Weird And Wonderful Irregular Galaxies

Weird and Wonderful Irregular Galaxies

Spiral and elliptical galaxies seem neatly put together, but what happened to irregular galaxies? Irregular galaxies have one-of-a-kind shapes and many look like blobs! Why do they look the way they do? Astronomers think the uniqueness of these galaxies results from their interactions with other galaxies — like when they pass close to one another or even collide!

Weird And Wonderful Irregular Galaxies

Looking back at the early universe with the help of our Hubble Space Telescope’s “deep field” observations, astronomers can peek at galaxies millions and billions of light-years away. They noticed that these far-away galaxies appear unusually messy, showing more star formation and mergers than galaxies closer to the Milky Way.

Weird And Wonderful Irregular Galaxies

We also see irregular galaxies closer to home, though. Some may form when two galaxies pass close together in a near-miss. When this happens, their gravity pulls stars out of place in both galaxies, messing up the neat structure they originally had as spiral or elliptical galaxies. Think of it like this: you happen to have a pile of papers sitting at the edge of a table and when someone passes close by the papers become ruffled and may scatter everywhere! Even though the two galaxies never touched, gravity's effects leave them looking smeared or distorted.

Weird And Wonderful Irregular Galaxies

Some irregular galaxies result from the collision between two galaxies. And while some of these look like a blob of stars and dust, others form dazzling ring galaxies! Scientists think these may be a product of collisions between small and large galaxies. These collisions cause ripples that disturb both galaxies, throwing dust, gas, and stars outward. When this happens, it pushes out a ring of material, causing gas clouds to collide and spark the birth of new stars. After just a few million years, stars larger than our Sun explode as supernovae, leaving neutron stars and black holes throughout the ring!

Weird And Wonderful Irregular Galaxies

Not all galaxy collisions create irregular galaxies — our Milky Way spiral galaxy has gone through many mergers but has stayed intact! And for some interacting galaxies, being an irregular galaxy may just be a phase in their transformation. We’re observing them at a snapshot in time where things are messy, but they may eventually become neat and structured spirals and ellipticals.

Weird And Wonderful Irregular Galaxies

Irregular galaxies are similar to each other, but unique and beautiful because of their different interactions, whether they’re just passing another galaxy or taking part in a dramatic collision. Keep up with NASA Universe on Facebook and Twitter where we post regularly about galaxies.

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9 years ago

What’s Up for October?

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This month is filled with exciting celestial sights. Here are 10 targets you can view this month:

10. Unusual Sunset

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During a sunset, our thick atmosphere absorbs most colors of sunlight, but red light is absorbed the least. Rarely, green flashes can be seen just above the sun’s edge. As the last sliver of the disk disappears below the horizon, be sure to watch its color.

9. Belt of Venus

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Just after sunset, turn around and face east. A dark shadow will move up from the horizon and gradually cover the pinkish sky. This is caused from the Earth itself blocking the sunlight and is called the Earth Shadow or the Belt of Venus.

8. Crepuscular Rays

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Also just after sunset, or before dawn, you may see rays of sunlight spread like a fan. These are called crepuscular rays and are formed when sunlight streams through gaps in the clouds or mountains.

7. Aurora Borealis

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The northern lights, also known as the aurora borealis, are caused by collisions between gaseous particles in Earth’s atmosphere and charged particles released from the sun. The color of the lights can changed depending on the type of gas being struck by particles of solar wind. You can find out when and where to expect aurorae at the Space Weather Prediction Center.

6. Andromeda Galaxy

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Did you now that The Andromeda Galaxy is one of the few you can actually see with your naked eye? In October, look nearly overhead after sunset to see it! This galaxy is more than twice the apparent width of the moon.

5. Moon Features

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Nights in mid-October are excellent for viewing the features on the moon. Areas like the Sea of Tranquility and the site of the 1969 Apollo 11 landing will be visible.

4. A Comet

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This month, the European Space Agency’s Rosetta mission target, a comet with a complicated name (Comet 67P Churyumov-Gerasimenko), is still bright enough for experienced astronomers to pick out in a dark sky. On October 9, you may be able to spot it in the east near the crescent moon and Venus.

