Location: In the Scorpius constellation
Distance from Earth: About 44,000 light-years
Object type: Globular star cluster
Discovered by: James Dunlop in 1826
Each tiny point of light in this image is its own star - and there are more than a million of them! This stunning image captured by the Hubble Telescope depicts NGC 6441, a globular cluster that weighs about 1.6 million times the mass of our Sun. Globular clusters like NGC 6441 are groups of old stars held together by their mutual gravitational attraction, appearing nearly spherical in shape due to the density of stars that comprises them. This particular cluster is one of the most massive and luminous in our Milky Way Galaxy. It is also home to a planetary nebula and four pulsars (rotating neutron stars that emit beams of radiation at steady intervals, detected when the beams are aimed at Earth).
Read more information about NGC 6441 here.
Right now, the Hubble Space Telescope is delving into its #StarrySights campaign! Find more star cluster content and spectacular new images by following along on Hubble’s Twitter, Facebook, and Instagram.
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What's Up for June? Saturn at its best! Plus, good views of Mars, Jupiter and Jupiter's moons continue from dusk to dawn.
You don't have to stay up late to see Jupiter, Mars and Saturn this month, because they're all visible soon after sunset. Jupiter is the brightest of the three, visible in the western sky all evening.
The four Galilean moons are easily visible in binoculars or telescopes. If you think you're seeing 5 moons on June 10th, you're not. One of them is a distant star in the constellation Leo.
For telescope viewers, the time near Mars' closest approach to Earth, May 30th this year, is the best time to try to see the two moons of Mars: Phobos and Deimos. It takes patience, very steady skies and good charts! Mars is still large and bright in early June, but it fades as speedy Earth, in its shorter orbit around the sun, passes it.
Saturn has been close to Mars recently. This month Saturn reaches opposition, when Saturn, Earth and the sun are in a straight line with Earth in the middle, providing the best and closest views of the ringed beauty and several of its moons. You'll be able to make out cloud bands on Saturn, in delicate shades of cream and butterscotch. They're fainter than the bands of Jupiter. Through a telescope you'll see Saturn's rings tilted about as wide as they get: 26 degrees.
You'll also have a ring-side view of the Cassini division, discovered by Giovanni Domenico Cassini, namesake of our Cassini spacecraft, orbiting Saturn since 2004 and continuing through September 2017. When you look at Saturn through a telescope, you can't help but see several of its 4 brightest moons, and maybe more. If you just see one, that's Titan, 50% larger than our own moon. A telescope can also reveal more moons, like Saturn's two-colored moon Iapetus. It takes 3 months to orbit Saturn, and it's fairly easy to see.
There's a bright comet visible this month, Comet PanSTARRS. It's best seen from the southern hemisphere, but it's also visible from the U.S. low in the morning sky. Comet PanSTARRS can be seen through a telescope near the beautiful Helix Nebula on June 4, but it is visible all month.
Watch the full June “What’s Up” video for more: https://youtu.be/M7RtIa9zBYA
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Our solar system is huge, so let us break it down for you. Here are a few things you should know this week:
1. Science at the Edge
As the New Horizons spacecraft speeds away at more than 31,000 miles per hour (14 km/s) it continues to explore the Kuiper Belt, the region of icy bodies beyond Neptune. New Horizons has now twice observed 1994 JR1, a 90-mile-wide object orbiting more than 3 billion miles from the sun.
2. A Spaceship, Refined
This artist’s rendering shows our Europa mission spacecraft, which is being developed for a launch sometime in the 2020s. The mission will place a spacecraft in orbit around Jupiter to explore the giant planet’s moon Europa. This updated concept image shows tow large solar arrays extending from the sides of the spacecraft, to which the mission’s ice-penetrating radar antennas are attached. A saucer-shaped high-gain antenna is also side mounted with a magnetometer boom placed next to it. Find out more about the spacecraft HERE.
3. Sojourn at Saturn
The Cassini spacecraft is hard at work this week, orbiting Saturn to study the planet and its rings. The recent pictures are spectacular, take a look at them HERE.
