are vaporized by the intense heat generated by the friction of passing through the atmosphere. In space, no blanket of atmosphere protects a spacecraft or a spacewalker.

Webb will be a million miles away from the Earth orbiting what we call the second Lagrange point (L2). Unlike in low Earth orbit, there is not much space debris out there that could damage the exposed mirror. 

But we do expect Webb to get impacted by these very tiny micrometeoroids for the duration of the mission, and Webb is designed to accommodate for them.

All of Webb's systems are designed to survive micrometeoroid impacts.

4. Why does the sunshield have five layers?

Webb has a giant, tennis-court sized sunshield, made of five, very thin layers of an insulating film called Kapton.  

Why five? One big, thick sunshield would conduct the heat from the bottom to the top more than would a shield with five layers separated by vacuum. With five layers to the sunshield, each successive one is cooler than the one below. 

The heat radiates out from between the layers, and the vacuum between the layers is a very good insulator. From studies done early in the mission development five layers were found to provide sufficient cooling. More layers would provide additional cooling, but would also mean more mass and complexity. We settled on five because it gives us enough cooling with some “margin” or a safety factor, and six or more wouldn’t return any additional benefits.

Fun fact: You could nearly boil water on the hot side of the sunshield, and it is frigid enough on the cold side to freeze nitrogen!

5. What kind of telescope is Webb?

Webb is a reflecting telescope that uses three curved mirrors. Technically, it’s called a three-mirror anastigmat.

6. What happens after launch? How long until there will be data?

We’ll give a short overview here, but check out our full FAQ for a more in-depth look.

In the first hour: About 30 minutes after liftoff, Webb will separate from the Ariane 5 launch vehicle. Shortly after this, we will talk with Webb from the ground to make sure everything is okay after its trip to space.

In the first day: After 24 hours, Webb will be nearly halfway to the Moon! About 2.5 days after launch, it will pass the Moon’s orbit, nearly a quarter of the way to Lagrange Point 1 (L2).

In the first week: We begin the major deployment of Webb. This includes unfolding the sunshield and tensioning the individual membranes, deploying the secondary mirror, and deploying the primary mirror.

In the first month: Deployment of the secondary mirror and the primary mirror occur. As the telescope cools in the shade of the sunshield, we turn on the warm electronics and initialize the flight software. As the telescope cools to near its operating temperature, parts of it are warmed with electronic heaters. This prevents condensation as residual water trapped within some of the materials making up the observatory escapes into space.

In the second month: We will turn on and operate Webb’s Fine Guidance Sensor, NIRCam, and NIRSpec instruments. 

The first NIRCam image, which will be an out-of-focus image of a single bright star, will be used to identify each mirror segment with its image of a star in the camera. We will also focus the secondary mirror.

In the third month: We will align the primary mirror segments so that they can work together as a single optical surface. We will also turn on and operate Webb’s mid-infrared instrument (MIRI), a camera and spectrograph that views a wide spectrum of infrared light. By this time, Webb will complete its journey to its L2 orbit position.

In the fourth through the sixth month: We will complete the optimization of the telescope. We will test and calibrate all of the science instruments.

After six months: The first scientific images will be released, and Webb will begin its science mission and start to conduct routine science operations.

7. Why not assemble it in orbit?

Various scenarios were studied, and assembling in orbit was determined to be unfeasible.

We examined the possibility of in-orbit assembly for Webb. The International Space Station does not have the capability to assemble precision optical structures. Additionally, space debris that resides around the space station could have damaged or contaminated Webb’s optics. Webb’s deployment happens far above low Earth orbit and the debris that is found there.

Finally, if the space station were used as a stopping point for the observatory, we would have needed a second rocket to launch it to its final destination at L2. The observatory would have to be designed with much more mass to withstand this “second launch,” leaving less mass for the mirrors and science instruments.

8. Who is James Webb?

This telescope is named after James E. Webb (1906–1992), our second administrator. Webb is best known for leading Apollo, a series of lunar exploration programs that landed the first humans on the Moon. 