3. Meteor Showers

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There are multiple meteor showers this month. On the 9th: watch the faint, slow-moving Draconids. On the 10th: catch the slow, super-bright Taurids. And on the 21st: don’t’ miss the swift and bright Orionids from the dust of Comet Halley.

2. Three Close Planets

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On October 28, you’ll find a tight grouping of Jupiter, Venus and Mars in the eastern sky before sunrise.

1. Zodiacal Light

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The Zodiacal light is a faint triangular glow that can be seen from a dark sky after sunset or before sunrise. What you’re seeing is sunlight reflecting off dust grains that circle the sun in the inner solar system. These dust grains travel in the same plane as the moon and planets as they journey across our sky.

For more stargazing tools visit: Star Tool Box

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5 years ago

Extraordinary Materials: Developed for Space, Useful for Just About Everything on Earth

Did you know technologies developed for space show up all over Earth? Our Technology Transfer Program has one major goal: bring our technology down to Earth. We patent space innovations developed for missions so that companies, startups and entrepreneurs can spin them off into new commercial products.

Our engineers and scientists create all sorts of materials and coatings—in fact, it is one of the most licensed technology categories in our patent portfolio. From materials that improve industrial and household products, to coatings and insulations that protect satellites, machinery and firefighters, our technologies offer smart solutions for modern challenges.

These are a few of our most in-demand technologies.

Dust-Resistant Coatings

Made by innovators at our Langley Research Center, this tech was first created for exploring dusty, dirty surfaces like the Moon, Mars and asteroids. Lunar dust has been shown to cause big problems with mechanical equipment, like clogging filters and damaging seals. This technology can be used in the production of films, coatings and surface treatments to create dust-resistant and self-cleaning products for biomedical devices, aircraft, cars and much more. This tech could be a game-changer when battling dirt and grime.

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Smart, Environmentally-Friendly Coating System

Looking for a technology to ward off corrosion that’s also safe for the environment? Developed to protect our launch pads at Kennedy Space Center from extreme heat and exhaust from rockets, this “smart” coating can detect and prevent corrosion. It can even be painted on damaged surfaces to heal and protect them going forward. This tech has commercial potential in building safer bridges, automobiles and machinery.  While it may seem like magic, this technology will reduce maintenance cost and improve safety.

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Multilayer Fire Protection System

Made to protect astronauts and vehicles during the dangerously hot task of reentry, scientists at Langley developed a flexible, lightweight and portable thermal protection system that can serve as a personal emergency fire shelter.

The flexible technology is made up of multilayer thermal blankets designed to handle external temperatures of up to 2,000°F – that’s as hot as magma found in some volcanos! The system can be formed as a sleeping bag, a tent, a blanket, a curtain, a flexible roll-up doorway or even for fire protection in housing structures.

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Super-Strength Aluminums

This award-winning tech was initially developed by researchers at our Marshall Space Flight Center to help reduce vehicle exhaust emissions. This special alloy is flexible and strong—even at temperatures of over 500°F. That means it can withstand more wear and tear than other similar materials. Currently, this tech can be found improving motors on fishing boats as well as in all kinds of different engines.

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Oil-Free Lubricants

Not all lubricants are liquids, for example, the non-stick coating on a frying pan. Truly in a class of its own, innovators at our Glenn Research Center have created solid lubricant materials to reduce friction and wear in mechanical parts, especially in extremely high heat. This tech could be useful in large engines, valves, turbines and power generation.

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High-Strength Super Elastic Compounds

We needed a better material than iron or steel to prevent corrosion and rust in the International Space Station’s wastewater treatment system. Enter: our high-strength, super elastic compounds. Shock-proof, lightweight, durable and immune to rust, this durable tech has applications in ships, machines, industrial knives and cutters, and engine bearings here on Earth. They also don’t chemically degrade or break down lubricants, a common problem with existing bearing materials.

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Interested in licensing the tech mentioned above? Follow the links to apply through our website, http://technology.nasa.gov.

You can also browse our entire materials and coatings portfolio at http://technology.nasa.gov/materials_and_coatings/.

