Visual 'Autocorrect' For NASA Space Telescope

Visual 'Autocorrect' for NASA Space Telescope

Telescopes located both on the ground and in space continue to dazzle us with incredible images of the universe. We owe these sharp vistas to a series of brilliant astronomers, including Andrea Ghez – an astrophysicist and professor at UCLA – and the “Mother of Hubble,” Nancy Grace Roman.

Did you know that stars don’t actually twinkle? They only look like they do because their light has to travel through our turbulent atmosphere to reach our eyes. As the atmosphere shifts and swirls around, the light from distant stars is slightly refracted, or bent, in different directions. Sometimes it’s directed right at us, but sometimes it’s directed a bit to the side.

Visual 'Autocorrect' For NASA Space Telescope

It's like someone’s shining a flashlight toward you but moving it around slightly. Sometimes the beam is pointed right at you and appears very bright, and sometimes it's pointed a bit to either side of you and it appears dimmer. The amount of light isn't really changing, but it looks like it is.

Visual 'Autocorrect' For NASA Space Telescope

This effect creates a problem for ground-based telescopes. Instead of seeing sharp images, astronomers get fuzzy pictures. Special tech known as adaptive optics helps resolve pictures of space so astronomers can see things more clearly. It’s even useful for telescopes that are in space, above Earth’s atmosphere, because tiny imperfections in their optics can blur images, too.

Visual 'Autocorrect' For NASA Space Telescope

In 2020, Andrea Ghez was awarded a share of the Nobel Prize in Physics for devising an experiment that proved there’s a supermassive black hole embedded in the heart of our galaxy – something Hubble has shown is true of almost every galaxy in the universe! She used the W. M. Keck Observatory’s adaptive optics to track stars orbiting the unseen black hole.

Visual 'Autocorrect' For NASA Space Telescope

A woman named Nancy Grace Roman, who was NASA’s first chief astronomer, paved the way for telescopes that study the universe from space. An upcoming observatory named in her honor, the Nancy Grace Roman Space Telescope, will use a special kind of adaptive optics in its Coronagraph Instrument, which is a technology demonstration designed to block the glare from host stars and reveal dimmer orbiting planets.

Roman’s Coronagraph Instrument will come equipped with deformable mirrors that will serve as a form of visual "autocorrect" by measuring and subtracting starlight in real time. The mirrors will bend and flex to help counteract effects like temperature changes, which can slightly alter the shape of the optics.

Visual 'Autocorrect' For NASA Space Telescope

Other telescopes have taken pictures of enormous, young, bright planets orbiting far away from their host stars because they’re usually the easiest ones to see. Taking tech that’s worked well on ground-based telescopes to space will help Roman photograph dimmer, older, colder planets than any other observatory has been able to so far. The mission could even snap the first real photograph of a planet like Jupiter orbiting a Sun-like star!

Find out more about the Nancy Grace Roman Space Telescope on Twitter and Facebook, and learn about the person from which the mission draws its name.

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More Posts from Nasa and Others

6 years ago

Things That Go Bump in the Gamma Rays

Some people watch scary movies because they like being startled. A bad guy jumps out from around a corner! A monster emerges from the shadows! Scientists experience surprises all the time, but they’re usually more excited than scared. Sometimes theories foreshadow new findings — like when there’s a dramatic swell in the movie soundtrack — but often, discoveries are truly unexpected. 

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Scientists working with the Fermi Gamma-Ray Space Telescope have been jumping to study mysterious bumps in the gamma rays for a decade now. Gamma rays are the highest-energy form of light. Invisible to human eyes, they’re created by some of the most powerful and unusual events and objects in the universe. In celebration of Halloween, here are a few creepy gamma-ray findings from Fermi’s catalog.