However, he also initiated a vigorous space science program that was responsible for more than 75 launches during his tenure, including America's first interplanetary explorers.

Looking for some more in-depth FAQs? You can find them HERE.

Learn more about the James Webb Space Telescope HERE, or follow the mission on Facebook, Twitter and Instagram.

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What’s in Store for 2017 at NASA?

With 2016 behind us, we take the time to not only reflect on what we’ve accomplished, but also take a look to what’s ahead for the next year.

Here are a few things to look forward to in 2017… 

New Telescope in Town

This year marked big progress on our James Webb Space Telescope and there are still a number of large milestones before the telescope is launched in 2018. Once launched, JWST will be the premier observatory of the next decade. 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.

In 2017, the telescope will be shipped to our Johnson Space Center in Houston, Texas where end-to-end optical testing in a simulated cryo-temperature and vacuum space environment will occur.

Epic Final Year at Saturn

After more than 12 years studying Saturn, its rings and moons, our Cassini spacecraft is in its final year of its epic voyage. The conclusion of the historic scientific odyssey is planned for September 2017, but not before the spacecraft completes a daring two-part endgame.

Cassini’s final phase – called the Grand Finale – begins in earnest in April 2017. During this time, Cassini will make the closest-ever observations of Saturn, mapping the planet’s magnetic and gravity fields with exquisite precision and returning ultra-close views of the atmosphere.

Delivering Supplies to Space

Our ambitious commercial space program has enabled a successful partnership with two American companies to resupply the International Space Station. 

The companies are successfully resupplying the space station, and more missions to deliver scientific investigations and cargo are planned for 2017.  

Launching Two Earth Missions

New Earth science missions got underway in 2016 to enable studies that will unravel the complexities of our planet from the highest reaches of Earth’s atmosphere to its core. In 2017, we will launch two Earth-observing instruments to the International Space Station as part of our ongoing use of the orbiting space laboratory to study our changing planet.

The Stratospheric Aerosol and Gas Experiment III (SAGE III) will give us a new way to monitor Earth’s protective ozone layer and document its ongoing recovery. The Lightning Imaging Sensor (LIS) will measure both in-cloud and cloud-to-ground lightning over much of the planet, data that will help improve our understanding of lightning’s connections to weather and related phenomena.

Commercial Crew

Our Commercial Crew Program is working with American aerospace industry as companies develop and operate a new generation of spacecraft and launch systems capable of carrying crews to low-Earth orbit and the International Space Station.

In 2017, astronauts will train for commercial flights and launch pad 39A will be completed at Kennedy Space Center in Florida. Work is wrapping up on a new structure built specifically for the needs of astronauts climbing into Boeing's CST-100 Starliner as it stands atop a United Launch Alliance Atlas V rocket at Space Launch Complex 41 in Florida. In 2017, the 200-foot-tall Crew Access Tower and Crew Access Arm will see installation and testing of emergency evacuation systems. 

SpaceX has also overhauled the historic Launch Pad 39A at Kennedy and built new support structures for the company's line of Falcon rockets. The Crew Access Arm, currently under construction, will be connected in mid-2017 to provide a bridge from the fixed service structure to the Crew Dragon spacecraft so astronauts can board before launch

Orion Progress

Our Orion spacecraft is being built to take humans farther than they’ve ever gone before. Orion will serve as the exploration vehicle that will carry the crew to space, provide emergency abort capability, sustain the crew during the space travel and provide safe re-entry from deep space return velocities.

In 2017, computers in the Orion crew module for the spacecraft’s first mission with our Space Launch System rocket will be turned on for the first time to verify the spacecraft can route power and send commands. While the Orion outfitting and assembly process for the first mission of the spacecraft atop the SLS rocket continues in 2017, construction will also begin on the vehicle for the first Orion flight with astronauts that will fly as early as 2021.