Follow our NASA Technology Transfer Program on Twitter (@NASAsolutions) for the latest updates on technologies available for licensing.

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1 year ago
: Data visualization of global temperature anomalies progressing from 1880 to 2023 mapped onto Earth. The map uses color to represent anomalies, ranging from blue for below average temperatures, white for temperatures at baseline, and yellows ranging through oranges and reds to represent higher and higher than average temperatures. At the beginning of the time series, the map is primarily blues and whites, with a few spots of yellow, indicating that temperatures overall are below the baseline. As time progresses, the colors shift and move, with less and less blue and white and more and more yellow, then orange, and red. By 2023, the map is mostly yellow with lots of orange and red. The Arctic region, Europe, Asia, North America, central South America, and the Antarctic peninsula are all dark red, indicating the highest temperature anomalies. Credit: NASA’s Scientific Visualization Studio

Six Answers to Questions You’re Too Embarrassed to Ask about the Hottest Year on Record

You may have seen the news that 2023 was the hottest year in NASA’s record, continuing a trend of warming global temperatures. But have you ever wondered what in the world that actually means and how we know?

We talked to some of our climate scientists to get clarity on what a temperature record is, what happened in 2023, and what we can expect to happen in the future… so you don’t have to!

Graph of carbon dioxide emissions from just before 1960 to present day. The X-axis shows years, with each decade listed. The Y-axis shows parts per million of carbon dioxide in the atmosphere. It starts at 300 and runs to 420 ppm. The line on the graph is a fairly straightforward upward trajectory, starting below 320 ppm in 1960 and running to over 420 ppm in 2023. The line on the graph does spike up and down within each year, showcasing the seasonal cycle of carbon dioxide uptake. However, the spikes are extremely minor compared to the upward trajectory. Credit: NOAA

1. Why was 2023 the warmest year on record?

The short answer: Human activities. The release of greenhouse gases like carbon dioxide and methane into the atmosphere trap more heat near Earth’s surface, raising global temperatures. This is responsible for the decades-long warming trend we’re living through.

But this year’s record wasn’t just because of human activities. The last few years, we’ve been experiencing the cooler phase of a natural pattern of Pacific Ocean temperatures called the El Niño Southern Oscillation (ENSO). This phase, known as La Niña, tends to cool temperatures slightly around the world. In mid-2023, we started to shift into the warmer phase, known as El Niño. The shift ENSO brought, combined with overall human-driven warming and other factors we’re continuing to study, pushed 2023 to a new record high temperature.

A climate spiral animation. The chart is circular with the year in the center and months of the year around the outside. There are three concentric circles labeled with measures from negative 2 degrees Fahrenheit to 2 degrees Fahrenheit, with the outer ring being the largest value. As the years count up, a line spirals through the months of the year and around the circle. The line starts with blue hues when temperatures are below average and changes to red and orange hues when temperatures are above average. As the spiral progresses, the lines form a deformed circle that becomes larger and more red, indicating Earth’s warming up to just above 2 degrees Fahrenheit above average. Credit: NASA’s Scientific Visualization Studio

2. So will every year be a record now?

Almost certainly not. Although the overall trend in annual temperatures is warmer, there’s some year-to-year variation, like ENSO we mentioned above.

Think about Texas and Minnesota. On the whole, Texas is warmer than Minnesota. But some days, stormy weather could bring cooler temperatures to Texas while Minnesota is suffering through a local heat wave. On those days, the weather in Minnesota could be warmer than the weather in Texas. That doesn’t mean Minnesota is warmer than Texas overall; we’re just experiencing a little short-term variation.

Something similar happens with global annual temperatures. The globe will naturally shift back to La Niña in the next few years, bringing a slight cooling effect. Because of human carbon emissions, current La Niña years will be warmer than La Niña years were in the past, but they’ll likely still be cooler than current El Niño years.

