Will We Need To Wear The Special Glasses All Day Or Just During That 2 Hour Window Where Viewing Is Happening?

Flying Observatory Has Big Plans for New Zealand

Our flying observatory, called SOFIA, carries a 100-inch telescope inside a Boeing 747SP aircraft. Scientists onboard study the life cycle of stars, planets (including the atmospheres of Pluto and Jupiter), nearby planetary systems, galaxies, black holes and complex molecules in space.

Flying South

Usually based in California, SOFIA and its team are returning to the Southern Hemisphere to study objects that aren't visible from the Northern Hemisphere and to take advantage of the long winter nights. The team operates from Christchurch, New Zealand, regularly between June and August and continues with more big plans for this year.

Working with New Horizons 

Our SOFIA and New Horizons teams are working together again, to learn more about the next object that the New Horizons spacecraft will fly past, Kuiper Belt Object 2014 MU69, or MU69. This will be the farthest object ever encountered by any spacecraft, but little is known about it. Our team on SOFIA will be searching for possible debris around MU69 that could damage the spacecraft and will measure its size, helping the New Horizons team plan their next flyby.

How We Study Distant Celestial Objects from Earth

Our SOFIA team will study MU69 on July 10, 2017, well before New Horizons arrives in January 2019. We can study this distant object from Earth by flying in the faint shadow that it will cast on Earth’s surface as it passes in front of a star. SOFIA will fly directly into the center of this shadow as it moves across the Pacific Ocean. From inside the shadow, the team onboard will study how the light from the star changes as MU69 passes in front it, allowing them to measure its size and to establish if there are any rings or debris around it. The observations will work in the same way that we studied Pluto using SOFIA two weeks before New Horizon’s Pluto Flyby in 2015.

Observing Other Galaxies

The Magellanic Clouds are neighboring galaxies to our own Milky Way Galaxy. We’re studying how stars are forming in the Large and Small Magellanic clouds to compare those processes to star formation in our own galaxy. The Magellanic Clouds are best observed from the southern hemisphere.

And Supernova 1987A

Inside the Large Magellanic Cloud is Supernova 1987A, the closest supernova explosion witnessed in almost 400 years. Our team onboard SOFIA will continue studying this supernova to better understand the material expanding out from it, which may become the building blocks of future stars and planets. Many of our telescopes have studied Supernova 1987A, including the Hubble Space Telescope, the Chandra X-ray Observatory and SOFIA’s predecessor, the Kuiper Airborne Observatory, but the instruments on SOFIA are the only tools we can use to study the debris around it at infrared wavelengths, to better understand characteristics of the dust that cannot be measured using other wavelengths of light.

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Love Letters from Space

Love is in the air, and it’s out in space too! The universe is full of amazing chemistry, cosmic couples held together by gravitational attraction, and stars pulsing like beating hearts.

Celestial objects send out messages we can detect if we know how to listen for them. Our upcoming Nancy Grace Roman Space Telescope will help us scour the skies for all kinds of star-crossed signals.

Celestial Conversation Hearts

Communication is key for any relationship – including our relationship with space. Different telescopes are tuned to pick up different messages from across the universe, and combining them helps us learn even more. Roman is designed to see some visible light – the type of light our eyes can see, featured in the photo above from a ground-based telescope – in addition to longer wavelengths, called infrared. That will help us peer through clouds of dust and across immense stretches of space.

Other telescopes can see different types of light, and some detectors can even help us study cosmic rays, ghostly neutrinos, and ripples in space called gravitational waves.

Intergalactic Hugs

This visible and near-infrared image from the Hubble Space Telescope captures two hearts locked in a cosmic embrace. Known as the Antennae Galaxies, this pair’s love burns bright. The two spiral galaxies are merging together, igniting the birth of brand new baby stars.

Stellar nurseries are often very dusty places, which can make it hard to tell what’s going on. But since Roman can peer through dust, it will help us see stars in their infancy. And Roman’s large view of space coupled with its sharp, deep imaging will help us study how galaxy mergers have evolved since the early universe.

Cosmic Chemistry

Those stars are destined to create new chemistry, forging elements and scattering them into space as they live, die, and merge together. Roman will help us understand the cosmic era when stars first began forming. The mission will help scientists learn more about how elements were created and distributed throughout galaxies.