Cutting Edge Technology

Our Space Technology office is dedicated to pushing the technological envelope, taking on challenges not only to further space agency missions near Earth, but also to sustain future deep space exploration activities. 

In 2016, the office focused on and made significant progress in advancing technologies and capabilities that will continue into 2017. 

Advances in Aeronautics

Our rich aeronautical research heritage added to its history of technical innovation in 2016 with advancements that will help make airplanes use less fuel, release fewer emissions and fly more quietly…and that includes working to return supersonic flight to the commercial marketplace.

We took steps in 2016 to resume designing, building and flying several experimental aircraft, or X-planes, as a means to demonstrate key green technologies and help accelerate their use by industry. In 2017, this research will continue to grow and develop.

Thanks for joining us in 2016, we look forward to sharing our progress with you in the coming year. 

Happy New Year!

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INCOMING! Roving scientist to arrive on Mars. 

Save the date! One year from today, Feb. 18, 2021, our next rover is set to land on Mars. Get to know #Mars2020 now! Click here. 

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Our Flying Observatory Goes to New Zealand!

Our flying observatory, called SOFIA, carries a 100-inch telescope inside a Boeing 747SP aircraft. Scientists onboard study the life cycle of stars, planets (including Pluto’s atmosphere), the area around black holes and complex molecules in space. 

Heading South

Once each year our flying observatory, SOFIA, its team and instruments travel to the Southern Hemisphere to Christchurch, New Zealand. From there the team studies stars and other objects that cannot be seen while flying in the Northern Hemisphere.

What We Study

We often study star formation in our Milky Way Galaxy. But from the Southern Hemisphere we can also study the lifecycle of stars in two other galaxies called the Magellanic Clouds. The Magallenic Clouds have different materials in them, which changes how stars form in these galaxies. Scientists are studying these differences to better understand how the first stars in our universe formed.  

Home Away from Home

The observatory and its team use the National Science Foundation’s U.S. Antarctic Program facility at Christchurch International Airport. The Antarctic program’s off-season is June and July, so it’s an ideal time for us to use these facilities.

Another Blast of Winter

The Southern Hemisphere’s seasons are opposite from our own. When we are operating from Christchurch in June and July, it’s winter. This means that the nights are very long – ideal for our nighttime observing flights, which last approximately 10 hours.

Light Show

These observations often bring us so far south that the team onboard can see the Southern Lights, also called the Aurora Australis. This is the Southern Hemisphere equivalent of the Northern Lights, or Aurora Borealis, visible near the North Pole. Auroras are caused by particles from space hitting the atmosphere near Earth’s magnetic poles. Our scientists onboard SOFIA don’t study the aurora, but they do enjoy the view.

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What in the Universe is an Exoplanet?

Simply put, an exoplanet is a planet that orbits another star. 

All of the planets in our solar system orbit around the Sun. Planets that orbit around other stars outside our solar system are called exoplanets.

Just because a planet orbits a star (like Earth) does not mean that it is automatically stable for life. The planet must be within the habitable zone, which is the area around a star in which water has the potential to be liquid…aka not so close that all the water would evaporate, and not too far away where all the water would freeze.

Exoplanets are very hard to see directly with telescopes. They are hidden by the bright glare of the stars they orbit. So, astronomers use other ways to detect and study these distant planets by looking at the effects these planets have on the stars they orbit.

One way to search for exoplanets is to look for "wobbly" stars. A star that has planets doesn’t orbit perfectly around its center. From far away, this off-center orbit makes the star look like it’s wobbling. Hundreds of planets have been discovered using this method. However, only big planets—like Jupiter, or even larger—can be seen this way. Smaller Earth-like planets are much harder to find because they create only small wobbles that are hard to detect.

How can we find Earth-like planets in other solar systems?

In 2009, we launched a spacecraft called Kepler to look for exoplanets. Kepler looked for planets in a wide range of sizes and orbits. And these planets orbited around stars that varied in size and temperature.

