What Dose It Feel Like Being Inside A Space Suit?

solivanas: I’ve been designing a space habitat for school that rotates to provide gravity for astronauts within it. Any tips?

Solar System: 2015 Year in Review

Two mysterious worlds explored for the first time. Liquid water seen flowing on Mars. A global ocean discovered hiding inside a moon of Saturn. Even during our Era of audacious solar system exploration, 2015 stands out. Here are a few highlights:

1. New Horizons Reveals the Face of Pluto

Whether or not you call it a planet, Pluto entranced the people of Earth when it sent a love note from three billion miles away via our New Horizons spacecraft.

2. Dawn Comes to Ceres

The dwarf planet Ceres, the largest object in the main asteroid belt, teased explorers with its bizarre bright spots before finally giving up some of its secrets to the Dawn spacecraft. HERE are the latest findings.

3. Cassini Marks Discoveries and Milestones at Enceladus

When the Cassini spacecraft performs its final close flyby of Saturn’s icy moon Enceladus on Dec. 19, it will be a true milestone. Scientists using data from Cassini’s instruments have uncovered astounding secrets about this small moon, including (confirmed this year) the fact that its underground ocean of liquid water is global, and is home to hydrothermal vents.

4. We Confirmed Evidence that Liquid Water Flows on Today’s Mars

Findings from our Mars Reconnaissance Orbiter (MRO) provided the strongest evidence yet that liquid water flows intermittently — on present-day Mars.

5. Rosetta Passes Perihelion

The European Space Agency’s Rosetta mission had a remarkable year, re-establishing contact with the Philae lander and following comet 67P/Churyumov-Gerasimenko as it swung near the sun.

6. Mars Explorers Confirm Lakes Once Dotted Mars

A study from the team behind our Mars Science Laboratory/Curiosity Rover confirmed that Mars was once, billions of years ago, capable of storing water in lakes over an extended period of time.

7. MAVEN Finds a Culprit in the Loss of Mars’ Atmosphere

The Mars Atmosphere and Volatile Evolution (MAVEN) mission identified the process that appears to have played a key role in the transition of the Martian climate from an early, warm and wet environment that might have supported surface life to the cold, arid planet that Mars is today.

8. Akatsuki Gets a Second Chance at Venus

Five years after a mishap sent the spacecraft off course, the Japan Aerospace Exploration Agency (JAXA) successfully inserted the Venus Climate Orbiter “Akatsuki” into orbit around Venus. While the mission is not funded by NASA, an agency partnership with JAXA provides an opportunity for eight of our scientists to work with the Akatsuki team and study data from the spacecraft over the next year or so.

9. A Trailblazing Mission Sends Its Final Message from Mercury

After a flight of nearly 11 years, the highly successful MESSENGER mission ended when, as planned, the spacecraft slammed into the surface of Mercury.

10. Mars Reconnaissance Orbiter Completes 40,000 Orbits

Mars Reconnaissance Orbiter, at Mars since 2006, has orbited the Red Planet more than 40,000 times. The mission, which studies the whole planet from space, has shown that Mars is diverse and dynamic by way of many thousands of spectacular images and other kinds of data.

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Seeing Saharan Dust from Space

Last year, Godzilla made its way across the Atlantic Ocean. No, it wasn’t a giant lizard monster, but a cloud of dust so large it could be seen from a million miles away in space.

The plume of dust blowing from the Sahara Desert broke records and was nicknamed the “Godzilla plume.”

This year, another massive dust plume is traveling across the Atlantic.

The transport of dust from the Sahara to the Americas isn’t unusual: every year, winds pick up more than 180 million tons of dust particles from the Sahara Desert, move them over the African continent and carry them all the way across the Atlantic Ocean, depositing much of the dust along the way.

What’s remarkable about the past two years is the size of the plumes. Last year, the “Godzilla plume” was the largest dust storm in our two decades of observations.

Although this year’s plume has yet to complete its journey across the Atlantic, dust plumes from the Sahara often have important impacts on the Americas.

So, why do the dust plumes matter?

Before the Sahara was a desert, it was a lakebed, where nutrients like phosphorous and iron were deposited before the lake dried up. As a result, winds pick up these nutrients in the dust plumes. Some of these nutrients get deposited in the Atlantic Ocean, feeding marine life – iron, for example, is critical for marine life. Phosphorus is also a much-needed nutrient that fertilizes vegetation in the Amazon rainforest. The amount of phosphorus deposited by Saharan dust plumes into the Amazon every year – around 22,000 tons – is roughly equivalent to the amount that gets removed from the rainforest’s soil by weather conditions. In other words, long term, the dust plumes provide an essential nutrient to the Amazon’s vegetation.