Visualization of Earth, rotating, speckled with tiny dots in various colors, representing surface temperature measurements taken over the course of a year. Most of the land surfaces are heavily covered in red dots, which represent land measurements. Yellow dots create streaks across the ocean, representing measurements taken by ships. Pink dots irregularly scattered across the ocean represent measurements from floating ocean buoys. Orange dots similar across the ocean represent measurements from moored buoys. Green dots, primarily along coasts, represent tidal gauge measurements. Finally, a handful of blue dots represent all other measurement locations. Credit: NASA’s Scientific Visualization Studio

3. What do we mean by “on record”?

Technically, NASA’s global temperature record starts in 1880. NASA didn’t exist back then, but temperature data were being collected by sailing ships, weather stations, and scientists in enough places around the world to reconstruct a global average temperature. We use those data and our modern techniques to calculate the average.

We start in 1880, because that’s when thermometers and other instruments became technologically advanced and widespread enough to reliably measure and calculate a global average. Today, we make those calculations based on millions of measurements taken from weather stations and Antarctic research stations on land, and ships and ocean buoys at sea. So, we can confidently say 2023 is the warmest year in the last century and a half.

A line graph of temperatures in the Northern Hemisphere Extratropics, Reconstructed Summer, which is May to August, Temperature. The Y-axis is Temperature Anomaly, running from -2 degrees Celsius to 2 degrees Celsius. The X-axis is Years, from 600 to 2023. A jagged black line runs just around the 0 degree Celsius line, with each year slightly higher or lower than the previous, but none jumping above or below 1 and -1 degrees, until just before the year 2000. Around the year 1900, the jagged line begins to climb upwards, reaching to above 1 degree Celsius. At around the time the temperature starts to climb, a red line, indicating NASA’s temperature record, maps very closely to the black line. At the very end, the red line jumps even higher than the black line, reaching almost to 2 degrees Celsius. Credit: NASA/Peter Jacobs using data from N-TREND / Rob Wilson at University of St. Andrews

However, we actually have a really good idea of what global climate looked like for tens of thousands of years before 1880, relying on other, indirect ways of measuring temperature. We can look at tree rings or cores drilled from ice sheets to reconstruct Earth’s more ancient climate. These measurements affirm that current warming on Earth is happening at an unprecedented speed.

4. Why does a space agency keep a record of Earth’s temperature?

It’s literally our job! When NASA was formed in 1958, our original charter called for “the expansion of human knowledge of phenomena in the atmosphere and space.” Our very first space missions uncovered surprises about Earth, and we’ve been using the vantage point of space to study our home planet ever since. Right now, we have a fleet of more than 20 spacecraft monitoring Earth and its systems.

Why we created our specific surface temperature record – known as GISTEMP – actually starts about 25 million miles away on the planet Venus. In the 1960s and 70s, researchers discovered that a thick atmosphere of clouds and carbon dioxide was responsible for Venus’ scorchingly hot temperatures.

The northern hemisphere of Venus, seen by the Magellan spacecraft. Venus is a burnt yellowish circle against the blackness of space. The planet’s surface has darker and yellow orange mottling and darker crater markings. Credit: NASA/JPL

Dr. James Hansen was a scientist at the Goddard Institute for Space Studies in New York, studying Venus. He realized that the greenhouse effect cooking Venus’ surface could happen on Earth, too, especially as human activities were pumping carbon dioxide into our atmosphere.

He started creating computer models to see what would happen to Earth’s climate as more carbon dioxide entered the atmosphere. As he did, he needed a way to check his models – a record of temperatures at Earth’s surface over time, to see if the planet was indeed warming along with increased atmospheric carbon. It was, and is, and NASA’s temperature record was born.

5. If last year was record hot, why wasn’t it very hot where I live?

The temperature record is a global average, so not everywhere on Earth experienced record heat. Local differences in weather patterns can influence individual locations to be hotter or colder than the globe overall, but when we average it out, 2023 was the hottest year.

Just because you didn’t feel record heat this year, doesn’t mean you didn’t experience the effects of a warming climate. 2023 saw a busy Atlantic hurricane season, low Arctic sea ice, raging wildfires in Canada, heat waves in the U.S. and Australia, and more.