Kepler detected exoplanets using something called the transit method. When a planet passes in front of its star, it’s called a transit. As the planet transits in front of the star, it blocks out a little bit of the star's light. That means a star will look a little less bright when the planet passes in front of it. Astronomers can observe how the brightness of the star changes during a transit. This can help them figure out the size of the planet.

By studying the time between transits, astronomers can also find out how far away the planet is from its star. This tells us something about the planet’s temperature. If a planet is just the right temperature, it could contain liquid water—an important ingredient for life.

So far, thousands of planets have been discovered by the Kepler mission.

We now know that exoplanets are very common in the universe. And future missions have been planned to discover many more!

Next month, we’re launching an explorer-class planet finder — the Transiting Exoplanet Survey Satellite (TESS). This mission will search the entire sky for exoplanets — planets outside our solar system that orbit sun-like stars.

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Much of the western United States began the morning with the view of a super blue blood moon total lunar eclipse. In this silent time lapse video, the complete eclipse is seen over NASA's Jet Propulsion Laboratory, located at the base of the San Gabriel Mountains near Pasadena, California.  This Jan. 31 full moon was special for three reasons: it was the third in a series of “supermoons,” when the Moon is closer to Earth in its orbit -- known as perigee -- and about 14 percent brighter than usual. It was also the second full moon of the month, commonly known as a “blue moon.” The super blue moon will pass through Earth’s shadow to give viewers in the right location a total lunar eclipse. While the Moon is in the Earth’s shadow it will take on a reddish tint, known as a “blood moon.”

Credits: NASA/JPL-Caltech

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50 years ago, three Apollo astronauts rode this 363 foot tall rocket, the Saturn V, embarking on one of the greatest missions of mankind – to step foot on another world. On July 20, 1969, astronauts Buzz Aldrin, Michael Collins and Neil Armstrong made history when they arrived at the Moon. Thanks to the Saturn V rocket, we were able to complete this epic feat, returning to the lunar surface a total of six times. The six missions that landed on the Moon returned a wealth of scientific data and almost 400 kilograms of lunar samples. 

In honor of this historic launch, the National Air and Space Museum is projecting the identical rocket that took our astronauts to the Moon on the Washington Monument in Washington, D.C.

This week, you can watch us salute our Apollo 50th heroes and look forward to our next giant leap for future missions to the Moon and Mars. Tune in to a special two-hour live NASA Television broadcast at 1 p.m. ET on Friday, July 19. Watch the program at www.nasa.gov/live.

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Science Launching to Station Looks Forward and Back

Some of the earliest human explorers used mechanical tools called sextants to navigate vast oceans and discover new lands. Today, high-tech tools navigate microscopic DNA to discover previously unidentified organisms. Scientists aboard the International Space Station soon will have both types of tools at their disposal.

Orbital ATK’s Cygnus spacecraft is scheduled to launch its ninth contracted cargo resupply mission to the space station no earlier than May 21. Sending crucial science, supplies and cargo to the crew of six humans living and working on the orbiting laboratory.

Our Gemini missions conducted the first sextant sightings from a spacecraft, and designers built a sextant into Apollo vehicles as a lost-communications navigation backup. The Sextant Navigation investigation tests use of a hand-held sextant for emergency navigation on missions in deep space as humans begin to travel farther from Earth.

Jim Lovell (far left) demonstrated on Apollo 8 that sextant navigation could return a space vehicle home. 

The remoteness and constrained resources of living in space require simple but effective processes and procedures to monitor the presence of microbial life, some of which might be harmful. Biomolecule Extraction and Sequencing Technology (BEST) advances the use of sequencing processes to identify microbes aboard the space station that current methods cannot detect and to assess mutations in the microbial genome that may be due to spaceflight.  

Genes in Space 3 performed in-flight identification of bacteria on the station for the first time. BEST takes that one step farther, identifying unknown microbial organisms using a process that sequences directly from a sample with minimal preparation, rather than with the traditional technique that requires growing a culture from the sample.