Did you know that U and I (uranium and iodine) were both made from merging neutron stars? Speaking of which…

Fatal Attraction

When two neutron stars come together in a marriage of sorts, it creates some spectacular fireworks! While they start out as stellar sweethearts, these and some other types of cosmic couples are fated for devastating breakups.

When a white dwarf – the leftover core from a Sun-like star that ran out of fuel – steals material from its companion, it can throw everything off balance and lead to a cataclysmic explosion. Studying these outbursts, called type Ia supernovae, led to the discovery that the expansion of the universe is speeding up. Roman will scan the skies for these exploding stars to help us figure out what’s causing the expansion to accelerate – a mystery known as dark energy.

Going Solo

Plenty of things in our galaxy are single, including hundreds of millions of stellar-mass black holes and trillions of “rogue” planets. These objects are effectively invisible – dark objects lost in the inky void of space – but Roman will see them thanks to wrinkles in space-time.

Anything with mass warps the fabric of space-time. So when an intervening object nearly aligns with a background star from our vantage point, light from the star curves as it travels through the warped space-time around the nearer object. The object acts like a natural lens, focusing and amplifying the background star’s light.

Thanks to this observational effect, which makes stars appear to temporarily pulse brighter, Roman will reveal all kinds of things we’d never be able to see otherwise.

Roman is nearly ready to set its sights on so many celestial spectacles. Follow along with the mission’s build progress in this interactive virtual tour of the observatory, and check out these space-themed Valentine’s Day cards.

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Subtle Lunar Eclipse

Today’s (Feb. 10) lunar activity comes in the form of a penumbral eclipse. What does that mean and how does this type differ from a total eclipse? Let’s take a look:

First off, what is a penumbra? During a lunar eclipse, two shadows are cast by the Earth. The first is called the umbra (UM bruh). This shadow gets smaller as it goes away from the Earth. It is the dark center of the eclipse shadow where the moon is completely in the shadow of the Earth.

The second shadow is called the penumbra (pe NUM bruh). The penumbra gets larger as it goes away from the Earth. The penumbra is the weak or pale part of the shadow. This occurs because the Earth is covering a portion of the sun.

Penumbral eclipses occur when only the outer shadow (the penumbra) of Earth falls on the moon’s surface. This type of eclipse is much more difficult to observe than total eclipses or when a portion of the moon passes into the umbra. That said, if you’re very observant, you may notice a dark shadow on the moon during mid-eclipse on Friday evening. You may not notice anything at all. It’s likely the moon will just look at little bit darker than normal…like this: 

Earth’s penumbral shadow forms a diverging cone that expands into space in the opposite direction of the sun. From within this zone, Earth blocks part but not the entire disk of the sun. Thus, some fraction of the sun’s direct rays continues to reach the most deeply eclipsed parts of the moon during a penumbral eclipse.

For most of North America, the penumbral eclipse will begin at moonrise (sunset) on Friday, Feb. 10 and will be obscured by evening light. Here’s a guide of when to look up:

Fun fact: Aristotle (384 – 322 BCE) first proved that Earth was round using the curved umbral shadow seen at partial eclipses. In comparing observations of several eclipses, he noted that Earth’s shadow was round no matter where the eclipse took place. Aristotle correctly reasoned that only a sphere casts a round shadow from every angle.

To learn more about lunar eclipses, visit: https://svs.gsfc.nasa.gov/11828

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What do you hope to find on the mars? / What would be the best possible outcome?

Ten Awe-Inspiring Photos

We’ve taken 10 of our top Instagram posts and put them here for your viewing pleasure. Now, your next 10 cell phone backgrounds can be found in one place.

10. Water on Mars

With 210,000 likes, this image is a favorite on Instagram. New findings from our Mars Reconnaissance Orbiter (MRO) provide the strongest evidence yet that liquid water flows intermittently on present-day Mars. Dark, narrow streaks on Martian slopes such as these at Hale Crater are inferred to be formed by seasonal flow of water on contemporary Mars. The streaks are roughly the length of a football field.

9. Smoke Ring for a Halo

With 210,000 likes, this image shined on Instagram. Two stars shine through the center of a ring of cascading dust in this image taken by the Hubble Space Telescope. The star system is named DI Cha, and while only two stars are apparent, it is actually a quadruple system containing two sets of binary stars. As this is a relatively young star system it is surrounded by dust.