Satellite image of smoke over the northeastern United States. The smoke is a light gray, cottony blanket creating an irregular shape over the center of the image. Behind it, the land surface is light browns and greens. Credit: NASA’s Earth Observatory

And these effects don’t stay in one place. For example, unusually hot and intense fires in Canada sent smoke swirling across the entire North American continent, triggering some of the worst air quality in decades in many American cities. Melting ice at Earth’s poles drives rising sea levels on coasts thousands of miles away.

Zoom in from a globe of Earth, showing warming temperatures in yellows, oranges, and reds. The zoom pushes in on the Arctic, which is primarily dark red, indicating the largest temperature anomalies throughout the region. Credit: NASA’s Scientific Visualization Studio/Katy Mersmann

6. Speaking of which, why is the Arctic – one of the coldest places on Earth – red on this temperature map?

Our global temperature record doesn’t actually track absolute temperatures. Instead, we track temperature anomalies, which are basically just deviations from the norm. Our baseline is an average of the temperatures from 1951-1980, and we compare how much Earth’s temperature has changed since then. 

Why focus on anomalies, rather than absolutes? Let’s say you want to track if apples these days are generally larger, smaller, or the same size as they were 20 years ago. In other words, you want to track the change over time.

Apples grown in Florida are generally larger than apples grown in Alaska. Like, in real life, how Floridian temperatures are generally much higher than Alaskan temperatures. So how do you track the change in apple sizes from apples grown all over the world while still accounting for their different baseline weights? 

By focusing on the difference within each area rather than the absolute weights. So in our map, the Arctic isn’t red because it’s hotter than Bermuda. It’s red because it’s gotten relatively much warmer than Bermuda has in the same time frame.

Want to learn more about climate change? Dig into the data at climate.nasa.gov.

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3 years ago

Congratulations to the Winner of the Name the Artemis Moonikin Challenge!

Congratulations To The Winner Of The Name The Artemis Moonikin Challenge!

Congratulations to Campos! After a very close competition among eight different names, the people have decided: Commander Moonikin Campos is launching on Artemis I, our first uncrewed flight test of the Space Launch System rocket and Orion spacecraft around the Moon later this year.

Congratulations To The Winner Of The Name The Artemis Moonikin Challenge!

The name Campos is a dedication to Arturo Campos, electrical power subsystem manager for the Apollo 13 lunar module. He is remembered as not only a key player instrumental to the Apollo 13 crew’s safe return home, but as a champion for equality in the workplace. The final bracket challenge was between Campos and Delos, a reference to the island where Apollo and Artemis were born, according to Greek mythology.

Congratulations To The Winner Of The Name The Artemis Moonikin Challenge!

The Moonikin is a male-bodied manikin previously used in Orion vibration tests. Campos will occupy the commander’s seat inside and wear a first-generation Orion Crew Survival System — a spacesuit Artemis astronauts will wear during launch, entry, and other dynamic phases of their missions. Campos' seat will be outfitted with sensors under the headrest and behind the seat to record acceleration and vibration data throughout the mission. Data from the Moonikin’s experience will inform us how to protect astronauts during Artemis II, the first mission around the Moon with crew in more than 50 years.

Congratulations To The Winner Of The Name The Artemis Moonikin Challenge!

The Moonikin is one of three passengers flying in place of crew aboard Orion on the mission to test the systems that will take astronauts to the Moon for the next generation of exploration. Two female-bodied model human torsos, called phantoms, will also be aboard Orion. Zohar and Helga, the phantoms named by the Israel Space Agency and the German Aerospace Center respectively, will support an investigation called the Matroshka AstroRad Radiation Experiment to provide data on radiation levels during lunar missions.

Congratulations To The Winner Of The Name The Artemis Moonikin Challenge!

Campos, Zohar, and Helga are really excited to begin the journey around the Moon and back. The Artemis I mission will be one of the first steps to establishing a long-term presence on and around the Moon under Artemis, and will help us prepare for humanity's next giant leap — sending the first astronauts to Mars.

Be sure to follow Campos, Zohar, and Helga on their journey by following @NASAArtemis on Facebook, Twitter, and Instagram. Make sure to follow us on Tumblr for your regular dose of space!


