How Does A Microgravity Garden Grow When There's No Up Or Down? An Advanced Chamber, About The Size Of

What is the most fascinating thing about black hole research for you, personally?

We’re sending people to space this week 🚀 Here’s your chance to ask a past Flight Director in Mission Control your questions!

Ginger Kerrick will be taking your questions in an Answer Time session on Friday, September 27 from 12pm - 1 pm ET here on NASA’s Tumblr! Ginger served as a Flight Director in Mission Control for 11 years and is now the Flight Integration Division Chief at Johnson Space Center. Find out what it’s like to send humans to space and learn more about her position as our first female Hispanic flight director. Make sure to ask your question now by visiting http://nasa.tumblr.com/ask!

Ginger Kerrick, as a child, dreamed of growing up to be either a basketball player or an astronaut. When neither dream came to fruition, Kerrick developed a fresh perspective – best summed up by the phrase “It just wasn’t meant to be” – and later became part of our team, serving in the Mission Control Center at the NASA Johnson Space Center as a Flight Director who has, to date, supported 13 International Space Station and five joint space shuttle missions. It was there that Kerrick, a few years earlier, became the first non-astronaut Capsule Communicator (CapCom), the flight controller that speaks directly to the astronaut crew in space, on behalf of the rest of the Mission Control team. 

Today, Ginger Kerrick is the Flight Integration Division Chief at our Johnson Space Center. Her department is responsible for crew safety and training, among a list of other duties. She has worked for NASA since 1994, and interned here while she was earning a bachelor’s degree in physics from Texas Tech University. She also has a master’s degree in physics from the university.

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

Tools of the Trade: How Parker Solar Probe Will Study the Sun

Our Parker Solar Probe will get closer to the Sun than any spacecraft has ever gone – it will fly right through the Sun's corona, part of the Sun's atmosphere.

This spacecraft is full of cutting-edge technology, from its heat shield down to its guidance and control systems. It also carries four suites of advanced instruments designed to study the Sun in a multitude of ways.  

1. Measuring particles

Two of Parker Solar Probe's instrument suites are focused on measuring particles – electrons and ions – within the corona.

One of these particle-measuring instrument suites is SWEAP (Solar Wind Electrons Alphas and Protons). SWEAP counts the most common particles in the solar wind – the Sun's constant outflow of material – and measures their properties, like velocity, density and temperature. Gathering this information about solar wind particles will help scientists better understand why the solar wind reaches supersonic speeds and exactly which part of the Sun the particles come from.

One instrument in the SWEAP suite is the Solar Probe Cup. Most of the instruments on Parker Solar Probe stay safe and cool in the shadow of the heat shield, but the Solar Probe Cup is one of the few that sticks out. That's so it can capture and measure particles streaming straight out from the Sun, and it had to go through some intense testing to get ready for this position in the Sun's incredibly hot corona.  

Credit: Levi Hutmacher/Michigan Engineering

The ISʘIS suite (pronounced EE-sis, and including the symbol for the Sun in its acronym) also measures particles. ISʘIS is short for Integrated Science Investigation of the Sun, and this instrument suite measures particles that move faster – and therefore have more energy – than the solar wind.

These measurements will help scientists understand these particles' lifecycles – where they came from, how they got to be traveling so fast (these particles can reach speeds more than half the speed of light!) and what path they take as they travel away from the Sun and into interplanetary space.

2. Taking pictures – but not of the Sun's surface.

WISPR (Wide-Field Imager for Parker Solar Probe) has the only two cameras on Parker Solar Probe – but they're not pointed directly at the Sun. Instead, WISPR looks out the side of the spacecraft, in the direction it's traveling, looking at the space Parker Solar Probe is about to fly through. From that vantage point, WISPR captures images of structures within the corona like coronal mass ejections, or CMEs. CMEs are clouds of solar material that occasionally explode from the Sun at millions of miles per hour. Because this solar material is magnetized, CMEs can trigger geomagnetic storms when they reach Earth – which, in turn, can cause effects like auroras and even, in extreme cases, power outages.  