4. Talking Juno
Our Juno mission arrives at Jupiter on July 4, and that presents a unique opportunity for educators, science communicators and anyone interested in space exploration. We are providing a growing set of Juno-related information resources. Take a look at them HERE.
5. Now THAT’S a Long Distance Call
How do explorers on Earth talk to astronauts and robotic spacecraft flung across the far reaches of space? They use the remarkable technology deployed by our Space Communications and Navigation (SCaN) Program Office. This month, SCaN is celebrating its 10th anniversary of managing the ultimate network. Find out how it works HERE.
Want to learn more? Read our full list of the 10 things to know this week about the solar system HERE.
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We will select between eight and 14 new astronaut candidates from among a record-breaking applicant class of more than 18,300, almost three times the number of applications the agency received in 2012 for the recent astronaut class, and far surpassing the previous record of 8,000 in 1978.
The candidates will be announced at an event at our Johnson Space Center in Houston, Texas at 2 p.m. EDT on June 7. You can find more information on how to watch the announcement HERE.
Applicants must meet the following minimum requirements before submitting an application.
Bachelor’s degree from an accredited institution in engineering, biological science, physical science, computer science or mathematics.
Degree must be followed by at least 3 years of related, progressively responsible, professional experience or at least 1,000 hours of pilot-in-command time in jet aircraft
Ability to pass the NASA Astronaut physical.
For more information, visit: https://astronauts.nasa.gov/content/faq.htm
There have been 22 classes of astronauts selected from the original “Mercury Seven” in 1959 to the most recent 2017 class. Other notable classes include:
The fourth class in 1965 known as “The Scientists: because academic experience was favored over pilot skills.
The eighth class in 1978 was a huge step forward for diversity, featuring the first female, African American and Asian American selections.
The 16th class in 1996 was the largest class yet with 44 members – 35 U.S. astronauts and 9 international astronauts. They were selected for the frequent Space Shuttle flights and the anticipated need for International Space Station crewmembers.
The 21st class in 2013 was the first class to have 50/50 gender split with 4 female members and 4 male members.
They could be assigned on any of four different spacecraft: the International Space Station, our Orion spacecraft for deep space exploration or one of two American-made commercial crew spacecraft currently in development – Boeing’s CST-199 Starliner or the SpaceX Crew Dragon.
These astronauts will be part of expanded crews aboard the space station that will significantly increase the crew time available to conduct the important research and technology demonstrations that are advancing our knowledge for missions farther into space than humans have gone before, while also returning benefits to Earth. They will also be candidates for missions beyond the moon and into deep space aboard our Orion spacecraft on flights that help pave the way for missions to Mars.
After completing two years of general training, these astronaut candidates will be considered full astronauts, eligible to be assigned spaceflight missions. While they wait for their turn, they will be given duties within the Astronaut Office at Johnson Space Center. Technical duties can range from supporting current missions in roles such as CAPCOM in Mission Control, to advising on the development of future spacecraft.
The first two years of astronaut candidate training will focus on the basic skills astronauts need. They’ll practice for spacewalks in Johnson’s 60-foot deep swimming pool, the Neutral Buoyancy Lab, which requires SCUBA certification. They’ll also simulate bringing visiting spacecraft in for a berthing to the space station using its robotic arm, Canadarm2, master the ins and outs of space station system and learn Russian.
And, whether they have previous experience piloting an aircraft of not, they’ll learn to fly our fleet of T-38s. In addition, they’ll perfect their expeditionary skills, such as leadership and fellowship, through activities like survival training and geology treks.
They will join a team that supports missions going on at many different NASA centers across the country, but they’ll also interact with commercial partners developing spaceflight hardware. In addition, they will work with our international partners around the globe: ESA (the European Space Agency, the Canadian Space Agency, the Japan Aerospace Exploration Agency and the Russian space agency, Roscosmos.
All 18,353 of the applications submitted were reviewed by human resources experts to determine if they met the basic qualifications. Those that did were then each reviewed by a panel of about 50 people, made up primarily of current astronauts. Called the Astronaut Rating Panel, that group narrowed to applicants down to a few hundred of what they considered the most highly qualified individuals, whose references were then checked.