Both the dust plumes themselves and the conditions associated with them can also influence the formation of tropical storms during hurricane season. As climate change appears to be strengthening the strongest storms, understanding the relationship between dust plumes and hurricanes has only grown more important.

The dust plumes can carry microbes that can be deadly and can worsen air quality, creating potentially dangerous conditions for sensitive populations. The iron in the plumes can also kick off blooms of toxic algae off the coast of Florida that result from the increase in nutrients in the ocean.

What comes next for Saharan dust? We’re still looking into it!

Some research suggests dust plumes will intensify with higher temperatures and dryer conditions, creating more loose dust to be picked up. However, other research shows that rising ocean temperatures and changing wind speeds would result in more rainfall and vegetation in the desert, reducing how much dust blows across the Atlantic. Make sure to follow us on Tumblr for your regular dose of space!

Meet Fermi: Our Eyes on the Gamma-Ray Sky

Black holes, cosmic rays, neutron stars and even new kinds of physics — for 10 years, data from our Fermi Gamma-ray Space Telescope have helped unravel some of the biggest mysteries of the cosmos. And Fermi is far from finished!

On June 11, 2008, at Cape Canaveral in Florida, the countdown started for Fermi, which was called the Gamma-ray Large Area Space Telescope (GLAST) at the time. 

The telescope was renamed after launch to honor Enrico Fermi, an Italian-American pioneer in high-energy physics who also helped develop the first nuclear reactor. 

Fermi has had many other things named after him, like Fermi’s Paradox, the Fermi National Accelerator Laboratory, the Enrico Fermi Nuclear Generating Station, the Enrico Fermi Institute, and the synthetic element fermium.

Photo courtesy of Argonne National Laboratory

The Fermi telescope measures some of the highest energy bursts of light in the universe; watching the sky to help scientists answer all sorts of questions about some of the most powerful objects in the universe. 

Its main instrument is the Large Area Telescope (LAT), which can view 20% of the sky at a time and makes a new image of the whole gamma-ray sky every three hours. Fermi’s other instrument is the Gamma-ray Burst Monitor. It sees even more of the sky at lower energies and is designed to detect brief flashes of gamma-rays from the cosmos and Earth.

This sky map below is from 2013 and shows all of the high energy gamma rays observed by the LAT during Fermi’s first five years in space.  The bright glowing band along the map’s center is our own Milky Way galaxy!

So what are gamma rays? 

Well, they’re a form of light. But light with so much energy and with such short wavelengths that we can’t see them with the naked eye. Gamma rays require a ton of energy to produce — from things like subatomic particles (such as protons) smashing into each other. 

Here on Earth, you can get them in nuclear reactors and lightning strikes. Here’s a glimpse of the Seattle skyline if you could pop on a pair of gamma-ray goggles. That purple streak? That’s still the Milky Way, which is consistently the brightest source of gamma rays in our sky.

In space, you find that kind of energy in places like black holes and neutron stars. The raindrop-looking animation below shows a big flare of gamma rays that Fermi spotted coming from something called a blazar, which is a kind of quasar, which is different from a pulsar... actually, let’s back this up a little bit.

One of the sources of gamma rays that Fermi spots are pulsars. Pulsars are a kind of neutron star, which is a kind of star that used to be a lot bigger, but collapsed into something that’s smaller and a lot denser. Pulsars send out beams of gamma rays. But the thing about pulsars is that they rotate. 

So Fermi only sees a beam of gamma rays from a pulsar when it’s pointed towards Earth. Kind of like how you only periodically see the beam from a lighthouse. These flashes of light are very regular. You could almost set your watch by them!

Quasars are supermassive black holes surrounded by disks of gas. As the gas falls into the black hole, it releases massive amount of energy, including — you guessed it — gamma rays. Blazars are quasars that send out beams of gamma rays and other forms of light — right in our direction. 

When Fermi sees them, it’s basically looking straight down this tunnel of light, almost all the way back to the black hole. This means we can learn about the kinds of conditions in that environment when the rays were emitted. Fermi has found about 5,500 individual sources of gamma rays, and the bulk of them have been blazars, which is pretty nifty.

But gamma rays also have many other sources. We’ve seen them coming from supernovas where stars die and from star factories where stars are born. They’re created in lightning storms here on Earth, and our own Sun can toss them out in solar flares. 

Gamma rays were in the news last year because of something Fermi spotted at almost the same time as the National Science Foundation (NSF)’s Laser Interferometer Gravitational-Wave Observatory (LIGO) and European Gravitational Observatory’s Virgo on August 17, 2017. Fermi, LIGO, Virgo, and numerous other observatories spotted the merger of two neutron stars. It was the first time that gravitational waves and light were confirmed to come from the same source.

