Planet - Blog Posts

Hail the Hexagon...

The full light of our sun allowed the Cassini spacecraft to capture this image of Saturn's hexagonal polar jet stream, but the sun does not provide much warmth. In addition to being low in the sky (just like summer at Earth's poles), the sun is nearly ten times as distant from Saturn as from Earth. This results in the sunlight being only about 1 percent as intense as at our planet. 

The view was obtained at a distance of approximately 560,000 miles (900,000 kilometers) from Saturn. Image scale is 33 miles (54 kilometers) per pixel.

More info: https://www.nasa.gov/image-feature/jpl/pia21327/hail-the-hexagon

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Happy Martian New Year!

For any planet, a year is the time it takes to make one orbit around the sun. Because Mars is farther away from the sun, it has to travel a greater distance than Earth. It takes Mars about twice as long as it does for Earth to make one circle around the sun…therefore, a year on Mars lasts twice as long.

On May 5, Mars passes solar longitude 0 as the sun crosses the equator on Mars. This is the vernal equinox and was chosen by planetary scientists as the start of a new year.

Mars has four seasons, roughly twice as long as those on Earth, but with more variation given Mars’ eccentric orbit and the fact its orbital speed varies more as a result.

Did you know that there’s a U.S. city named Mars? Mars, PA hosts an annual Mars New Year celebration and we’re participating in this two-day science, technology, engineering and math (STEM) event to inspire young people to pursue innovation and exploration.

More info on Mars, PA: http://www.marsnewyear.com/

Get updated images from the events in Mars, PA here: https://www.flickr.com/photos/nasahqphoto/sets/72157683457751005/

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Take a dive between Saturn and its rings to see what our Cassini spacecraft saw during its first daring plunge on April 26! 

As Cassini made its first-ever dive through the gap between Saturn and its rings on April 26, 2017, one of its imaging cameras took a series of rapid-fire images that were used to make this movie sequence. The video begins with a view of the vortex at Saturn's north pole, then heads past the outer boundary of the planet's hexagon-shaped jet stream and continues further southward. 

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

The Start of Cassini’s Grand Finale

Cue drumroll…

For the first time ever, our Cassini spacecraft dove through the narrow gap between Saturn and its rings on April 26. At 5 a.m. EDT, Cassini crossed the ring plane with its science instruments turned on and collecting data. 

During this dive, the spacecraft was not in contact with Earth. The first opportunity to regain contact with the spacecraft is expected around 3 a.m. EDT on April 27.

This area between Saturn and its rings has never been explored by a spacecraft before. What we learn from these daring final orbits will further our understanding of how giant planets, and planetary systems everywhere, form and evolve.

So, you might be asking…how did this spacecraft maneuver its orbit between Saturn and its rings? Well…let us explain!

On April 22, Cassini made its 127th and final close approach to Saturn’s moon Titan. The flyby put the spacecraft on course for its dramatic last act, known as the Grand Finale. 

As the spacecraft passed over Titan, the moon’s gravity bent its path, reshaping the robotic probe’s orbit slightly so that instead of passing just outside Saturn’s main rings, Cassini would begin a series of 22 dives between the rings and the planet.

With this assist, Cassini received a large increase in velocity of approximately 1,925 mph with respect to Saturn.

This final chapter of exploration and discovery is in many ways like a brand-new mission. Twenty-two times, the Cassini spacecraft will dive through the unexplored space between Saturn and its rings. What we learn from these ultra-close passes over the planet could be some of the most exciting revelations ever returned by the long-lived spacecraft.

Throughout these daring maneuvers, updates will be posted on social media at:

@CassiniSaturn on Twitter @NASAJPL on Twitter

Updates will also be available online at: https://saturn.jpl.nasa.gov/mission/grand-finale/milestones/ 

Follow along with us during this mission’s Grand Finale!

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Juno: Join the Mission!