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Stellar Graveyards

If you were to walk through a cemetery at night, you’d expect to trip over headstones or grave markers. Maybe you’d worry about running into a ghost. If you could explore the stellar gravesite created when a star explodes as a supernova, you’d find a cloud of debris expanding into interstellar space. Some of the chemical elements in that debris, like gold and platinum, go on to create new stars and planets! Fermi found that supernova remnants IC 443 and W44 also accelerate mysterious cosmic rays, high-energy particles moving at nearly the speed of light. As the shockwave of the supernova expands, particles escape its magnetic field and interact with non-cosmic-ray particles to produce gamma rays. 

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Ghost Particles

But the sources of cosmic rays aren’t the only particle mysteries Fermi studies. Just this July, Fermi teamed up with the IceCube Neutrino Observatory in Antarctica to discover the first source of neutrinos outside our galactic neighborhood. Neutrinos are particles that weigh almost nothing and rarely interact with anything. Around a trillion of them pass through you every second, ghost-like, without you noticing and then continue on their way. (But don’t worry, like a friendly ghost, they don’t harm you!) Fermi traced the neutrino IceCube detected back to a supermassive black hole in a distant galaxy. By the time it reached Earth, it had traveled for 3.7 billion years at almost the speed of light!

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Black Widow Pulsars

Black widows and redbacks are species of spiders with a reputation for devouring their partners. Astronomers have discovered two types of star systems that behave in a similar way. Sometimes when a star explodes as a supernova, it collapses back into a rapidly spinning, incredibly dense star called a pulsar. If there’s a lighter star nearby, it can get stuck in a close orbit with the pulsar, which blasts it with gamma rays, magnetic fields and intense winds of energetic particles. All these combine to blow clouds of material off the low-mass star. Eventually, the pulsar can eat away at its companion entirely.

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Dark Matter

What’s scarier than a good unsolved mystery? Dark matter is a little-understood substance that makes up most of the matter in the universe. The stuff that we can see — stars, people, haunted houses, candy — is made up of normal matter. But our surveys of the cosmos tell us there’s not enough normal matter to keep things working the way they do. There must be another type of matter out there holding everything together. One of Fermi’s jobs is to help scientists narrow down the search for dark matter. Last year, researchers noticed that most of the gamma rays coming from the Andromeda galaxy are confined to its center instead of being spread throughout. One possible explanation is that accumulated dark matter at the center of the galaxy is emitting gamma rays!

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Fermi has helped us learn a lot about the gamma-ray universe over the last 10 years. Learn more about its accomplishments and the other mysteries it’s working to solve. What other surprises are waiting out among the stars?

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


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5 years ago

Hi there! Does the study of Earth Science teach us much about the science of other planets? Can much be assumed to be similar, or is the geology/biology incomparable? Thank you!


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9 years ago

That’s a Wrap - September

Each month, the International Space Station focuses on an area of research. In September, the research focus was biology, encompassing cells, plants, animals, genetics, biochemistry, human physiology and more.

Benefits from this research are vast and include: combating diseases, reducing our environmental footprint, feeding the world’s population and developing cleaner energy.

Here’s a recap of some topics we studied this month:

Cells

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Scientists studied T-cells in orbit to better understand how human immune systems change as they age. For an immune cell, the microgravity environment mimics the aging process. Because spaceflight-induced and aging-related immune suppression share key characteristics, researchers expect the results from this study will be relevant for the general population.

NASA to Napa

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We raised a glass to the space station to toast how the study of plants in space led to air purification technology that keeps the air clean in wine cellars and is also used in homes and medical facilities to help prevent mold.

One-Year Mission

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This month also marked the halfway point of the One-Year Mission. NASA Astronaut Scott Kelly and Roscosmos Cosmonaut Mikhail Kornienko reached the midpoint on Sept. 15. This mission will result in valuable data about human health and the effects of microgravity on the body.

Microbes

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Since microbes can threaten crew health and jeopardize equipment, scientists study them on astronauts’ skin and aboard the space station. Samples like saliva, blood, perspiration and swaps of equipment are collected to determine how microgravity, environment, diet and stress affect the microorganisms.