Right now, our observations of events like these come from satellites orbiting near Earth, so WISPR will give us a whole new perspective. And, scientists will be able to combine WISPR's images with Parker Solar Probe's direct particle measurements to get a better idea of how these structures change as they travel.

3. Studying electric & magnetic fields

The FIELDS instrument suite is appropriately named: It's what scientists will use to study the electric and magnetic fields in the corona.

Electric and magnetic fields are key to understanding what happens, not only on the Sun, but throughout space, because they are the primary driver accelerating charged particles. In particular, a process called magnetic reconnection – when magnetic field lines explosively realign, sending particles rocketing away at incredible speeds – is thought to drive solar explosions, as well as space weather effects on Earth, like the aurora.

FIELDS measures electric and magnetic field at high time resolution, meaning it takes lots of measurements in a short amount of time, to track these processes and shed some light on the mechanics underlying the Sun's behavior. FIELDS' measurements are precisely synced up with those of the SWEAP suite (one of the sets of instruments studying particles) so that scientists can match up the immediate effects that electric and magnetic fields have on the material of the solar wind.

Parker Solar Probe launches summer 2018 on its mission to study the Sun. Keep up with the latest on the mission at nasa.gov/solarprobe or follow us on Twitter and Facebook.

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

What range/area will Perseverance be able to cover on the Martian surface? I'm assuming it's greater than the other rovers but by how much?

TweetChat from Space!

Astronaut Scott Kelly, who is currently in the middle of his #YearInSpace mission, hosted his second TweetChat Saturday, Sept. 19, from the International Space Station. He received tons of great questions about his life in orbit, and we’ve selected a few to highlight below: 

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

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

Solar System: Things to Know This Week

Go for Venus! Fifty-five years ago this week, Mariner 2, the first fully successful mission to explore another planet launched from Cape Canaveral in Florida. Here are 10 things to know about Mariner 2.

1. Interplanetary Cruise 

On August 27, 1962, Mariner 2 launched on a three and a half month journey to Venus. The little spacecraft flew within 22,000 miles (about 35,000 kilometers) of the planet. 

2. Quick Study 

Mariner 2's scan of Venus lasted only 42 minutes. And, like most of our visits to new places, the mission rewrote the books on what we know about Earth's sister planet.

3. Hot Planet 

The spacecraft showed that surface temperature on Venus was hot enough to melt lead: at least 797 degrees Fahrenheit (425 degrees Celsius) on both the day and night sides.

4. Continuous Clouds 

The clouds that make Venus shine so bright in Earth's skies are dozens of miles thick and permanent. It's always cloudy on Venus, and the thick clouds trap heat - contributing to a runaway "greenhouse effect."

5. Night Light 

Those clouds are why Venus shines so brightly in Earth's night sky. The clouds reflect and scatter sunlight, making Venus second only to our Moon in celestial brightness.

6. Under Pressure 

Venus' clouds also create crushing pressure. Mariner 2's scan revealed pressure on the surface of Venus is equal to pressure thousands of feet under Earth's deepest oceans.

7. Slow Turn 

Mariner 2 found Venus rotates very slowly, and in the opposite direction of most planets in our solar system.

8. Space Travel Is Tough 

Mariner 2 was a remarkable accomplishment, considering that in 1962 engineers were still in the very early stages of figuring out how operate spacecraft beyond Earth orbit. The first five interplanetary missions launched - by the U.S. and Soviet Union, the only two spacefaring nations at the time - were unsuccessful.

9. Not Ready for Its Close Up 

Mariner 2 carried no cameras. The first close-up pictures of Venus came from NASA's Mariner 10 in 1974.  

10. Hot Shot 

The first (and still incredibly rare) photo of the surface of Venus was taken by the Soviet Venera 9 lander, which survived for a little more than a minute under the crushing pressure and intense heat on the ground.

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

What is a typical day in the international space station like?? I cant help but express my admiration for you.