Our Juno spacecraft may be millions of miles from Earth, but that doesn’t mean you can’t get involved with the mission and its science. Here are a few ways that you can join in on the fun:

Juno Orbit Insertion

This July 4, our solar-powered Juno spacecraft arrives at Jupiter after an almost five-year journey. In the evening of July 4, the spacecraft will perform a suspenseful orbit insertion maneuver, a 35-minute burn of its main engine, to slow the spacecraft by about 1,212 miles per hour so it can be captured into the gas giant’s orbit. Watch live coverage of these events on NASA Television:

Pre-Orbit Insertion Briefing Monday, July 4 at 12 p.m. EDT

Orbit Insertion Coverage Monday, July 4 at 10:30 p.m. EDT

Join Us On Social Media

Orbit Insertion Coverage Facebook Live Monday, July 4 at 10:30 p.m. EDT

Be sure to also check out and follow Juno coverage on the NASA Snapchat account!

JunoCam

The Juno spacecraft will give us new views of Jupiter’s swirling clouds, courtesy of its color camera called JunoCam. But unlike previous space missions, professional scientists will not be the ones producing the processed views, or even choosing which images to capture. Instead, the public will act as a virtual imaging team, participating in key steps of the process, from identifying features of interest to sharing the finished images online.

After JunoCam data arrives on Earth, members of the public will process the images to create color pictures. Juno scientists will ensure JunoCam returns a few great shots of Jupiter’s polar regions, but the overwhelming majority of the camera’s image targets will be chosen by the public, with the data being processed by them as well. Learn more about JunoCam HERE.

Follow our Juno mission on the web, Facebook, Twitter, YouTube and Tumblr.

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

Juno: Exploring Jupiter’s Intense Radiation

Since 2011, our Juno spacecraft has been heading towards Jupiter, where it will study the gas giant’s atmosphere, aurora, gravity and magnetic field. Along the way, Juno has had to deal with the radiation that permeates space.

All of space is filled with particles, and when these particles get moving at high speeds, they’re called radiation. We study space radiation to better protect spacecraft as they travel through space, as well as to understand how this space environment influences planetary evolution. Once at Jupiter, Juno will have a chance to study one of the most intense radiation environments in our solar system.

Near worlds with magnetic fields – like Earth and Jupiter – these fast-moving particles can get trapped inside the magnetic fields, creating donut-shaped swaths of radiation called radiation belts.

Jupiter’s radiation belts – the glowing areas in the animation below – are especially intense, with particles so energetic that they zip up and down the belts at nearly the speed of light.

Earth also has radiation belts, but they aren’t nearly as intense as Jupiter’s – why? First, Jupiter’s magnetic field is much stronger than Earth’s, meaning that it traps and accelerates faster particles.

Second, while both Earth’s and Jupiter’s radiation belts are populated with particles from space, Jupiter also has a second source of particles – its volcanically active moon Io. Io’s volcanoes constantly release plumes of particles that are energized by Jupiter’s magnetic field. These fast particles get trapped in Jupiter’s radiation belts, making the belts that much stronger and more intense.  

In addition to studying this vast space environment, Juno engineers had to take this intense radiation into consideration when building the spacecraft. The radiation can cause instruments to degrade, interfere with measurements, and can even give the spacecraft itself an electric charge – not good for something with so many sensitive electronics.  

Since we know Jupiter is a harsh radiation environment, we designed Juno with protections in place to keep it safe. Most of Juno’s electronics live inside a half-inch-thick titanium vault, where most of the radiation can’t reach them. We also planned Juno’s orbit to swoop in very close to Jupiter’s surface, underneath the most intense pockets of radiation in Jupiter’s radiation belts.

Juno arrives at Jupiter on July 4th. Throughout its time orbiting the planet, it will send back data on Jupiter’s magnetic field and energetic particles, helping us understand this intense radiation environment better than ever before.

For updates on the Juno mission, follow the spacecraft on Facebook, Twitter, YouTube and Tumblr.

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

Juno: Inside the Spacecraft

Our Juno spacecraft was carefully designed to meet the tough challenges in flying a mission to Jupiter: weak sunlight, extreme temperatures and deadly radiation. Lets take a closer look at Juno:

It Rotates!

Roughly the size of an NBA basketball court, Juno is a spinning spacecraft. Cartwheeling through space makes the spacecraft’s pointing extremely stable and easy to control. While in orbit at Jupiter, the spinning spacecraft sweeps the fields of view of its instruments through space once for each rotation. At three rotations per minute, the instruments’ fields of view sweep across Jupiter about 400 times in the two hours it takes to fly from pole to pole.