From that point, a smaller group called the Astronaut Selection Board brought in the top 120 applicants for an intense round of interviews and some initial medical screening tests. That group is further culled to the top 50 applicants afterward, who are brought back for a second round of interviews and additional screening. The final candidates are selected from that group.
Each applicant selected to become an astronaut receives a phone call from the head of the Flight Operations Directorate at our Johnson Space Center and the chief of the astronaut office. They’re asked to share the good news with only their immediate family until their selection has been officially announced.
Astronaut candidates will report for duty at Johnson Space Center in August 2017, newly fitted flight suits in tow, and be sworn into civil service. Between their selection and their report for duty, they will make arrangements to leave their current positions and relocate with their family to Houston, Texas.
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It’s no secret the Sun affects us here on Earth in countless ways, from causing sunburns to helping our houseplants thrive. The Sun affects other objects in space, too, like asteroids! It can keep them in place. It can move them. And it can even shape them.
Asteroids embody the story of our solar system’s beginning. Jupiter’s Trojan asteroids, which orbit the Sun on the same path as the gas giant, are no exception. The Trojans are thought to be left over from the objects that eventually formed our planets, and studying them might offer clues about how the solar system came to be.
Over the next 12 years, NASA’s Lucy mission will visit eight asteroids—including seven Trojans— to help answer big questions about planet formation and the origins of our solar system. It will take the spacecraft about 3.5 years to reach its first destination.
How does the Sun affect what Lucy might find?
Credits: Astronomical Institute of CAS/Petr Scheirich
The Sun makes up 99.8% of the solar system’s mass and exerts a strong gravitational force as a result. In the case of the Trojan asteroids that Lucy will visit, their very location in space is dictated in part by the Sun’s gravity. They are clustered at two Lagrange points. These are locations where the gravitational forces of two massive objects—in this case the Sun and Jupiter—are balanced in such a way that smaller objects (like asteroids or satellites) stay put relative to the larger bodies. The Trojans lead and follow Jupiter in its orbit by 60° at Lagrange points L4 and L5.
The Sun can move and spin asteroids with light! Like many objects in space, asteroids rotate. At any given moment, the Sun-facing side of an asteroid absorbs sunlight while the dark side sheds energy as heat. When the heat escapes, it creates an infinitesimal amount of thrust, pushing the asteroid ever so slightly and altering its rotational rate. The Trojans are farther from the Sun than other asteroids we’ve studied before, and it remains to be seen how sunlight affects their movement.
The Sun can break asteroids, too. Rocks expand as they warm and contract when they cool. This repeated fluctuation can cause them to crack. The phenomenon is more intense for objects without atmospheres, such as asteroids, where temperatures vary wildly. Therefore, even though the Trojans are farther from the Sun than rocks on Earth, they’ll likely show more signs of thermal fracturing.
Like everything in our solar system, asteroids are battered by the solar wind, a steady stream of particles, magnetic fields, and radiation that flows from the Sun. For the most part, Earth’s magnetic field protects us from this bombardment. Without magnetic fields or atmospheres of their own, asteroids receive the brunt of the solar wind. When incoming particles strike an asteroid, they can kick some material off into space, changing the fundamental chemistry of what’s left behind.
Follow along with Lucy’s journey with NASA Solar System on Instagram, Facebook, and Twitter, and be sure to tune in for the launch at 5 a.m. EDT (09:00 UTC) on Saturday, Oct. 16 at nasa.gov/live.
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Observers all over the world are hoping to catch a glimpse of Comet NEOWISE before it speeds away into the depths of space, not to be seen again for another 6,800 years.
For those that are, or will be, tracking Comet NEOWISE there will be a few particularly interesting observing opportunities this week.
Over the coming days it will become increasingly visible shortly after sunset in the northwest sky.
The object is best viewed using binoculars or a small telescope, but if conditions are optimal, you may be able to see it with the naked eye. If you’re looking in the sky without the help of observation tools, Comet NEOWISE will likely look like a fuzzy star with a bit of a tail. Using binoculars will give viewers a good look at the fuzzy comet and its long, streaky tail.