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8 years ago

Two New Missions to Explore the Early Solar System

We’ve got big science news…!

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We’ve just added two more science missions to our lineup! The two selected missions have the potential to open new windows on one of the earliest eras in the history of our solar system – a time less than 10 millions years after the birth of our sun.

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The missions, known as Lucy and Psyche, were chosen from five finalists and will proceed to mission formulation.

Let’s take a dive into each mission…

Lucy

Lucy, a robotic spacecraft, will visit a target-rich environment of Jupiter’s mysterious Trojan asteroids. Scheduled to launch in October 2021, the spacecraft is slated to arrive at its first destination, a main asteroid belt, in 2025. 

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Then, from 2027 to 2033, Lucy will explore six Jupiter Trojan asteroids. These asteroids are trapped by Jupiter’s gravity in two swarms that share the planet’s orbit, one leading and one trailing Jupiter in its 12-year circuit around the sun. The Trojans are thought to be relics of a much earlier era in the history of the solar system, and may have formed far beyond Jupiter’s current orbit.

Studying these Trojan asteroids will give us valuable clues to deciphering the history of the early solar system.

Psyche

The Psyche mission will explore one of the most intriguing targets in the main asteroid belt – a giant metal asteroid, known as 16 Psyche, about three times farther away from the sun than is the Earth. The asteroid measures about 130 miles in diameter and, unlike most other asteroids that are rocky or icy bodies, it is thought to be comprised of mostly metallic iron and nickel, similar to Earth’s core.

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Scientists wonder whether psyche could be an exposed core of an early planet that could have been as large as Mars, but which lost its rocky outer layers due to a number of violent collisions billions of years ago.

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The mission will help scientists understand how planets and other bodies separated into their layers early in their histories. The Psyche robotic mission is targeted to launch in October of 2023, arriving at the asteroid in 2030, following an Earth gravity assist spacecraft maneuver in 2024 and a Mars flyby in 2025.

Get even more information about these two new science missions HERE. 

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2 years ago

What is Artemis I?

The SLS and Orion spacecraft can be seen in the foreground with a full Moon to the left of the spacecraft. The SLS is orange, Orion is white, and the Moon is grey and white. A lightning tower is to the left of the Moon.

Credit: NASA/Ben Smegelsky

On November 14, NASA is set to launch the uncrewed Artemis I flight test to the Moon and back. Artemis I is the first integrated flight test of the Space Launch System (SLS) rocket, the Orion spacecraft, and Exploration Ground Systems at NASA’s Kennedy Space Center in Florida. These are the same systems that will bring future Artemis astronauts to the Moon.

The Vehicle Assembly Building (VAB), mobile launcher, and Space Launch System (SLS) rocket can all be seen from a low-angle perspective. The VAB is a large grey and white cube-shaped building with large doors. The mobile launcher is grey, black, and white, with many pipes and levels, and the SLS rocket is orange with two white boosters on either side.

Credit: NASA/Ben Smegelsky

Standing 322 feet (98 meters) tall, the SLS rocket comprises of a core stage, an upper stage, two solid boosters, and four RS-25 engines. The SLS rocket is the most powerful rocket in the world, able to carry 59,500 pounds (27 metric tons) of payloads to deep space — more than any other vehicle. With its unprecedented power, SLS is the only rocket that can send the Orion spacecraft, astronauts, and cargo directly to the Moon on a single mission.

The massive Vehicle Assembly Building (VAB) is a large grey and white cube-shaped building with large doors. It has an American flag on it, along with the NASA meatball logo and the Artemis mission logo. The Space Launch System (SLS) rocket stands to the right of the VAB. The SLS is orange with two white boosters on either side.

Credit: NASA/Kim Shiflett

Before launch, Artemis I has some big help: the Vehicle Assembly Building (VAB) at KSC is the largest single-story building in the world. The VAB was constructed for the assembly of the Apollo/Saturn V Moon rocket, and this is where the SLS rocket is assembled, maintained, and integrated with the Orion spacecraft. 

