10 Things: How To Photograph A Meteor Shower

Taking the Vital Signs of Mars

Does Mars have quakes? What is the temperature of the Red Planet? How did Mars even form? What can it tell us about how other rocky planets formed?

The Mars InSight lander is scheduled to launch in May 2018 to search for the answers to those questions.

InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) will conduct the first thorough “check-up” of Mars in more than 4.5 billion years, measuring its “pulse”, or seismic activity; its temperature; and its “reflexes” (the way the planet wobbles when it is pulled by the Sun and its moons).

How and Why?

By using sophisticated instruments – tools that can measure the vital signs of a planet – InSight will delve deep beneath the surface of Mars, detecting the clues left by the earliest stages of planetary formation.  

Previous Mars missions have explored the surface history of the Red Planet. Mars has been less geologically active than Earth, so it retains a more complete record of its history in its core, mantle and crust. InSight will study the sizes, densities and overall structure of the Red Planet’s core, mantle and crust. 

The lander will also measure the rate at which heat escapes from the planet’s interior, and provide glimpses into the evolutionary processes of all the rocky planets in our solar system, including Earth, and even those circling other stars!

Send Your Name to Mars!

You can send your name to Mars onboard the InSight lander! The deadline to get your Martian boarding pass is Nov. 1. To submit your name, visit: mars.nasa.gov/syn/insight

Learn more about Mars InSight HERE.

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Solar System: Things to Know This Week

Our solar system is huge, let us break it down for you. Here are a few things to know this week:

1. The New New Horizons

Seven months after the  Pluto flyby, information and discoveries continue to flow from the New Horizons mission, as the spacecraft transmits more and more data to scientists on Earth.

2. A Longlasting Dawn

The Dawn orbiter is in good health as it carries out the ongoing reconnaissance of the dwarf planet Ceres, which is revealing some spectacular and mysterious landscapes.

3. Storm Watch: Saturn

This week the Cassini spacecraft will be watching for storms in Saturn’s turbulent atmosphere. On March 6, it will spend about 14 hours acquiring a movie of the narrow, braided F ring. Check out some past photos of Saturnian storms HERE.

4. The Next Flight to Mars Departs Soon

The ExoMars 2016 mission, a joint endeavor between the European Space Agency and the Russian space agency Roscosmos, is set to lift off in March. The 2016 mission consists of the Trace Gas Orbiter and the Schiaparelli Entry, Descent and Landing Demonstrator Module. We’re supplying some of the technology that will fly aboard the orbiter. In 2018, the ExoMars rover is slated to follow.

5. Early Encounter with a Comet

As we continue to marvel at the latest images from Rosetta, this week is a good time to remember the 30th anniversary of the Vega 1 Comet Halley flyby. This Russian spacecraft dropped off a balloon probe at Venus before continuing on to the comet, which is photographed and examined at close range by flying through its coma.

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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What are Perseid Meteors, and why should you be excited for them this year? Let us tell you!

The Perseid meteor shower is caused by debris from Comet Swift-Tuttle as it swings through the inner solar system and ejects a trail of dust and gravel along its orbit. When the Earth passes through the debris, specs of comet-stuff hit the atmosphere at 140,000 mph and disintegrate in flashes of light. Meteors from this comet are called Perseids because they seem to fly out of the constellation Perseus.

Last year, this meteor shower peaked during a bright “supermoon”, so visibility was reduced. Luckily, forecasters say the show could be especially awesome this year because the Moon is nearly new when the shower peaks on Aug. 12-13.

The best place to view the event is away from city lights around midnight. Under a clear, dark sky forecasters predict meteor rates as high as 100 per hour on peak night. So, get outside, look up and enjoy the show!

If your area has poor visibility on the peak night, we’ve got you covered! We’ll be hosting a live broadcast about the meteor shower from 10 p.m. EDT Wednesday, Aug. 12, to 2 a.m. Thursday, Aug. 13. In addition to footage from our live skycam, the program will highlight the science behind the Perseids, as well as our research related to meteors and comets. Tune in on NASA TV or our UStream Channel.

Have you ever had to troubleshoot a problem in space?

Hi!! I’m a high school sophomore and I love the work NASA does! I’ve always wondered, what’s an astronaut’s first thought when leaving earth? What kind of experiences do you leave the expedition with? Thanks! :) - Lauren

Ready for a virtual adventure through the Orion Nebula?

Suspended in space, the stars that reside in the Orion Nebula are scattered throughout a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that are reminiscent of the Grand Canyon. This visualization uses visible and infrared views, combining images from the Hubble Space Telescope and the Spitzer Space Telescope to create a three-dimensional visualization.

Learn more about Hubble’s celebration of Nebula November and see new nebula images, here.

You can also keep up with Hubble on Twitter, Instagram, Facebook, and Flickr!

Visualization credits: NASA, ESA, and F. Summers, G. Bacon, Z. Levay, J. DePasquale, L. Hustak, L. Frattare, M. Robberto, M. Gennaro (STScI), R. Hurt (Caltech/IPAC), M. Kornmesser (ESA); Acknowledgement: A. Fujii, R. Gendler

How Will We Safely Send the First Humans to the Red Planet?