8. Pluto’s Largest Moon, Charon

With 216,000 likes, a lot of people thought this image was interesting on Instagram. Our New Horizons spacecraft has returned the best color and the highest resolution images yet of Pluto's largest moon, Charon - and these pictures show a surprisingly complex and violent history. This high-resolution enhanced color view of Charon was captured just before closest approach on July 14. The image combines blue, red and infrared images; the colors are processed to best highlight the variation of surface properties across Charon.

7. Veil Nebula

With 220,000 likes, many people favorited this image  on Instagram. This is the expanding remains of a massive star that exploded about 8,000 years ago. This view is a mosaic of six pictures from our Hubble Space Telescope of a small area roughly two light-years across, covering only a tiny fraction of the nebula's vast structure. This close-up look unveils wisps of gas, which are all that remain of what was once a star 20 times more massive than our sun.

6. Messier 94 Galaxy

With 234,000 likes, this image is a favorite on Instagram. This image shows the galaxy Messier 94, which lies in the small northern constellation of the Hunting Dogs, about 16 million light-years away. Within the bright ring or starburst ring around Messier 94, new stars are forming at a high rate and many young, bright stars are present within it.

5. Solar ‘Pumpkin’

With 247,000 likes, many followers enjoyed this image on Instagram. This photo was posted on Halloween and shows active regions on the sun combined to look something like a jack-o-lantern’s face. The image was captured by NASA's Solar Dynamics Observatory in October 2014, which watches the sun at all times from its orbit in space.

4. Italy from the International Space Station

With 251,000 likes, this image captivated many of you on Instagram. Before drifting off to sleep, NASA astronaut Scott Kelly (@stationcdrkelly) captured this images from the International Space Station and wrote, " Day 180. Moonlight over Italy. #BuonaNotte Good night from @ISS! #YearInSpace.”

3. Cosmic Archaeological Dig

With 286,000 likes, this image dazzled many of you on Instagram. Peering deep into the Milky Way's crowded central hub of stars, researchers using our Hubble Space Telescope have uncovered for the first time a population of ancient white dwarfs -- smoldering remnants of once-vibrant stars that inhabited the core. Finding these relics at last can yield clues to how our galaxy was built, long before Earth and our sun formed. This image is a small section of Hubble's view of the dense collection of stars crammed together in the galactic bulge.

2. Super Blood Moon

With 310,000 likes, this image was very popular on Instagram. It shows the Super Blood Moon behind the Washington Monument on Sunday, Sept. 27, in Washington, DC. The combination of a supermoon and total lunar eclipse last occurred in 1982 and will not happen again until 2033.

1. Pluto

With 363,000 likes, this image is one of our most popular pictures on Instagram. The dwarf planet sent a love note back to Earth via our New Horizons spacecraft, which traveled more than 9 years and 3+ billion miles. This was the last and most detailed image of Pluto sent to Earth before the moment of closest approach, which was at 7:49 a.m. EDT Tuesday, July 14 - about 7,750 miles above the surface -- roughly the same distance from New York to Mumbai, India - making it the first-ever space mission to explore a world so far from Earth.

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Much of the western United States began the morning with the view of a super blue blood moon total lunar eclipse. In this silent time lapse video, the complete eclipse is seen over NASA's Jet Propulsion Laboratory, located at the base of the San Gabriel Mountains near Pasadena, California.  This Jan. 31 full moon was special for three reasons: it was the third in a series of “supermoons,” when the Moon is closer to Earth in its orbit -- known as perigee -- and about 14 percent brighter than usual. It was also the second full moon of the month, commonly known as a “blue moon.” The super blue moon will pass through Earth’s shadow to give viewers in the right location a total lunar eclipse. While the Moon is in the Earth’s shadow it will take on a reddish tint, known as a “blood moon.”

Credits: NASA/JPL-Caltech

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How have you used the experience gained from Curiosity to make Perseverance better? Like, Curiosity's wheels are showing wear and tear, so is there something different about Perseverance's wheels?

Using All of Our Senses in Space

Today, we and the National Science Foundation (NSF) announced the detection of light and a high-energy cosmic particle that both came from near a black hole billions of trillions of miles from Earth. This discovery is a big step forward in the field of multimessenger astronomy.