NASA’s Space Launch System (SLS) rocket, with the Orion capsule atop, slowly rolls out of the Vehicle Assembly Building on the crawler-transporter 2. The crawler is grey with treads and walkways, and the SLS is orange with two white boosters on either side.

Credit: NASA/Kim Shiflett

The mobile launcher is used to assemble, process, and launch the SLS rocket and Orion spacecraft. The massive structure consists of a two-story base and a tower equipped with a number of connection lines to provide the rocket and spacecraft with power, communications, coolant, and fuel prior to launch.

The crawler-transporter 2 is on the left, with the Space Launch System (SLS) rocket on the right of this photo. The crawler is grey with treads and walkways, and the SLS is orange with two white boosters on either side. The sky is blue with fluffy white clouds in the background.

Credit: NASA/Joel Kowsky

Capable of carrying 18 million pounds (8.2 million kg) and the size of a baseball infield, crawler-transporter 2 will transport SLS and Orion the 4.2 miles (6.8 km) to Launch Pad 39B. This historic launch pad was where the Apollo 10 mission lifted off from on May 18, 1969, to rehearse the first Moon landing.

An artist’s rendition of the Orion flight shows a portion of a blue and white Earth in a semi-circle at the bottom of this photo; at the center, a white and grey Orion heads towards a semi-lit Moon in grey. The rest of the image is black, with some small stars dotted throughout.

Credit: NASA/Liam Yanulis

During the launch, SLS will generate around 8.8 million pounds (~4.0 million kg) of thrust, propelling the Orion spacecraft into Earth’s orbit. Then, Orion will perform a Trans Lunar Injection to begin the path to the Moon. The spacecraft will orbit the Moon, traveling 40,000 miles beyond the far side of the Moon — farther than any human-rated spacecraft has ever flown.

An artist’s rendition of the Orion spacecraft is in the foreground in front of the Moon. The perspective is from one of the spacecraft’s solar arrays. The solar array is black, with white and orange dots throughout. The spacecraft has a large NASA logo in red and is grey, white, and black overall.

Credit: NASA/Liam Yanulis

The Orion spacecraft is designed to carry astronauts on deep space missions farther than ever before. Orion contains the habitable volume of about two minivans, enough living space for four people for up to 21 days. Future astronauts will be able to prepare food, exercise, and yes, have a bathroom. Orion also has a launch abort system to keep astronauts safe if an emergency happens during launch, and a European-built service module that fuels and propels the spacecraft.

Commander Moonikin Campos, a manikin, sits aboard the Orion spacecraft in the Orion Crew Survival suit, which is orange with blue straps. The helmet is white with a black tinted visor. A black hose connects to the suit, and the blue background shows NASA and Artemis logos.

Credit: NASA/Frank Michaux

While the Artemis I flight test is uncrewed, the Orion spacecraft will not be empty: there will be three manikins aboard the vehicle. Commander Moonikin Campos will be sitting in the commander’s seat, collecting data on the vibrations and accelerations future astronauts will experience on the journey to the Moon. He is joined with two phantom torsos, Helga and Zohar, in a partnership with the German Aerospace Center and Israeli Space Agency to test a radiation protection vest.

Seen from above is the upside-down, open interior of the Orion capsule with 10 CubeSats secured onto its walls. The interior is yellowish-green and textured, and the exterior of the capsule segment is white with a few black panels. It sits in a processing facility with white walls and servicing platforms surrounding the spacecraft.

Credit: NASA/Cory Huston

A host of shoebox-sized satellites called CubeSats help enable science and technology experiments that could enhance our understanding of deep space travel and the Moon while providing critical information for future Artemis missions.

An artist’s rendition of the Orion spacecraft reentering Earth’s atmosphere. Orion is an orange streak coming from the top right to the left center of the photo, and Earth is seen at night with city lights as dots and a thin strip of atmosphere beneath the Sun.

Credit: NASA/Liam Yanulis

At the end of the four-week mission, the Orion spacecraft will return to Earth. Orion will travel at 25,000 mph (40,000 km per hour) before slowing down to 300 mph (480 km per hour) once it enters the Earth’s atmosphere. After the parachutes deploy, the spacecraft will glide in at approximately 20 mph (32 km per hour) before splashdown about 60 miles (100 km) off the coast of California. NASA’s recovery team and the U.S. Navy will retrieve the Orion spacecraft from the Pacific Ocean.