We’ve been exploring the Red Planet for over 50 years -- Mariner 4 launched on this day (Nov. 28) in 1964 and took the first photos of Mars from space the following summer.

We first explored the surface 40 years ago (Viking, 1976) and have had a continuous scientific presence on Mars for nearly 20 years, starting with the landing of the Pathfinder lander and Sojourner rover on July 4, 1997.

We currently have three orbiters – MAVEN, MRO and Mars Odyssey – and two rovers – Curiosity and Opportunity – actively exploring Mars.

These robotic explorers have already taught us a lot about the Red Planet, and future missions will teach us even more about how humans can live and work on the surface.

After sending humans on space exploration missions for the last 50 years, we have gained the experience and knowledge to send the first people to Mars. We are working across all areas to prepare for that historic day and want to share our progress with you. 

Building the ride to Mars: NASA’s Space Launch System.

Our ride to Mars, the Space Launch System, is being built right now to meet the challenges of exploring deep space. When it comes to our journey to Mars and beyond, there are no small steps. Our video series by the same name breaks down those steps to show how SLS will send missions to the Red Planet.

Living on the Space Station will help humans live safely on Mars.

New crew members of Expedition 50 will soon conduct more than 250 experiments on the International Space Station. More than 2,000 experiments have already been done! 

Experiments in fields such as biology, Earth science, physical sciences and human research are helping us unlock the knowledge needed to enable humans to live in space for long durations. If you missed the recent launch, check out NASA TV for a replay.

Testing Orion helps crew live and work in space and get home safely.

Scheduled to launch atop the Space Launch System rocket for the first time in 2018, an uncrewed Orion will travel farther into space than any spacecraft built for humans has ever gone before. When Orion returns to Earth, splashing down into the Pacific Ocean, it will take a landing and recovery group to safely return the capsule and crew back to land. A variety of testing on the ground, including to structures and parachutes, is helping make sure Orion can safely carry crew to new destinations in the solar system.

In late October, this recovery group, including NASA’s Ground Systems Development and Operations Program, the U.S. Navy, U.S. Air Force and contractor employees, completed its fifth successful practice run to recover Orion aboard the USS San Diego. 

We're using high resolution imagery from the Mars Reconnaissance Orbiter to learn more about potential landing sites for a human mission.

Who knows what surprises the Red Planet holds?

Our Curiosity Rover has discovered all kinds of interesting Mars features including meteorites. How do you learn more about a meteorite? Zap it with lasers, of course.

This golf-ball-sized, iron-nickel meteorite was recently found on Mars where ancient lakebed environments once existed. Named “Egg Rock” for the area in which it was found, it is the first meteorite to be examined using a laser-firing spectrometer.

By studying the conditions on Mars with vehicles like Curiosity, scientists are able to help prepare future astronauts to live on Mars.

How do you prepare the tallest rocket ever built for its first launch?

Another important component in successfully launching the Space Launch System rocket and Orion spacecraft on a Journey to Mars is the infrastructure work being done by our Ground Systems Development and Operations Program at Kennedy Space Center.

While efforts at our Vehicle Assembly Building continue, we hope you’ll be making your plans to join us at the launch pad for the first flight of SLS with Orion in 2018!

Preparing for a human journey to Mars

The next Mars rover will launch in 2020, and will investigate a region of Mars where the ancient environment may have been favorable for microbial life, probing the Martian rocks for evidence of past life. 

It will collect samples and cache them on the surface for potential return to Earth by a future mission. Mars 2020 will also conduct the first investigation into the usability and availability of Martian resources, including oxygen, in preparation for human missions.

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Record Number of Americans Apply to #BeAnAstronaut

On Dec. 14, 2015, we announced that astronaut applications were open on USAJOBS. The window for applications closed on Feb. 18. We’re happy to announce that we have received more than 18,300 applications from excited individuals from around the country, all hoping to join the 2017 astronaut class. This surpasses the more than 6,100 received in 2012 for the most recent astronaut class, and the previous record - 8,000 applicants in 1978. 

So you applied to be an astronaut...now what?

Since the applications closed on Feb. 18, many people are curious to know…what’s next? Let us help you navigate the selection process:

Now that we have received all the applications, we will review them to determine the “Highly Qualified” applicants. This process will take place through summer 2016.

What is a “Highly Qualified” Applicant?

The diversity of experiences is what separates the highly qualified from qualified. Experience that demonstrates good leadership, fellowship and decision making are beneficial.

Between fall 2016 and spring 2017, interviewees will be brought to Johnson Space Center for evaluation. This process will help us determine the finalists, which takes place in spring 2017. 

Finally, in summer 2017, the Astronaut Candidate Class of 2017 is announced! These candidates will report to Johnson Space Center starting in August 2017. 

To view the full astronaut candidate selection process timeline, visit: http://astronauts.nasa.gov/content/timeline.htm

*Note that the high volume of applications received, dates in the timeline could be adjusted. 