Adding these new processes to the proven technology opens new avenues for inflight research, such as how microorganisms on the station change or adapt to spaceflight.

The investigation’s sequencing components provide important information on the station’s microbial occupants, including which organisms are present and how they respond to the spaceflight environment -- insight that could help protect humans during future space exploration. Knowledge gained from BEST could also provide new ways to monitor the presence of microbes in remote locations on Earth.

Moving on to science at a scale even smaller than a microbe, the new Cold Atom Lab (CAL) facility could help answer some big questions in modern physics.

CAL creates a temperature ten billion (Yup. BILLION) times colder than the vacuum of space, then uses lasers and magnetic forces to slow down atoms until they are almost motionless. CAL makes it possible to observe these ultra-cold atoms for much longer in the microgravity environment on the space station than would be possible on the ground.

Results of this research could potentially lead to a number of improved technologies, including sensors, quantum computers and atomic clocks used in spacecraft navigation.

A partnership between the European Space Agency (ESA) and Space Application Services (SpaceAps), The International Commercial Experiment, or ICE Cubes Service, uses a sliding framework permanently installed on the space station and “plug-and-play” Experiment Cubes.

The Experiment Cubes are easy to install and remove, come in different sizes and can be built with commercial off-the-shelf components, significantly reducing the cost and time to develop experiments.

ICE Cubes removes barriers that limit access to space, providing more people access to flight opportunities. Potential fields of research range from pharmaceutical development to experiments on stem cells, radiation, and microbiology, fluid sciences, and more.

For daily nerd outs, follow @ISS_Research on Twitter!

Watch the Launch + More!

What’s On Board Briefing

Join scientists and researchers as they discuss some of the investigations that will be delivered to the station on Saturday, May 19 at 1 p.m. EDT at nasa.gov/live. Have questions? Use #askNASA

CubeSat Facebook Live

The International Space Station is often used to deploy small satellites, a low-cost way to test technology and science techniques in space. On board this time, for deployment later this summer, are three CubeSats that will help us monitor rain and snow, study weather and detect and filter radio frequency interference (RFI). 

Join us on Facebook Live on Saturday, May 19 at 3:30 p.m. EDT on the NASA’s Wallops Flight Facility page to hear from experts and ask them your questions about these small satellites. 

Pre-Launch Briefing

Tune in live at nasa.gov/live as mission managers provide an overview and status of launch operations at 11 a.m. EDT on Sunday, May 20. Have questions? Use #askNASA

LIFTOFF!

Live launch coverage will begin on Monday, May 21 4:00 a.m. on NASA Television, nasa.gov/live, Facebook Live, Periscope, Twitch, Ustream and YouTube. Liftoff is slated for 4:39 a.m.

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Solar System: Things to Know This Week

Almost every day, we receive a message from a spacecraft more than 10.6 billion miles (about 17 billion km) away.

At that unimaginable distance, it takes the radio signal almost 16 hours to arrive. The spacecraft is Voyager 2, which launched 40 years ago this month. It's still operating, sending back dispatches from the dark reaches well beyond the orbit of Pluto. Even now, scientists are still actively exploring the outer boundaries of the solar system using Voyager 2, decades after its "Grand Tour" of the giant planets Jupiter, Saturn, Uranus and Neptune revealed their splendors like never before. This week, we recall 10 highlights from one of the most epic voyages in human history.

1. A Journey of 10 Billion Miles Begins With the First Step

Voyager 2 set out from Earth on Aug. 20, 1977. Even though it launched before its twin spacecraft, Voyager 1, it carried the '2' moniker because mission planners knew its trajectory would bring it to Jupiter after Voyager 1's arrival there.

2. The Grand Tour

Voyager 2's trajectory was special because it took advantage of a rare orbital alignment to fly by all four gas giant planets: Jupiter, Saturn, Uranus and Neptune. It was the first, and so far the only, spacecraft to carry out a close-up reconnaissance of Uranus and Neptune.

