What Is The Most Interesting Fact That You Discovered About Black Holes? And What Is The One You Would

#InternationalCatDay? Try #IntergalacticCatDay. 

Check out features of our feline friends that have come to life as interstellar phenomena! 

Pictured first, the Cat’s Paw Nebula is located about 4,200-5,500 light-years from Earth – situated in our very own Milky Way Galaxy. It was named for the large, round features that create the impression of a feline footprint and was captured by our Spitzer Space Telescope. After gas and dust inside the nebula collapse to form stars, the stars may in turn heat up the pressurized gas surrounding them. This process causes the gas to expand into space and form the bright red bubbles you see. The green areas show places where radiation from hot stars collided with large molecules called "polycyclic aromatic hydrocarbons," causing them to fluoresce.

Next, you’ll find the Cat’s Eye Nebula. Residing 3,000 light-years from Earth, the Cat’s Eye represents a brief, yet glorious, phase in the life of a sun-like star. This nebula's dying central star may have produced the simple, outer pattern of dusty concentric shells by shrugging off outer layers in a series of regular convulsions. To create this view, Hubble Space Telescope archival image data have been reprocessed. Compared to well-known Hubble pictures, the alternative processing strives to sharpen and improve the visibility of details in light and dark areas of the nebula and also applies a more complex color palette. Gazing into the Cat's Eye, astronomers may well be seeing the fate of our sun, destined to enter its own planetary nebula phase of evolution ... in about 5 billion years.

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Our Eight Favorite Things About This Weekend’s Student Launch

We’re ready for another year of sky-high fun, literally, as student teams launch nearly 50 high-powered rockets during the 16th annual Student Launch, April 16, near NASA’s Marshall Space Flight Center in Huntsville, Alabama.

Hundreds of students from high schools, colleges and universities across 22 states have spent the past several months designing, fabricating and testing single-stage rockets and autonomous ground support systems. So, what makes this event so great? Start here to find out as we list our eight favorite things.

1. A Mile-High Target

Setting goals is a part of life, and so, too, is this competition. Teams will attempt to launch their rocket to an altitude of one mile, or 5,280 feet. That'll earn the maximum number of altitude points of 5,280. But, if teams go over or under, there's a penalty. Teams lose 2 points for every foot over and 1 point for every foot under.

2. Return of the Mars Ascent Vehicle Challenge

Back for a second consecutive year – the MAV challenge runs parallel with Student Launch -- requiring teams to design an autonomous system capable of retrieving and storing a mock Martian sample into their rocket. Sponsored by the Centennial Challenges program – our citizen prize program -- MAV focuses on designing rockets for future sample return missions to Mars.

3. Why, Yes, It Really Is Rocket Science

Static stability margin, thrust-to-weight ratios and ammonium perchlorate composite propellants may seem like a foreign language, but it’s just everyday lingo for these young rocket scientists. In addition to designing and fabricating a rocket, students hone skills by completing electrical wiring and operating computer-aided software for launching rockets and analyzing payloads.

4. Putting Rocketry Skills to the Test

During launch week, we host a “Rocket Fair,” where each team gives a technical presentation about their rocket and any autonomous systems, to hundreds of engineers and team members from NASA, corporate sponsor Orbital ATK of Promontory, Utah, and the media. Doing so provides students an opportunity to gain valuable feedback from real rocket scientists and engineers.

5. Hard Work Pays Off, Literally

Yes, a year’s worth of bragging rights are on the line, but so, too, is some cold, hard cash. Orbital ATK offers an overall cash prize of $5,000 to the highest-ranking college/university team to meet the Student Launch objectives. Plus, the MAV challenge offers a share of $50,000 for completion of its objectives.

6. Safety, Safety and More Safety

Teams complete a lengthy series of comprehensive flight and safety reviews, all overseen by our staff, engineers and scientists. Multiple reviews are scheduled throughout the 8-month-long design process, as well as during the launch week at Marshall Space Flight Center. These reviews mirror the engineering design lifecycle used by our workforce.

7. Celebrate Good Times

After the smoke clears from rocket launches, teams gather for a well-earned evening of celebration. The awards banquet -- held at the U.S. Space & Rocket Center in Huntsville, Alabama, and funded by Orbital ATK -- recognizes teams with awards including Best Design, Altitude, Safety and more.