A large gray ship in the background is deploying small boats, with the Orion spacecraft has large inflatable balloons on top.

Credit: NASA

With the ultimate goal of establishing a long-term presence on the Moon, Artemis I is a critical step as NASA prepares to send humans to Mars and beyond.

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9 years ago

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: 

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

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8 years ago

What are the most important skills an astronaut should have m?

First of all, the basic requirement is a bachelor’s degree in a STEM field, and 3 years of experience (which can also be substituted for by an advanced degree). Other than that, operational experience (things with a technical/active/hands on nature like flying airplanes, SCUBA diving, taking things apart and putting them back together, basic fix-it skills, etc. etc.) is very important, as this is an integral aspect of every day of a space mission.  What we call “expeditionary skills” are also essential, basically the types of things you try to instill in your children, like how to play nicely with others, self care, team care, etc.  I like to think about this on the lines of a camping trip and who you would like to have along with you . . .someone that is competent and can take good care of themselves and their equipment, someone that contributes to the team and helps with group tasks, someone that is good natured and pleasant to be around, etc., someone fun!  These things are increasingly important now that we are regularly doing long duration missions (typical International Space Station mission is 6 months).  Experience living in extreme/remote/isolated environments with small teams is also useful, as it is similar to what we experience as astronauts.     


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5 years ago

Watch Mercury Transit the Sun on Nov. 11

On Nov. 11, Earthlings will be treated to a rare cosmic event — a Mercury transit.

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For about five and a half hours on Monday, Nov. 11 — from about 7:35 a.m. EST to 1:04 p.m. EST — Mercury will be visible from Earth as a tiny black dot crawling across the face of the Sun. This is a transit and it happens when Mercury lines up just right between the Sun and Earth.

Mercury transits happen about 13 times a century. Though it takes Mercury only about 88 days to zip around the Sun, its orbit is tilted, so it's relatively rare for the Sun, Mercury and Earth to line up perfectly. The next Mercury transit isn't until 2032 — and in the U.S., the next opportunity to catch a Mercury transit is in 2049!

How to watch

Our Solar Dynamics Observatory satellite, or SDO, will provide near-real time views of the transit. SDO keeps a constant eye on the Sun from its position in orbit around Earth to monitor and study the Sun's changes, putting it in the front row for many eclipses and transits.

Visit mercurytransit.gsfc.nasa.gov to tune in!

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Our Solar Dynamics Observatory also saw Mercury transit the Sun in 2016.

If you're thinking of watching the transit from the ground, keep in mind that it is never safe to look directly at the Sun. Even with solar viewing glasses, Mercury is too small to be easily seen with the unaided eye. Your local astronomy club may have an opportunity to see the transit using specialized, properly-filtered solar telescopes — but remember that you cannot use a regular telescope or binoculars in conjunction with solar viewing glasses.

Transits in other star systems

Transiting planets outside our solar system are a key part of how we look for exoplanets.

Our Transiting Exoplanet Survey Satellite, or TESS, is NASA’s latest planet-hunter, observing the sky for new worlds in our cosmic neighborhood. TESS searches for these exoplanets, planets orbiting other stars, by using its four cameras to scan nearly the whole sky one section at a time. It monitors the brightness of stars for periodic dips caused by planets transiting those stars.

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This is similar to Mercury’s transit across the Sun, but light-years away in other solar systems! So far, TESS has discovered 29 confirmed exoplanets using transits — with over 1,000 more candidates being studied by scientists!

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Discover more transit and eclipse science at nasa.gov/transit, and tune in on Monday, Nov. 11, at mercurytransit.gsfc.nasa.gov.

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 Mr Neeley, thank you for answering questions! I’ve got two things I want to know- how does the cockpit differ form a normal one? Are there special instruments in there? And do you get tired in long flights? What sort of system is in place to make sure you get sufficient rest if you are flying 12+ hours?


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