But wait — what is multimessenger astronomy? And why is it a big deal?

People learn about different objects through their senses: sight, touch, taste, hearing and smell. Similarly, multimessenger astronomy allows us to study the same astronomical object or event through a variety of “messengers,” which include light of all wavelengths, cosmic ray particles, gravitational waves, and neutrinos — speedy tiny particles that weigh almost nothing and rarely interact with anything. By receiving and combining different pieces of information from these different messengers, we can learn much more about these objects and events than we would from just one.

Lights, Detector, Action!  

Much of what we know about the universe comes just from different wavelengths of light. We study the rotations of galaxies through radio waves and visible light, investigate the eating habits of black holes through X-rays and gamma rays, and peer into dusty star-forming regions through infrared light.

The Fermi Gamma-ray Space Telescope, which recently turned 10, studies the universe by detecting gamma rays — the highest-energy form of light. This allows us to investigate some of the most extreme objects in the universe.

Last fall, Fermi was involved in another multimessenger finding — the very first detection of light and gravitational waves from the same source, two merging neutron stars. In that instance, light and gravitational waves were the messengers that gave us a better understanding of the neutron stars and their explosive merger into a black hole.

Fermi has also advanced our understanding of blazars, which are galaxies with supermassive black holes at their centers. Black holes are famous for drawing material into them. But with blazars, some material near the black hole shoots outward in a pair of fast-moving jets. With blazars, one of those jets points directly at us!

Multimessenger Astronomy is Cool

Today’s announcement combines another pair of messengers. The IceCube Neutrino Observatory lies a mile under the ice in Antarctica and uses the ice itself to detect neutrinos. When IceCube caught a super-high-energy neutrino and traced its origin to a specific area of the sky, they alerted the astronomical community.

Fermi completes a scan of the entire sky about every three hours, monitoring thousands of blazars among all the bright gamma-ray sources it sees. For months it had observed a blazar producing more gamma rays than usual. Flaring is a common characteristic in blazars, so this did not attract special attention. But when the alert from IceCube came through about a neutrino coming from that same patch of sky, and the Fermi data were analyzed, this flare became a big deal!

IceCube, Fermi, and followup observations all link this neutrino to a blazar called TXS 0506+056. This event connects a neutrino to a supermassive black hole for the very first time.  

Why is this such a big deal? And why haven’t we done it before? Detecting a neutrino is hard since it doesn’t interact easily with matter and can travel unaffected great distances through the universe. Neutrinos are passing through you right now and you can’t even feel a thing!

The neat thing about this discovery — and multimessenger astronomy in general — is how much more we can learn by combining observations. This blazar/neutrino connection, for example, tells us that it was protons being accelerated by the blazar’s jet. Our study of blazars, neutrinos, and other objects and events in the universe will continue with many more exciting multimessenger discoveries to come in the future.

Want to know more? Read the story HERE.

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Comin’ in Hot: Seven Things to Know About our New Heat Shield

What goes up, must come down, and from space, without burning up in an atmosphere. That’s why we’re pumped for the Low-Earth Orbit Flight Test of an Inflatable Decelerator, or LOFTID. Launching on Nov. 1, 2022, with the National Oceanic and Atmospheric Administration’s (NOAA) Joint Polar Orbiting Satellite System-2 (JPSS-2) mission, this technology demonstration marks the next step in advancing an innovative heat shield design that could one day be used to land heavy payloads – including humans – on Mars!

Here are seven things to know about this innovative re-entry system: 

1. LOFTID is the first-ever in-orbit test of this technology. 

Inflatable heat shields, called Hypersonic Inflatable Aerodynamic Decelerators (HIADs), have been in the works for more than a decade. In 2012, the third of the Inflatable Re-entry Vehicle Experiments (IRVE) launched on a suborbital sounding rocket from the Wallops Flight Facility, demonstrating a 3-meter (10-foot) diameter inflatable heat shield.

But the LOFTID re-entry vehicle, at 19.7 feet (6 meters) in diameter, will be the largest blunt body aeroshell to ever go through atmospheric entry. Designed to withstand temperatures as high as 2900°F (1600°C), this first-ever in-orbit test of this technology will prove if it can successfully slow down large payloads – such as crewed spacecraft, robotic explorers, and rocket components – enabling them to survive the heat of re-entry at planetary destinations with an atmosphere.