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

Answer Time with NASA Astronaut Peggy Whitson

Ever wonder what it’s like to be a NASA astronaut? On Thursday, Oct. 29, NASA Astronaut Peggy Whitson will answer your questions! She’ll explain how it takes the NASA Village to help train for her mission to space, what the challenges of living in space are and what it’s like to be a NASA astronaut.

Enter your questions here. The Answer Time begins at 3 p.m. EDT on Thursday, Oct. 29.

Fun facts about NASA Astronaut Peggy Whitson:

Astronaut Whitson was selected as an Astronaut Candidate in April 1996, and started training in August of the same year.

After completing two years of training and evaluation, she served as the lead for the Crew Test Support Team in Russia from 1998 to 1999.

Astronaut Whitson completed two six-month tours of duty aboard the International Space Station.

She has accumulated 377 days in space between two missions, which is the most for any woman.

Astronaut Whitson has performed a total of six career spacewalks, adding up to 39 hours and 46 minutes! She is also one of only a handful of people to perform spacewalks in both Russian and US spacesuits.

She is scheduled to launch in late 2016 as part of the Expedition 50/51.

Firsts:

Science Officer of the International Space Station

Female Commander for the International Space Station

Female to serve as Chief of the Astronaut Office

Follow her on social media to see how it takes a NASA Village to train her for her upcoming mission: Tumblr, Facebook and Twitter. 

Eight Things to Know About Our Flying Observatory

Our flying observatory, called SOFIA, is the world’s largest airborne observatory. It is a partnership with the German Aerospace Center (DLR). SOFIA studies the life cycle of stars, planets (including Pluto’s atmosphere), how interstellar dust can contribute to planet formation, analyzes the area around black holes, and identifies complex molecules in space.

1. A Telescope in an Airplane

SOFIA stands for the Stratospheric Observatory for Infrared Astronomy. It is a Boeing 747SP aircraft that carries a 100-inch telescope to observe the universe while flying between 38,000 and 45,000 feet – the layer of Earth’s atmosphere called the stratosphere.

2. The Short Aircraft Means Long Flights

SP stands for “special performance.” The plane is 47 feet shorter than a standard 747, so it’s lighter and can fly greater distances.  Each observing flight lasts 10-12 hours.

3. It Flies with A Hole in the Side of the Plane…

The telescope is behind a door that opens when SOFIA reaches altitude so astronomers on board can study the universe. The kind of light SOFIA observes, infrared, is blocked by almost all materials, so engineers designed the side of the aircraft to direct air up-and-over the open cavity, ensuring a smooth flight.

4. …But the Cabin is Pressurized!

A wall, called a pressure bulkhead, was added between the telescope and the cabin so the team inside the aircraft stays comfortable and safe. Each flight has pilots, telescope operators, scientists, flight planners and mission crew aboard.

5. This Telescope Has to Fly

Water vapor in Earth’s atmosphere blocks infrared light from reaching the ground. Flying at more than 39,000 feet puts SOFIA above more than 99% of this vapor, allowing astronomers to study infrared light coming from space. The airborne observatory can carry heavier, more powerful instruments than space-based observatories because it is not limited by launch weight restrictions and solar power.

6. Studying the Invisible Universe

Humans cannot see what is beyond the rainbow of visible light. However, many interesting astronomical processes happen in the clouds of dust and gas that often surround the objects SOFIA studies, like newly forming stars. Infrared light can pass through these clouds, allowing astronomers to study what is happening inside these areas.

7. The German Telescope

The telescope was built our partner, the German Aerospace Center, DLR. It is made of a glass-ceramic material called Zerodur that does not change shape when exposed to extremely cold temperatures. The telescope has a honeycomb design, which reduces the weight by 80%, from 8,700 lb to 1,764 lb. (Note that the honeycomb design was only visible before the reflective aluminum coating was applied to the mirror’s surface).

8. ZigZag Flights with a Purpose

The telescope can move up and down, between 20-60 degrees above the horizon. But it can only move significantly left and right by turning the whole aircraft. Each new direction of the flight means astronomers are studying a new celestial object. SOFIA’s flight planners carefully map where the plane needs to fly to best observe each object planned for that night.

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