Fermi has been looking at the sky for almost 10 years now, and it’s helped scientists advance our understanding of the universe in many ways. And the longer it looks, the more we’ll learn. Discover more about how we’ll be celebrating Fermi’s achievements all year.

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Have you seen any eclipse in your life?

I saw a partial eclipse once, I think back in middle school (not sure I want to check the date as that would remind me how old I am...). I’m really looking forward to Monday, and then 2024  and 2045 which will be the next couple of times we have totality in the continental US. 

Space Station Research: Observing Earth

Each month, we highlight a different research topic on the International Space Station. In April, our focus is how the space station provides a platform for studying the Earth.

You might wonder how a laboratory 250 miles above Earth could help us study and observe our home planet, but the space station actually gives us a unique view of the blue marble we call home.

The space station is part of a fleet of Earth remote-sensing platforms to develop a scientific understanding of Earth’s systems and its response to natural or human-induced changes and to improve prediction of climate, weather and natural hazards. Unlike automated remote-sensing platforms, the space station has a human crew, a low-orbit altitude and orbital parameters that provide variable views and lighting. Crew members have the ability to collect unscheduled data of an unfolding event, like severe weather, using handheld digital cameras.

The Cupola, seen above, is one of the many ways astronauts aboard the space station are able to observe the Earth. This panoramic control tower allows crew members to view and guide operations outside the station, like the station’s robotic arm.

The space station also has an inclined, sun-asynchronous orbit, which means that it travels over 90% of the inhabited surface of the Earth, and allows for the station to pass over ground locations at different times of the day and night. This perspective is different and complimentary to other orbiting satellites.

The space station is also home to a few Earth-observing instruments, including:

The ISS-RapidScat monitors ocean winds for climate research, weather prediction and hurricane science. This vantage point gives scientists the first near-global direct observations of how ocean winds can vary over the course of the day, while adding extra eyes in the tropics and mid-latitudes to track the formation and movement of tropical cyclones.

CATS (Cloud-Aerosol Transport System) is a laser instrument that measures clouds and airborne particles such as pollution, mineral dust and smoke. Improving cloud data allows scientists to create more accurate climate models, which in turn, will improve air quality forecasts and health risk alerts.

In late 2016, we will launch Stratospheric Aerosol and Gas Experiment III (SAGE III). This experiment will measure ozone and other gases in the atmosphere to help scientists assess how the ozone layer is recovering.

Want to observe the Earth from a similar vantage point? You can thanks to our High Definition Earth-Viewing System (HDEV). This experiment is mounted on the exterior of the space station and includes several commercial HD video cameras aimed at the Earth.

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what has nasa and jpl learned from opportunity that has helped with developing this new project?

It’s a U.S. Record! Cumulative Days in Space: 383

Today, Astronaut Scott Kelly has broken the record for longest time spent in space by a U.S. astronaut! Over the course of his four missions, Kelly has spent 383 cumulative days in space. This record was previously held by Astronaut Mike Fincke, with 382 days in space over three flights. Here are some more fun facts about this milestone:

4: The number of humans that have spent a year or more in orbit on a single mission

215 Days: The record currently held by Mike Lopez-Alegria for most time on a single spaceflight by U.S. astronaut. On Oct. 29, Kelly will break this record

377 Days: The current record for most days in space by a U.S. female astronaut, held by Peggy Whitson

879 Days: The record for most cumulative days in space by a human, currently held by Russian cosmonaut Gennady Padalka

Why Spend a Year in Space?

Kelly’s One-Year Mission is an important stepping stone on our journey to Mars and other deep space destinations. These investigations are expected to yield beneficial knowledge on the medical, psychological and biomedical challenges faced by astronauts during long-duration spaceflight.

Kelly is also involved in the Twins Study, which consists of ten separate investigations that are being conducted with his twin brother, who is on Earth. Since we are able to study two individuals who have the same genetics, but are in different environments for one year, we can gain a broader insight into the subtle effects and changes that may occur in spaceflight.

For regular updates on Kelly’s one-year mission aboard the space station, follow him on social media: Facebook, Twitter, Instagram.

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That’s a wrap! Thank you all very much for the wonderful questions.


We’re so excited to send Perseverance off on her journey to Mars, and we will be launching on July 30 at 7:50 a.m. EDT from Kennedy Space Center in Florida. 


If today’s Answer Time got you excited, team up with us to #CoutdownToMars! We created a virtual Mars photo booth, 3D rover experience and more for you to put your own creative touch on sending Perseverance well wishes for her launch to the Red Planet! View them all, HERE. 


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What do you do on a daily basis?