8. Teams Make Dreams Come True

More than just a friendly competition, Student Launch and MAV Challenge provide long-lasting life experiences outside of the classroom. Students benefit from working as a team, applying STEM skills and overcoming technical obstacles -- all aspects related to the success of our work. 

The MAV Challenge and Student Launch are open to the public and will stream live on line at: http://www.ustream.tv/channel/nasa-msfc

For more details, rules, photos from previous events, and links to social media accounts providing real-time updates, visit: http://www.nasa.gov/education/studentlaunch

For more information about the Centennial Challenges MAV Challenge, visit: http://www.nasa.gov/winit

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Exploration in Extreme Environments: Under Water and in Outer Space

Living in the depths of the sea…to prepare for travel in deep space. 

Sounds strange, but that’s what our NEEMO expedition aims to do.

This 10-day NASA Extreme Environment Mission Operations (NEEMO) 22 expedition is slated to begin on June 18. NEEMO 22 will focus on both exploration spacewalks (or in this case waterwalks?) and objectives related to the International Space Station and deep space missions.

Analog (noun): is a situation on Earth that produces effects on the body similar to those experienced in space, both physical and mental/emotional. These studies help us prepare for long duration missions.

As an analog for future planetary science concepts and strategies, marine science also will be performed under the guidance of Florida International University’s marine science department.

NASA astronaut Kjell Lindgren will command the NEEMO 22 mission aboard the Aquarius laboratory, 62 feet below the ocean surface near Key Largo Florida. Lindgren was part of the space station Expeditions 44 and 45 in 2015, where he spent 141 days living and working in the extreme environment of space. He also conducted two spacewalks.

Fun Fact: These underwater explorers are referred to as “aquanauts”

Lindgren will be joined by ESA (European Space Agency) astronaut Pedro Duque, Trevor Graff, a Jacobs Engineering employee working as a planetary scientist at our Johnson Space Center; and research scientists Dom D’Agostino from the University of South Florida and the Florida Institute of Human and Machine Cognition.

While living underwater for 10 days, the crew will:

Test spaceflight countermeasure equipment

Validate technology for precisely tracking equipment in a habitat

Complete studies of body composition and sleep

Assess hardware sponsored by ESA that will help crew members evacuate someone who has been injured on a lunar spacewalk

Why do we use Analog Missions?

Analog missions prepare us for near-future exploration to asteroids, Mars and the moon. Analogs play a significant role in problem solving for spaceflight research.

Not all experiments can be done in space – there is not enough time, money, equipment and manpower

Countermeasures can be tested in analogs before trying them in space. Those that do not work in analogs will not be flown in space

Ground-based analog studies are completed more quickly and less expensively

For more information about the NEEMO mission, visit: https://www.nasa.gov/mission_pages/NEEMO/index.html

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Exploring an Asteroid Without Leaving Earth

This 45 day mission – which begins Feb. 1, 2018 – will help our researchers learn how isolation and close quarters affect individual and group behavior. This study at our Johnson Space Center prepares us for long duration space missions, like a trip to an asteroid or even to Mars.

The Human Research Exploration Analog (HERA) that the crew members will be living in is one compact, science-making house. But unlike in a normal house, these inhabitants won’t go outside for 45 days. Their communication with the rest of planet Earth will also be very limited, and they won’t have any access to internet. So no checking social media, kids!

The only people they will talk with regularly are mission control and each other.

The HERA XVI crew is made up of 2 men and 2 women, selected from the Johnson Space Center Test Subject Screening (TSS) pool. The crew member selection process is based on a number of criteria, including criteria similar to what is used for astronaut selection. The four would-be astronauts are:

Kent Kalogera

Jennifer Yen

Erin Hayward

Gregory Sachs

What will they be doing?

The crew are going on a simulated journey to an asteroid, a 715-day journey that we compress into 45 days. They will fly their simulated exploration vehicle around the asteroid once they arrive, conducting several site surveys before 2 of the crew members will participate in a series of virtual reality spacewalks.

They will also be participating in a suite of research investigations and will also engage in a wide range of operational and science activities, such as growing and analyzing plants and brine shrimp, maintaining and “operating” an important life support system, exercising on a stationary bicycle or using free weights, and sharpening their skills with a robotic arm simulation. 

During the whole mission, they will consume food produced by the Johnson Space Center Food Lab – the same food that the astronauts enjoy on the International Space Station – which means that it needs to be rehydrated or warmed in a warming oven.