Here’s what to do:
Find a spot away from city lights with an unobstructed view of the sky
Just after sunset, look below the Big Dipper in the northwest sky
Each night, the comet will continue rising increasingly higher above the northwestern horizon.
There will be a special bonus for viewers observing comet NEOWISE from the northeast United States near Washington, DC. For several evenings, there will be a brief conjunction as the International Space Station will appear to fly near the comet in the northeast sky. Approximate times and locations of the conjunctions are listed below (the exact time of the conjunction and viewing direction will vary slightly based on where you are in the Washington, DC area):
July 17 : ~10:56 p.m. EDT = NEOWISE elevation: ~08° Space Station elevation: ~14°
July 18 : ~10:08 p.m. EDT = NEOWISE elevation: ~13° Space Station elevation: ~18°
July 19 : ~10:57 p.m. EDT = NEOWISE elevation: ~10° Space Station elevation: ~08°
July 20 : ~10:09 p.m. EDT = NEOWISE elevation: ~17° Space Station elevation: ~07°
It will be a late waning Moon, with the New Moon on July 20, so the viewing conditions should be good as long as the weather cooperates.
Comet NEOWISE is about 3 miles across and covered in soot left over from its formation near the birth of our solar system 4.6 billion years ago - a typical comet.
Comets are frozen leftovers from the formation of the solar system composed of dust, rock and ices. They range from a few miles to tens of miles wide, but as they orbit closer to the sun, they heat up and spew gases and dust into a glowing head that can be larger than a planet. This material forms a tail that stretches millions of miles.
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On Friday, March 29, Christina Koch and Anne McClain were scheduled to perform a spacewalk together to upgrade the power systems of the International Space Station. It would have been the first all-female spacewalk in human history. While disappointing to many people, after the last spacewalk was completed on March 22, NASA changed the assignments to protect the safety of the crew and the timing of the mission. Now, Christina Koch and Nick Hague will be performing this upcoming spacewalk, leaving lots of people wondering: What’s the deal?
Spacesuits are not “one size fits all.” We do our best to anticipate the spacesuit sizes each astronaut will need, based on the spacesuit size they wore in training on the ground, and in some cases astronauts train in multiple sizes.
McClain trained in both a medium and a large on Earth. However, living in microgravity can change the size of your body! In fact, Anne McClain has grown two inches since she launched to the Space Station.
McClain realized that the medium she wore during the March 22 spacewalk was a better fit for her in space. She had planned to wear a large during the March 29 spacewalk.
In a tweet, McClain explained: “This decision was based on my recommendation. Leaders must make tough calls, and I am fortunate to work with a team who trusts my judgement. We must never accept a risk that can instead be mitigated. Safety of the crew and execution of the mission come first.”
To provide each astronaut the best fitting spacesuit during their spacewalks, Koch will wear the medium torso on March 29, and McClain will wear it again on April 8.
The spacesuit is a mini spaceship that keeps our astronauts alive while they are spacewalking!
Astronauts train several hours on Earth in the Neutral Buoyancy Lab for every hour they spend spacewalking. Spacewalks are the most physically demanding thing we ask astronauts to do, which is why an optimally fitted spacesuit is important to completing the assigned tasks and overall mission!
We do have enough torsos. The spacesuit takes into account more than 80 different body measurements to be configured for each astronaut. The suit has three sizes of upper torso, eight sizes of adjustable elbows, over 65 sizes of gloves, two sizes of adjustable waists, five sizes of adjustable knees and a vast array of padding options for almost every part of the body.
In space, we have two medium hard upper torsos, two larges and two extra larges; however, one of the mediums and one of the extra larges are spares that would require 12 hours of crew time for configuration.
Configuring the spare medium is a very methodical and meticulous process to ensure the intricate life support system — including the controls, seals, and hoses for the oxygen, water and power as well as the pressure garment components — are reassembled correctly with no chance of leaks.
Nothing is more important than the safety of our crew!
12 hours might not seem like a long time, but the space station is on a very busy operational schedule. An astronaut's life in space is scheduled for activities in five minute increments. Their time is scheduled to conduct science experiments, maintain their spaceship and stay healthy (they exercise two hours a day to keep their bones and muscles strong!).