It Uses the Power of the Sun

Jupiter’s orbit is five times farther from the sun than Earth’s, so the giant planet receives 25 times less sunlight than Earth. Juno will be the first solar-powered spacecraft we've designed to operate at such a great distance from the sun. Because of this, the surface area of the solar panels required to generate adequate power is quite large.

Three solar panels extend outward from Juno’s hexagonal body, giving the overall spacecraft a span of about 66 feet. Juno benefits from advances in solar cell design with modern cells that are 50% more efficient and radiation tolerant than silicon cells available for space missions 20 years ago. Luckily, the mission’s power needs are modest, with science instruments requiring full power for only about six out of each 11-day orbit.

It Has a Protective Radiation Vault

Juno will avoid Jupiter’s highest radiation regions by approaching over the north, dropping to an altitude below the planet’s radiation belts, and then exiting over the south. To protect sensitive spacecraft electronics, Juno will carry the first radiation shielded electronics vault, a critical feature for enabling sustained exploration in such a heavy radiation environment.

Juno Science Payload:

Gravity Science and Magnetometers – Will study Jupiter’s deep structure by mapping the planet’s gravity field and magnetic field.

Microwave Radiometer – Will probe Jupiter’s deep atmosphere and measure how much water (and hence oxygen) is there.

JEDI, JADE and Waves – These instruments will work to sample electric fields, plasma waves and particles around Jupiter to determine how the magnetic field is connected to the atmosphere, and especially the auroras (northern and southern lights).

JADE and JEDI

Waves

UVS and JIRAM – Using ultraviolet and infrared cameras, these instruments will take images of the atmosphere and auroras, including chemical fingerprints of the gases present.

UVS

JIRAM

JunoCam – Take spectacular close-up, color images.

Follow our Juno mission on the web, Facebook, Twitter, YouTube and Tumblr.

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

Solar System: Things to Know This Week

Earlier this month, Mars was at opposition, which is the point in their orbits when Mars, Earth and the sun all line up, making for good conditions to view the Red Planet from Earth.

Now, it’s Saturn’s turn. The ringed planet will be at opposition on June 3, and this week is a great time to see it — both in the sky as well as up close, thanks to our spacecraft. Here are a few things to know about Saturn exploration this week:

1. Group Portrait

Thanks to their current orbital positions, our sun-observing spacecraft STEREO-A was recently able to capture the sun, Saturn, Mars and Earth in one image. Take a closer look HERE. Discover more about the STEREO mission HERE.

2. Likable, Lick-able Saturn

Saturn’s handsome visage is featured among the new stamps that the US Postal Service is releasing this week to highlight our adventures in planetary exploration.

3. Do You Even Know Saturn?

Yes, yes, it’s the one with the rings. But did you know Saturn has winds that can exceed 1000 miles per hour? Or that its magnetic field is hundreds of times as powerful as the Earth’s? Or that its day is just 10 hours long? How well do you really know the sixth planet?

4. Picking Up Signals

One thing you many not know about the planet is that it’s loud, at least if you listen to its radio signals. When our robotic Cassini spacecraft first approached Saturn, it detected the powerful fields that surround it. Engineers turned those signals into beautiful, eerie sounds. Listen to them HERE.

5.  Not All Who Wander Are Lost

The Cassini mission’s explorations of the Saturn system are very much ongoing. In the next few days, the spacecraft will be touring many locations, including the giant moon Titan, Saturn’s turbulent clouds, the tiny moon Albiorix and more! Get the full itinerary HERE.

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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Earth By The Numbers

Ahhh, Earth. Our home planet and oasis in space. You’re probably very familiar with this world, but here are a few things you may not know about our “Pale Blue Dot” of a planet.

From the vantage point of space, we are able to observe our planet globally using sensitive instruments to understand the delicate balance among its oceans, air, land and life. Satellite observations help study and predict weather, drought, pollution, climate change and many other phenomena that affect the environment, economy and society. 

1. Known to Harbor Life

Of the nine planets, countless asteroids and meteors in our solar system, Earth is the only one known to harbor life. It has a thin layer of atmosphere that separates us from the coldness of space.

