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Meet BurstCube! This shoebox-sized satellite is designed to study the most powerful explosions in the cosmos, called gamma-ray bursts. It detects gamma rays, the highest-energy form of light.
BurstCube may be small, but it had a huge journey to get to space.
First, BurstCube was designed and built at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Here you can see Julie Cox, an early career engineer, working on BurstCube’s gamma-ray detecting instrument in the Small Satellite Lab at Goddard.
BurstCube is a type of spacecraft called a CubeSat. These tiny missions give early career engineers and scientists the chance to learn about mission development — as well as do cool science!
Then, after assembling the spacecraft, the BurstCube team took it on the road to conduct a bunch of tests to determine how it will operate in space. Here you can see another early career engineer, Kate Gasaway, working on BurstCube at NASA’s Wallops Flight Facility in Virginia.
She and other members of the team used a special facility there to map BurstCube’s magnetic field. This will help them know where the instrument is pointing when it’s in space.
The next stop was back at Goddard, where the team put BurstCube in a vacuum chamber. You can see engineers Franklin Robinson, Elliot Schwartz, and Colton Cohill lowering the lid here. They changed the temperature inside so it was very hot and then very cold. This mimics the conditions BurstCube will experience in space as it orbits in and out of sunlight.
Then, up on a Goddard rooftop, the team — including early career engineer Justin Clavette — tested BurstCube’s GPS. This so-called open-sky test helps ensure the team can locate the satellite once it’s in orbit.
The next big step in BurstCube’s journey was a flight to Houston! The team packed it up in a special case and took it to the airport. Of course, BurstCube got the window seat!
Once in Texas, the BurstCube team joined their partners at Nanoracks (part of Voyager Space) to get their tiny spacecraft ready for launch. They loaded the satellite into a rectangular frame called a deployer, along with another small satellite called SNoOPI (Signals of Opportunity P-band Investigation). The deployer is used to push spacecraft into orbit from the International Space Station.
From Houston, BurstCube traveled to Cape Canaveral Space Force Station in Florida, where it launched on SpaceX’s 30th commercial resupply servicing mission on March 21, 2024. BurstCube traveled to the station along with some other small satellites, science experiments, as well as a supply of fresh fruit and coffee for the astronauts.
A few days later, the mission docked at the space station, and the astronauts aboard began unloading all the supplies, including BurstCube!
And finally, on April 18, 2024, BurstCube was released into orbit. The team will spend a month getting the satellite ready to search the skies for gamma-ray bursts. Then finally, after a long journey, this tiny satellite can embark on its big mission!
BurstCube wouldn’t be the spacecraft it is today without the input of many early career engineers and scientists. Are you interested in learning more about how you can participate in a mission like this one? There are opportunities for students in middle and high school as well as college!
Keep up on BurstCube’s journey with NASA Universe on X and Facebook. And make sure to follow us on Tumblr for your regular dose of space!
The universe is full of mysteries, and we continue to search for answers. How can we study matter and energy that we can’t see directly? What’s it like inside the crushed core of a massive dead star? And how do some of the most powerful explosions in the universe evolve and interact with their surrounding environment?
Luckily for us, NASA’s Neil Gehrels Swift Observatory is watching the skies and helping astronomers answer that last question and more! As we celebrate its 15-year anniversary, let’s get you up to speed about Swift.
Gamma-ray bursts are the most powerful explosions in the universe. When they occur, they are about a million trillion times as bright as the Sun. But these bursts don’t last long — from a few milliseconds (we call those short duration bursts) to a few minutes (long duration). In the 1960s, spacecraft were watching for gamma rays from Earth — a sign of nuclear testing. What scientists discovered, however, were bursts of gamma rays coming from space!
Gamma-ray bursts eventually became one of the biggest mysteries in science. Scientists wanted to know: What events sparked these fleeting but powerful occurrences?
When it roared into space on a rocket, Swift’s main goals included understanding the origin of gamma-ray bursts, discovering if there were additional classes of bursts (besides the short and long ones), and figuring out what these events could tell us about the early universe.
With Swift as our eyes on the sky, we now know that gamma-ray bursts can be some of the farthest objects we’ve ever detected and lie in faraway galaxies. In fact, the closest known gamma-ray burst occurred more than 100 million light-years from us. We also know that these explosions are associated with some of the most dramatic events in our universe, like the collapse of a massive star or the merger of two neutron stars — the dense cores of collapsed stars.
Swift is still a powerful multiwavelength observatory and continues to help us solve mysteries about the universe. In 2018 it located a burst of light that was at least 10 times brighter than a typical supernova. Last year Swift, along with NASA’s Fermi Gamma-ray Space Telescope, announced the discovery of a pair of distant explosions which produced the highest-energy light yet seen from gamma-ray bursts.
Swift can even study much, much closer objects like comets and asteroids!
How do we study events that happen so fast? Swift is first on the scene because of its ability to automatically and quickly turn to investigate sudden and fascinating events in the cosmos. These qualities are particularly helpful in pinpointing and studying short-lived events.
The Burst Alert Telescope, which is one of Swift’s three instruments, leads the hunt for these explosions. It can see one-sixth of the entire sky at one time. Within 20 to 75 seconds of detecting a gamma-ray burst, Swift automatically rotates so that its X-ray and ultraviolet telescopes can view the burst.
Because of the “swiftness” of the satellite, it can look at a lot in 24 hours — between 50 and 100 targets each day! Swift has new “targets-of-opportunity” to look at every day and can also look at objects for follow up observations. By doing so, it can see how events in our cosmos change over time.
You may have noticed that lots of spacecraft have long names that we shorten to acronyms. However, this isn’t the case for Swift. It’s named after the bird of the same name, and because of the satellite’s ability to move quickly and re-point its science instruments.
When it launched, Swift was called NASA’s Swift Observatory. But in January 2018, Swift was renamed the Neil Gehrels Swift Observatory in memory of the mission’s original principal investigator, Neil Gehrels.
Follow along with Swift to see a typical day in the life of the satellite:
Time for another out of this world comic for starry cosmos month!
This week’s entry, “Gamma Ray Bursts”
http://imagine.gsfc.nasa.gov/science/objects/bursts1.html
http://earthsky.org/space/gamma-ray-bursts-are-the-most-powerful-explosions-in-the-universe