The teams don’t want to delay this spacewalk because two resupply spacecraft – Northrop Grumman Cygnus and SpaceX cargo Dragon – are scheduled to launch to the space station in the second half of April. That will keep the crew very busy for a while!
NASA does not make assignments based on gender.
The first female space shuttle commander, the first female space station commander and the first female spacewalker were all chosen because they the right individuals for the job, not because they were women. It is not unusual to change spacewalk assignments as lessons are learned during operations in space.
McClain became the 13th female spacewalker on March 22, and Koch will be the 14th this Friday – both coincidentally during Women’s History Month! Women also are filling two key roles in Mission Control: Mary Lawrence as the lead flight director and Jaclyn Kagey as the lead spacewalk officer.
An all-female spacewalk is inevitable! As the percentage of women who have become astronauts increases, we look forward to celebrating the first spacewalk performed by two women! McClain, Koch (and Hague!) are all part of the first astronaut class that was 50 percent women, and five of the 11 members of the 2017 astronaut candidate class are also women.
You can watch the upcoming spacewalk on March 29 at 6:30 ET, which is one in a series to upgrade the station’s power technology with new batteries that store power from the solar arrays for the station to use when it is in orbital night.
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Did the training ever get so hard that you would regret getting into this?
No because the end goal is space!
Flying directly through thick plumes of smoke may seem more harrowing than exciting. But for members of the CAMP2Ex science team, the chance to fly a P-3 Orion straight through clouds of smoke billowing off fires from Borneo this week was too good an opportunity to pass up.
CAMP2Ex stands for the Cloud, Aerosol and Monsoon Processes in the Philippines Experiment. The 2, by the way, is silent.
It’s a field campaign based out of Clark in the Philippines, flying our P-3, a Learjet and collaborating with researchers on the research vessel Sally Ride to understand how tiny particles in the atmosphere affect cloud formations and monsoon season.
The tiny aerosol particles we’re looking at don’t just come from smoke. Aerosol particles also come from pollution, billowing dust and sea salt from the ocean. They can have an outsized effect on weather and climate, seeding clouds that bring rain and altering how the atmosphere absorbs the Sun’s heat.
The smoke we were flying Monday came from peat fires, burning through the soil. That’s pretty unusual — the last time Borneo had these kind of fires was in 2015, so it was a rare opportunity to sample the chemistry of the smoke and find out what’s mixing with the air.
The planes are loaded with instruments to learn more about aerosol particles and the makeup of clouds, like this high-speed camera that captures images of the particles in flight.
One instrument on the plane collects droplets of cloud water as the plane flies through them, and on the ground, we test how acidic and what kind of particles form the cloud drops.
All of these measurements are tools in improving our understanding of the interaction between particles in the air and clouds, rainfall and precipitation in the Pacific Ocean.
Learn more about the CAMP2Ex field campaign, here!
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The eclipse should be visible to some extent across the continental U.S. Here’s map of its path.
Our eclipse page can help you find the best viewing locations by longitude and latitude: eclipse.gsfc.nasa.gov/SEgoogle/SEgoogle2001/SE2017Aug21Tgoogle.html
Want to know more about citizen science projects? Find a list of citizen science projects for the eclipse: https://eclipse.aas.org/resources/citizen-science
Get your eclipse viewing safety glasses beforehand: eclipse2017.nasa.gov/safety
In this interactive, 3D simulation of the total eclipse on August 21, 2017, you can see a view of the eclipse from anywhere on the planet:
http://eyes.jpl.nasa.gov/eyes-on-eclipse.html
Join the conversation on social media. Tag your posts: #Eclipse2017.
Twitter: @NASASolarSystem, @NASA, @NASASunEarth Facebook: NASA Solar System
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Get dazzled by the true spectrum of solar beauty. From fiery reds to cool blues, explore the vibrant hues of the Sun in a mesmerizing color order. The images used to make this gradient come from our Solar Dynamics Observatory. Taken in a variety of wavelengths, they give scientists a wealth of data about the Sun. Don't miss the total solar eclipse crossing North America on April 8, 2024. (It's the last one for 20 years!) Set a reminder to watch with us.
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