2.  All By Its Lonesome

Unlike some other planets in the system that have three or more rings, the Earth has zero, but we do have one lonely moon that orbits us.

3. Moving At The Speed Of Life

Earth is the third planet from the sun and is located about 93,000,000 miles away from it. At this distance, the Earth moves at 66,000 miles per hour through space to complete its 365 day rotation.

4. You Can Breathe Easy

Earth’s atmosphere is 78% nitrogen, 21% oxygen and about 1% other ingredients. Most other planets in our solar system have an atmosphere, but Earth’s is the only one that’s breathable. 

5. For Real?

Did you grow up thinking that each calendar year was 365 days long? It’s actually 365 days, 5 hours, 48 minutes and 56 seconds...in other words, it’s 365.2564 days long. This is why an extra day is add during a leap year: to help offset this time difference. 

6. Far Out

We measure the distance of planets in our solar system in a measurement known as an Astronomical Unit, or AU. This measurement is based on the distance of the Earth from the sun. Earth is one AU from the sun, while Mars is 1.52 AU and Jupiter is 5.2 AU.

7. Taking Selfies...Before It Was Cool

The first ever photo of Earth was captured on October 24, 1946 when a V-2 test rocket was launched into space from New Mexico.

8. Slumped Over Already

The Earth doesn’t sit upright like you would think. It’s actually sitting on its side a bit, or rotational axis as it’s called, the Earth sits at a 23.45 degree rotational axis spin.

9. How Original...

How did it get the name Earth? The name “Earth” is at least 1,000 years old. All the planets in our system are named after Greek and Roman gods and goddesses, except for Earth. The name itself is of English and German origin and simply means “ground”.

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Fun Facts About Mars

Mars is a cold desert world, and is the fourth planet from the sun. It is half the diameter of Earth and has the same amount of dry land. Like Earth, Mars has seasons, polar ice caps, volcanoes, canyons and weather, but its atmosphere is too thin for liquid water to exist for long on the surface. There are signs of ancient floods on the Red Planet, but evidence for water now exists mainly in icy soil and thin clouds.

Earth has one, Mars has two…moons of course! Phobos (fear) and Deimos (panic) are the Red Planet’s two small moons. They are named after the horses that pulled the chariot of the Greek war god Ares, the counterpart to the Roman war god Mars.

The diameter of Mars is 4220 miles (6792 km). That means that the Red Planet is twice as big as the moon, but the Earth is twice as big as Mars.

Since Mars has less gravity than Earth, you would weigh 62% less than you do here on our home planet. Weigh yourself here on the Planets App. What’s the heaviest thing you’ve ever lifted? On Mars, you could have lifted more than twice that! Every 10 pounds on Earth only equals 4 pounds on the Red Planet. Find out why HERE.

Mass is the measurement of the amount of matter something contains. Mars is about 1/10th of the mass of Earth.

Mars and Earth are at their closest point to each other about every two years, with a distance of about 33 million miles between them at that time. The farthest that the Earth and Mars can be apart is: 249 million miles. This is due to the fact that both Mars and Earth have elliptical orbits and Mars’ orbit is tilted in comparison with the Earth’s. They also orbit the sun at different rates.

The temperature on Mars can be as high as 70 degrees Fahrenheit (20 degrees Celsius) or as low as about –225 degrees Fahrenheit (-153 degrees Celsius). How hot or cold the surface varies between day and night and among seasons. Mars is colder than Earth because it is farther from the sun.

You know that onions have layers, but did you know that Mars has layers too? Like Earth, Mars has a crust, a mantle and a core. The same stuff even makes up the planet layers: iron and silicate.

Ever wonder why it’s so hard launching things to space? It’s because the Earth has a log of gravity! Gravity makes things have weight, and the greater the gravity, the more it weights. On Mars, things weigh less because the gravity isn’t as strong.

Take a deep breath. What do you think you just breathed in? Mostly Nitrogen, about a fifth of that breath was Oxygen and the rest was a mix of other gases. To get the same amount of oxygen from one Earth breath, you’d have to take around 14,500 breaths on Mars! With the atmosphere being 100 times less dense, and being mostly carbon dioxide, there’s not a whole lot of oxygen to breathe in.

Mars has about 15% of Earth’s volume. To fill Earth’s volume, it would take over 6 Mars’ volumes.