This simulation means that even when communicating with mission control, there will be a delay on all communications ranging from 1 to 5 minutes each way.

A few other details:

The crew follows a timeline that is similar to one used for the space station crew.

They work 16 hours a day, Monday through Friday. This includes time for daily planning, conferences, meals and exercise.

Mission: February 1, 2018 - March 19, 2018

But beware! While we do all we can to avoid crises during missions, crews need to be able to respond in the event of an emergency. The HERA crew will conduct a couple of emergency scenario simulations, including one that will require them to respond to a decrease in cabin pressure, potentially finding and repairing a leak in their spacecraft.

Throughout the mission, researchers will gather information about living in confinement, teamwork, team cohesion, mood, performance and overall well-being. The crew members will be tracked by numerous devices that each capture different types of data.

Learn more about the HERA mission HERE. 

Explore the HERA habitat via 360-degree videos HERE.

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Celebrating Five Years at Jupiter!

We just released new eye-catching posters and backgrounds to celebrate the five-year anniversary of Juno’s orbit insertion at Jupiter in psychedelic style.

On July 4, 2016, our Juno spacecraft arrived at Jupiter on a mission to peer through the gas giant planet’s dense clouds and answer questions about the origins of our solar system. Since its arrival, Juno has provided scientists a treasure trove of data about the planet’s origins, interior structures, atmosphere, and magnetosphere.

Juno is the first mission to observe Jupiter’s deep atmosphere and interior, and will continue to delight with dazzling views of the planet’s colorful clouds and Galilean moons. As it circles Jupiter, Juno provides critical knowledge for understanding the formation of our own solar system, the Jovian system, and the role giant planets play in putting together planetary systems elsewhere.

Get the posters and backgrounds here!

For more on our Juno mission at Jupiter, follow NASA Solar System on Twitter and Facebook.

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Does space have a standard time or do you rely on the time zones on Earth while you are in space?

Great question.  Really it is up to the particular space agency/mission which time zone they use.  For example, since the International Space Station is a collaboration between NASA, the Russian Space Agency, the European Space Agency, the Japanese Space Agency, and the Canadian Space Agency, we came up with the compromise of operating on Greenwich Mean Time (GMT).  So, Space Station time is the same as London time!  The International Space Station orbits our planet every 90 minutes, so of course we’re transiting across multiple time zones constantly.  

Pi Guides the Way

It may be irrational but pi plays an important role in the everyday work of scientists at NASA. 

What Is Pi ?

Pi is the ratio of a circle’s circumference to its diameter. It is also an irrational number, meaning its decimal representation never ends and it never repeats. Pi has been calculated to more than one trillion digits, 

Why March 14?

March 14 marks the yearly celebration of the mathematical constant pi. More than just a number for mathematicians, pi has all sorts of applications in the real world, including on our missions. And as a holiday that encourages more than a little creativity – whether it’s making pi-themed pies or reciting from memory as many of the never-ending decimals of pi as possible (the record is 70,030 digits).

While 3.14 is often a precise enough approximation, hence the celebration occurring on March 14, or 3/14 (when written in standard U.S.  month/day format), the first known celebration occurred in 1988, and in 2009, the U.S. House of Representatives passed a resolution designating March 14 as Pi Day and encouraging teachers and students to celebrate the day with activities that teach students about pi.

5 Ways We Use Pi at NASA

Below are some ways scientists and engineers used pi.

Keeping Spacecraft Chugging Along

Propulsion engineers use pi to determine the volume and surface area of propellant tanks. It’s how they size tanks and determine liquid propellant volume to keep spacecraft going and making new discoveries. 

Getting New Perspectives on Saturn

A technique called pi transfer uses the gravity of Titan’s moon, Titan, to alter the orbit of the Cassini spacecraft so it can obtain different perspectives of the ringed planet.

Learning the Composition of Asteroids

Using pi and the asteroid’s mass, scientists can calculate the density of an asteroid and learn what it’s made of--ice, iron, rock, etc.

Measuring Craters

knowing the circumference, diameter and surface area of a crater can tell scientists a lot about the asteroid or meteor that may have carved it out.

Determining the Size of Exoplanets

Exoplanets are planets that orbit suns other than our own and scientists use pi to search for them. The first step is determining how much the light curve of a planet’s sun dims when a suspected planets passes in front of it.

Want to learn more about Pi? Visit us on Pinterest at: https://www.pinterest.com/nasa/pi-day/

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What’s Up for November?