Why do we need more astronauts?

We are continuing human spaceflight on the International Space Station, which has a continuous crew of six people on board. The Boeing and SpaceX commercial crew spacecraft that will travel to the station both have seats for four astronauts (the current Soyuz spacecraft, on which astronauts travel, only has three). This will add a seventh astronaut to the orbiting laboratory, and enable us to do more science!

How many astronauts will be selected?

The exact number will be determined by mission requirements, but current analysis shows about 8 - 14 astronauts will be needed. The final number will depend on updates to program plans, budgets, etc. 

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Observing the Ozone Hole from Space: A Science Success Story

Using our unique ability to view Earth from space, we are working together with NOAA to monitor an emerging success story – the shrinking ozone hole over Antarctica.

Thirty years ago, the nations of the world agreed to the landmark ‘Montreal Protocol on Substances that Deplete the Ozone Layer.’ The Protocol limited the release of ozone-depleting chlorofluorocarbons (CFCs) into the atmosphere.

Since the 1960s our scientists have worked with NOAA researchers to study the ozone layer. 

We use a combination of satellite, aircraft and balloon measurements of the atmosphere.

The ozone layer acts like a sunscreen for Earth, blocking harmful ultraviolet, or UV, rays emitted by the Sun.

In 1985, scientists first reported a hole forming in the ozone layer over Antarctica. It formed over Antarctica because the Earth’s atmospheric circulation traps air over Antarctica.  This air contains chlorine released from the CFCs and thus it rapidly depletes the ozone.

Because colder temperatures speed up the process of CFCs breaking up and releasing chlorine more quickly, the ozone hole fluctuates with temperature. The hole shrinks during the warmer summer months and grows larger during the southern winter. In September 2006, the ozone hole reached a record large extent.

But things have been improving in the 30 years since the Montreal Protocol. Thanks to the agreement, the concentration of CFCs in the atmosphere has been decreasing, and the ozone hole maximum has been smaller since 2006’s record.

That being said, the ozone hole still exists and fluctuates depending on temperature because CFCs have very long lifetimes. So, they still exist in our atmosphere and continue to deplete the ozone layer.

To get a view of what the ozone hole would have looked like if the world had not come to the agreement to limit CFCs, our scientists developed computer models. These show that by 2065, much of Earth would have had almost no ozone layer at all.

Luckily, the Montreal Protocol exists, and we’ve managed to save our protective ozone layer. Looking into the future, our scientists project that by 2065, the ozone hole will have returned to the same size it was thirty years ago.

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Laying the Groundwork for a New Generation of Commercial Supersonic Aircraft

Cabin crew, prepare for takeoff. Engines roar; speed increases. You sip a cold beverage as the aircraft accelerates quietly past Mach 1 or around 600 mph. There’s no indication you’re flying over land faster than the speed of sound except when you glance at your watch upon arrival and see you’ve reached your destination in half the time. You leisurely walk off the plane with ample time to explore, finish a final report or visit a familiar face. This reality is closer than you think.

We’re on a mission to help you get to where you want to go in half the time. Using our single-pilot X-59 Quiet SuperSonic Technology (QueSST) research aircraft, we will provide rule-makers the data needed to lift current bans on faster-than-sound air travel over land and help enable a new generation of commercial supersonic aircraft.

The X-59 QueSST is unique in shape. Each element of the aircraft’s design will help reduce a loud sonic boom, typically produced by conventional supersonic aircraft, to a gentle sonic thump, making it quieter for people on the ground. To prove the quiet technology works, we will fly the X-59 over select U.S. communities to gauge the public’s response to the sound.

We are working with Lockheed Martin in Palmdale, California, to manufacture the X-59 and are making significant progress, despite the pandemic.

We finished the majority of work on the wing and closed its interior, marking the halfway point on construction of the aircraft. 

The X-59 team at Lockheed Martin completed the final touches by fastening skins to the wing. A special sealant is applied so that fuel can be carried in the wings of the aircraft.

Moving at a steady pace, technicians continue to work on many parts of the aircraft simultaneously. The forebody section of the aircraft will carry the pilot and all the avionics needed to fly the aircraft.

Because of the X-59’s long nose, the pilot will rely on an eXternal Vision System (XVS), rather than a window, for forward-facing visibility. The XVS will display fused images from an advanced computing system and cameras mounted on the upper and lower part of the aircraft’s nose.

The aft part of the aircraft will hold an F414 GE engine and other critical systems. Unlike typical aircraft, the engine inlet will be located on the upper surface of the X-59 and is one of many features that will help reduce the noise heard on the ground.

Over the next several months, the team will merge all three sections together. After final assembly in 2021, the X-59 will undergo numerous tests to ensure structural integrity of the aircraft and that ¬its components work properly. First flight of the aircraft will be in 2022 and community testing will start in 2024, making way for a new market of quiet commercial supersonic aircraft.

Want to learn more about the X-59 and our mission? Visit nasa.gov/X59. 

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