For more fun Mars facts, visit HERE.

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How Well Do You Know Venus?

Similar in structure and size to Earth, Venus’ thick, toxic atmosphere traps heat in a runaway greenhouse effect. A permanent layer of clouds traps heat, creating surface temperatures hot enough to melt lead.

How did Venus get its name? It is named for the ancient Roman goddess of love and beauty. It is believed that Venus was named for the most beautiful of the ancient gods because it shone the brightest of the five planets known to ancient astronomers.

Here are a few fun facts that you might not know:

One day on Venus lasts as long as 243 Earth days (aka the time it takes for Venus to rotate or spin once)

Venus is a rocky planet, also known as a terrestrial planet

Venus’ thick and toxic atmosphere is made up mostly of carbon dioxide and nitrogen, with clouds of sulfuric acid droplets

Venus has no moons or rings

More than 40 spacecraft have explored the planet

No evidence of life has been found on Venus. The planet’s extreme high temperatures of almost 480 degrees Celsius (900 degrees Fahrenheit) makes it seem an unlikely place for life as we know it

Venus spins backwards when compared to the other planets. This means that the sun rises in the west and sets in the east

Night Light

Did you know that Venus is the brightest planet in Earth’s dark skies? Only the moon — which is not a planet — is brighter. Venus outshines the other planets because it is closer and its thick cloud cover is excellent at reflecting sunlight.

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10 Intriguing Worlds Beyond Our Solar System

In celebration of the 20th anniversary of the first confirmed planet around a sun-like star, a collection of some interesting exoplanets has been put together. Some of these are rocky, some are gaseous and some are very, very cold. But there’s one thing each these strange new worlds have in common: All have advanced scientific understanding of our place in the cosmos. Check out these 10 exoplanets, along with artist’s concepts depicting what they might look like. For an extended list of 20 exoplanets, go HERE. 

1. Kepler-186f

Kepler-186f was the first rocky planet to be found within the habitable zone -- the region around the host star where the temperature is right for liquid water. This planet is also very close in size to Earth. Even though we may not find out what’s going on at the surface of this planet anytime soon, it’s a strong reminder of why new technologies are being developed that will enable scientists to get a closer look at distance worlds. 

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2. HD 209458 b (nickname “Osiris”)

The first planet to be seen in transit (crossing its star) and the first planet to have it light directly detected. The HD 209458 b transit discovery showed that transit observations were feasible and opened up an entire new realm of exoplanet characterization.

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3. Kepler-11 system

This was the first compact solar system discovered by Kepler, and it revealed that a system can be tightly packed, with at least five planets within the orbit of Mercury, and still be stable. It touched off a whole new look into planet formation ideas and suggested that multiple small planet systems, like ours, may be common.

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4. Kepler-16b

A real-life "Tatooine," this planet was Kepler's first discovery of a planet that orbits two stars -- what is known as a circumbinary planet.

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5. 51 Pegasi b

This giant planet, which is about half the mass of Jupiter and orbits its star every four days, was the first confirmed exoplanet around a sun-like star, a discovery that launched a whole new field of exploration.

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6. CoRoT 7b

The first super-Earth identified as a rocky exoplanet, this planet proved that worlds like the Earth were indeed possible and that the search for potentially habitable worlds (rocky planets in the habitable zone) might be fruitful.

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7. Kepler-22b

A planet in the habitable zone and a possible water-world planet unlike any seen in our solar system.

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8. Kepler-10b

Kepler's first rocky planet discovery is a scorched, Earth-size world that scientists believe may have a lava ocean on its surface.

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9. Kepler-444 system

The oldest known planetary system has five terrestrial-sized planets, all in orbital resonance. This weird group showed that solar systems have formed and lived in our galaxy for nearly its entire existence.

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10. 55 Cancri e

Sauna anyone? 55 Cancri e is a toasty world that rushes around its star every 18 hours. It orbits so closely -- about 25 times closer than Mercury is to our sun -- that it is tidally locked with one face forever blistering under the heat of its sun. The planet is proposed to have a rocky core surrounded by a layer of water in a “supercritical” state, where it is both liquid and gas, and then the whole planet is thought to be topped by a blanket of steam. 

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