3. Not-So-Gentle Giant

Voyager 2 flew by Jupiter in April 1979, capturing striking images of the planet's volcanic moon Io and its violent storms larger than the entire Earth.

4. Saturn's Not the Only One

Jupiter has its own ring system, and Voyager 2 provided the first pictures.

5. An Ocean Under Ice

During its Jupiter encounter, Voyager 2 obtained close-up looks at Jupiter's moon Europa, including linear cracks and other features which first led scientists to realize Europa probably hides a vast sea of liquid water beneath an icy shell, the first known world outside Earth that could have an ocean.

6. Ringworld, the Prequel

Voyager 2 zoomed through the Saturn system in August 1981. It saw hints of mysterious features that the Cassini mission would later reveal in stunning detail, including Enceladus, with its bright surface that suggested geologic activity, and Saturn's intriguing hexagonal jet stream.

7. Swiftly by a Tilted Planet

In January 1984, Voyager offered humanity its first detailed look at the seventh planet, Uranus, the only one tilted on its side relative to the Sun. Voyager images revealed 11 new moons, including Juliet, Puck, Cressida, Rosalind and Ophelia. The moon Miranda presented a bizarre landscape that left scientists debating its origins for years. Voyager also captured views of the planet's lacy rings, and found that it is the coldest in the solar system, at minus 353 degrees Fahrenheit (59 Kelvin).

8. In Neptune's Blue Realm

After picking up a gravitational speed boost at each previous planetary encounter, by the time Voyager reached Neptune it shot through the entire system of Neptunian rings and moons in a matter of hours. Voyager saw a titanic storm in Neptune's windy atmosphere, discovered new moons, and revealed active geysers erupting on Triton's frigid surface.

9. Postcards From the Edge

Although their cameras are no longer functioning, other key scientific instruments on board both Voyager spacecraft are still collecting data. Voyager 1 is exploring the boundary between the Sun's realm and interstellar space. Voyager 2 hasn't traveled quite as far. In September 2007, it crossed the termination shock (where the speed of the solar wind of charged particles drops below the speed of sound) at a point about 84 Astronomical Units from the Sun (more than twice the distance to Pluto). See https://go.nasa.gov/2uwrndb

10. Ride Along

Voyager's mission is far from over. Engineers estimate the spacecraft will have enough power to operate into the mid-2020s. You can ride along at www.jpl.nasa.gov/voyager, or by following @NASAVoyager on Twitter and by downloading our free 3-D space simulation software, Eyes on the Solar System at eyes.nasa.gov.

One more thing: Inspired by the messages of goodwill carried on Voyager's Golden Record, you're invited to send a short, uplifting message to Voyager and all that lies beyond it via social media. With input from the Voyager team and a public vote, one of these messages will be selected for us to beam into interstellar space on Sept. 5, 2017—the 40th anniversary of Voyager 1's launch. Post your message on social media with the tag #MessageToVoyager by Aug 15. Details: www.jpl.nasa.gov/voyager/message/

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A View into the Past

Our Hubble Space Telescope just found the farthest individual star ever seen to date!

Nicknamed “Earendel” (“morning star” in Old English), this star existed within the first billion years after the universe’s birth in the big bang. Earendel is so far away from Earth that its light has taken 12.9 billion years to reach us, far eclipsing the previous single-star record holder whose light took 9 billion years to reach us.

Though Earendel is at least 50 times the mass of our Sun and millions of times as bright, we’d normally be unable to see it from Earth. However, the mass of a huge galaxy cluster between us and Earendel has created a powerful natural magnifying glass. Astronomers expect that the star will be highly magnified for years.

Earendel will be observed by NASA’s James Webb Space Telescope. Webb's high sensitivity to infrared light is needed to learn more about this star, because its light is stretched to longer infrared wavelengths due to the universe's expansion.