Model Organisms

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Model organisms have characteristics that allow them to easily be maintained, reproduced and studied in a laboratory. Scientists investigate roundworms, medaka fish and rodents on the station because of this reason. They can also provide insight into the basic cellular and molecular mechanisms of the human body.

For more information about research on the International Space Station, go HERE.

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7 years ago

What’s Up for July 2017

Prepare for the August total solar eclipse by observing the moon phases this month. Plus, two meteor showers peak at the end of July.

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Solar eclipses occur when the new moon passes between the Earth and the sun and moon casts a traveling shadow on Earth. A total solar eclipse occurs when the new moon is in just the right position to completely cover the sun’s disk.

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This will happen next month on August 21, when the new month completely blocks our view of the sun along a narrow path from Oregon to South Carolina.

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It may even be dark enough during the eclipse to see some of the brighter stars and few planets!

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Two weeks before or after a solar eclipse, there is often, but not always, a lunar eclipse. This happens because the full moon, the Earth and the sun will be lined up with Earth in the middle.

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Beginning July 1, we can see all the moon’s phases.

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Many of the Apollo landing sites are on the lit side of the first quarter moon. But to see these sites, you’ll have to rely on images for lunar orbiting spacecraft.

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On July 9, the full moon rises at sunset and July 16 is the last quarter. The new moon begins on July 23 and is the phase we’ll look forward to in August, when it will give us the total solar eclipse. The month of July ends with a first quarter moon.

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We’ll also have two meteor showers, both of which peak on July 30. The Delta Aquarids will have 25 meteors per hour between midnight and dawn.

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The nearby slow and bright Alpha Capricornids per at 5 per hour and often produce fireballs.

Watch the full video:

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


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7 years ago

What exactly is a sun eclipse? Will I be able to see it and if so when from the Netherlands?

The solar eclipse is when the moon is directly in front of the Sun and creates a shadow on the Earth. They happen about once every 18 months. I don’t believe that you’ll be able to see this eclipse from the Netherlands. I think the next one to be in Europe is in 2026. There’s one in Chillie and Argentia in 2019 and another in Antartica in 2021. 


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5 years ago

History Made: Apollo 11 Splashes Down Today in 1969

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The Apollo 11 Command Module “Columbia” is hoisted onto its recovery ship the USS Hornet, following splashdown on July 24, 1969. Credit: NASA

Four days after their historic achievement, Apollo 11 astronauts Neil Armstrong, Buzz Aldrin and Michael Collins splashed down in the Pacific Ocean at 12:49 p.m. EDT, about 900 miles from Hawaii. The crew was recovered by the crew of the USS Hornet where President Richard Nixon was waiting to greet them. 

Watch a replay of the original live broadcast of the recovery on NASA TV starting at 12:45 p.m. EDT. 

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


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8 years ago

Eight Small Satellites Will Give Us a New Look Inside Hurricanes

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The same GPS technology that helps people get where they’re going in a car will soon be used in space in an effort to improve hurricane forecasting. The technology is a key capability in a NASA mission called the Cyclone Global Navigation Satellite System (CYGNSS).

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The CYGNSS mission, led by the University of Michigan, will use eight micro-satellite observatories to measure wind speeds over Earth’s oceans, increasing the ability of scientists to understand and predict hurricanes. Each microsatellite observatory will make observations based on the signals from four GPS satellites.

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The CYGNSS microsatellite observatories will only receive signals broadcast directly to them from GPS satellites already orbiting the Earth and the reflection of the same satellite’s signal reflected from the Earth’s surface. The CYGNSS satellites themselves will not broadcast.

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The use of eight microsatellite observatories will decrease the revisit time as compared with current individual weather satellites. The spacecraft will be deployed separately around the planet, with successive satellites passing over the same region every 12 minutes.