2. You can find out how this tech works in real-time.  

LOFTID is unique in that all operations will happen within a few hours of launch. After the JPSS-2 satellite safely reaches orbit, the LOFTID vehicle will separate from the upper stage of the Atlas V rocket and begin re-entry into Earth’s atmosphere. If all goes as planned, the technology will help the vehicle decelerate from hypersonic (more than 25 times faster than the speed of sound) down to subsonic flight, less than 609 miles per hour for a safe splash down and recovery from the Pacific Ocean. 

While in flight, engineers at NASA’s Langley Research Center will receive location data every 20 seconds and onboard sensors and cameras will record more comprehensive data about the technology’s performance. You can get a behind-the-scenes look at Langley’s Flight Mission Support Center where the LOFTID project team will be monitoring the flight test at NASA.gov/live following the launch.

3. A lemon-sized capsule ejected into the Pacific Ocean will hold key flight data. 

The LOFTID re-entry vehicle will record both sensor and camera data during its flight. The data will include the temperatures and pressures experienced by the heat shield and will illustrate how well the technology performed during the demonstration.

Although the goal is to retrieve the LOFTID re-entry vehicle after it splashes down in the Pacific Ocean, the team wanted a back-up option just in case they can’t recover it. Enter the tiny yellow package called an ejectable data module (EDM) which will also record flight data. The EDM will be released from the spacecraft at an altitude of about 50,000 feet. It will free fall into the Pacific Ocean off the coast of Hawaii and should land within 10 miles of the spacecraft’s splash down location. A recovery team, that has practiced hide-and-seek of the EDM on land and sea, will use GPS to search an approximately 900-mile area of the Pacific Ocean to find their “lemon.”

4. This heat shield packs a punch. 

Although NASA has historically relied on rigid aeroshells, parachutes, and retro-propulsion (rockets) to decelerate people, vehicles, and hardware during entry, descent, and landing operations, a benefit of inflatable heat shields is that they take up less space in a rocket, allowing more room for other hardware or payloads. LOFTID’s aeroshell has been folded and tightly packed down to 4 by 1.5 feet for launch and stacked in the United Launch Alliance (ULA) Atlas V rocket payload fairing.

5. LOFTID is dedicated in honor of one of its innovators.  

LOFTID was developed as a partnership with ULA and is dedicated to the memory of Bernard Kutter, ULA manager of advanced programs, who passed away in August 2020. Kutter was instrumental in advancing the inflatable heat shield design and developing the plan to test the system on an Atlas V rocket. He was an advocate for both space technology and expanding access to space. Kutter’s NASA and ULA counterparts agree that LOFTID is unlikely to have made it to space without his vision and passion.

6. LOFTID is made of tough stuff. 

Synthetic fibers make up the inflatable structure, braided into tubes that are, by weight, 10 times stronger than steel. The tubes are coiled so that they form the shape of a blunt cone when inflated. The thermal protection system that covers the inflatable structure can survive searing entry temperatures up to 2,900 degrees Fahrenheit. Researchers used the same heat-shielding materials to create a fire shelter prototype for firefighters battling forest fires.

7. You can make your own LOFTID Halloween costume! 

Still looking for an out-of-this world Halloween costume? With a few commonly found materials, like orange pool noodles and duct tape, you can create your own LOFTID costume. However, we make no promises of protecting or slowing you down from becoming the life of the party.

Follow @NASA_Technology for the latest updates on LOFTID. Don’t miss our live coverage leading up to launch from the Vandenberg Space Force Base in California. The NASA Edge JPSS-2 Tower Rollback Show airs live on NASA TV and YouTube on Tuesday, Nov. 1 at 12 a.m. EDT, and NASA TV live launch coverage will begin at 4:45 a.m. EDT. 

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We’re studying a new method of water recycling and carbon dioxide removal that relies on specific geometric shapes and fluid dynamics, rather than complex machinery, in an effort to help build better life support systems for spacecraft. The research could also teach us more about the water processing approaches we take on Earth. Here, NASA astronaut Jack Fischer, is working with the Capillary Structures for Exploration Life Support (Capillary Structures) investigation capillary sorbent hardware that is made up of 3D printed contractors that are supported by tubing, valves and a pump.

Learn more about how this highly interactive investigation works, and what we could learn from the results HERE.

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