November weather can be challenging for backyard astronomers, but the moon is a reliable target, even when there are clouds.

Did you know that the moon takes about 29 days to go around the Earth once? It also takes the moon about 29 days to spin on its axis. This causes the same side of the moon to always face Earth.

On Nov. 3, the moon reaches last quarter when it rises at midnight and sets at noon. This is a great time to see the moon in the morning sky.

On Nov. 11, the new moon isn’t visible, because it’s between Earth and the sun, and the unlit side faces Earth. In the days after the new moon, the slender crescent gets bigger and brighter. Look just after sunset on Nov. 13 and 14 near the setting sun in the western sky.

The next phase on Nov. 19 is called the first quarter, because the moon has traveled one quarter of its 29-day orbit around Earth. The moon rises at noon and sets at midnight, so you can see it in the afternoon sky. It will rise higher in the sky after dark. That’s when you can look for the areas where four of the six Apollo missions landed on the moon! You won’t see the landers, flag or footprints, but it’s fun and easy to see these historic places with your own eyes or with binoculars.

To see the area: Look for three dark, smooth maria, or seas. The middle one is the Sea of Tranquility. Apollo 11 landed very near a bright crater on the edge of this mare in 1969. The Apollo 15, 16 and 17 landing areas form the points of a triangle above and below the Apollo 11 site.

On Nov. 25, you can see the full moon phase, which occurs on the 14th day of the lunar cycle. The moon will rise at sunset and will be visible all night long, setting at sunrise.

On Thanksgiving (Nov. 26), the 15-day-old moon will rise an hour after sunset. You may even see some interesting features! And this is a great time to see the impact rays of some of the larger craters.

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Orion’s top images of 2020

The Orion program showed its resilience this year during an unprecedented time, racking up several success stories building and testing the spacecraft in preparation for upcoming Artemis missions to the Moon. From hot fire and structural testing, to crew and service module assembly activities, progress on Orion brought the agency closer to sending the first woman and next man to the Moon by 2024, and sustainable lunar exploration by 2028.

Ensuring crew safety, a hot fire test was conducted on the Northrop Grumman-built attitude control motor – which provides steering for Orion’s  launch abort system in the event of an emergency during ascent – at the company’s facility in Elkton, Maryland. The 30-second hot fire was the third and final test to qualify the motor for human missions, beginning with Artemis II.

During a three-month testing campaign at NASA’s Plum Brook Station in Sandusky, Ohio, the Orion spacecraft was subjected to the extreme temperatures and electromagnetic environment it will experience on Artemis I – Orion’s first uncrewed test flight to the Moon atop the agency’s  Space Launch System (SLS) rocket. Testing wrapped up early and the vehicle was readied for its journey back to NASA’s Kennedy Space Center aboard the agency’s one-of-a-kind Super Guppy.

Before NASA astronauts fly Orion on missions to the Moon and back, testing is necessary to verify the spacecraft’s ability to withstand the stresses of launch, climb to orbit, the harsh conditions of deep space transit, and return to Earth. Engineers from NASA and its prime contractor, Lockheed Martin, completed testing on Orion’s Structural Test Article (STA) for Artemis I. The STA is structurally identical to Orion’s main spacecraft elements: the crew module, service module and launch abort system.

The first element machined for the Artemis III Orion crew module – a cone panel with openings for windows, which will provide a spectacular view – was designed by Lockheed Martin, and manufactured by AMRO Fabricating Corp., of South El Monte, California. The completed panel made its way to NASA’s Michoud Assembly Facility near New Orleans, where engineers will weld it with other elements as part of Orion’s pressure vessel.

Orion’s European Service Module primary structure for the Artemis for the Artemis III mission arrived at the Airbus facility in Bremen, Germany, from its Thales Alenia Space manufacturing site in Turin, Italy. The service module will be equipped with components to power Orion and provide life support to astronauts – such as air, water, heat and cooling – during the mission that will land the first woman and next man on the Moon.

Three spacecraft adapter jettison fairing panels were fitted onto Orion’s service module inside the Neil Armstrong Operations and Checkout Building at Kennedy. Once secured, the panels encapsulate the service module to protect it from harsh environments such as heat, wind, and acoustics as the spacecraft is propelled out of Earth’s atmosphere atop the SLS rocket during NASA’s Artemis I mission.

What has been the best memory you have so far at NASA?