This will be the first time that satellites can peer through heavy tropical rainfall into the middle of hurricanes and predict how intense they are before and during landfall.

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As the CYGNSS and GPS constellations orbit around the Earth, the interaction of the two systems will result in a new image of wind speed over the entire tropics every few hours, compared to every few days for a single satellite.

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Another advantage of CYGNSS is that its orbit is designed to measure only in the tropics…where hurricanes develop and are most often located. The focus on tropical activity means that the instruments will be able to gather much more useful data on weather systems exclusively found in the tropics. This data will ultimately be used to help forecasters and emergency managers make lifesaving decisions.

Launch!

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CYGNSS launched at 8:37 a.m. EST on Thursday, Dec. 15, from our Kennedy Space Center in Florida. CYGNSS launched aboard an Orbital ATK Pegasus XL rocket, deployed from Orbital’s “Stargazer” L-1011 carrier aircraft. 

Pegasus is a winged, three-stage solid propellant rocket that can launch a satellite into low Earth orbit. How does it work? Great question! 

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After takeoff, the aircraft (which looks like a commercial airplane..but with some special quirks) flies to about 39,000 feet over the ocean and releases the rocket. 

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After a five-second free fall in a horizontal position, the Pegasus first stage ignites. The aerodynamic lift, generated by the rocket’s triangle-shaped wing, delivers the payload into orbit in about 10 minutes. 

Pegasus is used to deploy small satellites weighing up to 1,000 pounds into low Earth orbit. 

And success! The eight CYGNSS satellites were successfully deployed into orbit! 

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


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6 years ago

@aura3700: What's the most beautiful thing you've ever seen while in space?


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1 year ago

Hi do you guys really say Houston when responding to each other !?!🤪


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1 year ago
An illustration showing the planet Jupiter rising over the horizon of its moon Europa. Europa’s surface consists of a rough landscape of blue, semi-translucent ice. Jupiter’s colorful orange, blue and cream-colored bands and swirling storms are visible in its atmosphere. In the middle distance, the Europa Clipper spacecraft can be seen, its solar panel wings glinting in the sunlight. 

Image credit: NASA/JPL-Caltech

Hurry! You Can Catch a Ride to Jupiter with NASA

Well, at least your name can.  

One of the planet Jupiter’s largest and most intriguing moons is called Europa. Evidence hints that beneath its icy shell, Europa hides an ocean of liquid water – more water than all of Earth’s oceans combined. In 2024, our Europa Clipper robotic spacecraft sets sail to take a closer look…and when it launches, your name can physically be aboard! Here’s how: 

NASA’s Message in a Bottle campaign invites people around the world to sign their names to a poem written by the U.S. Poet Laureate, Ada Limón. The poem connects the two water worlds — Earth, yearning to reach out and understand what makes a world habitable, and Europa, waiting with secrets yet to be explored.

An illustration showing the planet Jupiter, its moon Europa with its cracked, icy surface, and the Europa Clipper spacecraft, all lined up against the dark background of space.

Image credit: NASA/JPL-Caltech

The poem will be engraved on Europa Clipper, along with participants' names that will be physically etched onto microchips mounted on the spacecraft. Together, the poem and names will travel 1.8 billion miles to the Jupiter system.

A poster with a background illustration showing the planet Jupiter and the surface of its moon Europa. The text reads: Message In a Bottle – Send your name. Next to the text is an illustration of a paper scroll rolled up inside a glass bottle sealed with a cork.

Image credit: NASA/JPL-Caltech

Signing up is easy! Just go to this site to sign your name to the poem and get on board. You can send your name en español, too. Envía tu nombre aquí.

The Europa Clipper launch window opens in October 2024, but don’t wait – everyone’s names need to be received this year so they can be loaded onto the spacecraft in time. Sign up by Dec. 31, 2023.

We hope you’ll be riding along with us! Follow the mission at europa.nasa.gov.

Make sure to follow us on Tumblr for your regular dose of space!


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