The warm embrace of a star could be the stuff of nightmares. 😱 Small stars like our Sun puff out into red giants at the ends of their lives, engulfing anything orbiting too close, but brown dwarf WD 1202-024 B may have survived just such a hug. #MondayMotivation
NASA Exoplanets
NASA Exoplanets
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Data from Swift’s three telescopes has contributed to about 7,000 published scientific papers. Swift leaves behind a treasure trove of 12 TB of data — equivalent to about 600 HD movies — that astronomers will continue to comb through for years to come. t.co/y048ZptEf9 🔗 go.nasa.gov/4sucstU
Doing some pumpkin carving this weekend? Make space on your front porch for some out-of-this-world jack-o’-lanterns! 🎃 Check out these stencils featuring some cosmic cartoon characters, @NASAWebb, @NASARoman, and more. Download them here: t.co/RnyEsx4ATp
LISA is an @ESA-led mission in partnership with @NASA that will detect and measure ripples in space-time called gravitational waves. LISA’s three spacecraft will fly in a triangular formation that follows Earth as it orbits the Sun. What object could fill this triangle?
Each arm of this triangle will be about 1.6 million miles long, big enough that our Sun would snugly fit inside. Gravitational waves from cosmic events will ripple across the triangle, slightly changing the distances between the spacecraft. Meet LISA: t.co/QMRE0g44Yy 🔗 nasa.gov/lisa
With its quick reflexes, flexible scheduling, and multiwavelength vision, our Neil Gehrels Swift Observatory has made discoveries with nearly every NASA space telescope during its 22 years in space. As the mission winds down, let’s see how Swift’s collaboratio... 🔗 x.com/NASAUniverse/status/2...
@chandraxray Observatories often complement each other. Take gamma-ray burst 230307A, as an example. Our Fermi telescope detected it, then Swift and others pinpointed it, allowing @NASAWebb to find the signature of tellurium, an element rarer than platinum on Earth. t.co/cAw5RbPjUT
@chandraxray @NASAWebb In 2019, our planet-hunting TESS telescope saw a black hole tear apart a star in a tidal disruption event. Rapid follow-up by Swift and other observatories — on the ground and in space — caught intriguing details of this rare, star-destroying blast. t.co/bJqxxIC6XI
With its quick reflexes, flexible scheduling, and multiwavelength vision, our Neil Gehrels Swift Observatory has made discoveries with nearly every NASA space telescope during its 22 years in space. As the mission winds down, let’s see how Swift’s collaboratio... 🔗 x.com/NASAUniverse/status/2...
Last year, Swift teamed up with our IXPE, @ChandraXray, and NuSTAR telescopes to study a black hole jet in the Perseus galaxy cluster. They traced the X-rays to interactions between light and particles, helping us better understand black hole environments. t.co/LGNTx80mBH 🔗 go.nasa.gov/4jJ9q2D
#TBT to Oct. 17, 2002, when @ESA's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) launched to study the cosmos using the highest-energy form of light. INTEGRAL contributed to many discoveries, sometimes in tandem with @NASA observatories. t.co/NO7ka7BWtM 🔗 go.nasa.gov/4s911rk
Only a few dozen brown dwarfs have been studied in detail with space-based telescopes, but SPHEREx’s ability to measure 102 colors makes it uniquely suited to studying these “dark wanderers.” Learn more:
Our Swift observatory’s UVOT (Ultraviolet/Optical Telescope) was designed to investigate some of the universe’s brightest bursts, but it’s also helped us study stars, galaxies, and more. Since Swift's launch in 2004, how many images has the UVOT taken? Check back for the answer!
If you guessed the UVOT has taken over 1,500,000 images, you’re right! Each one features a piece of the sky, combining with data from Swift’s other two telescopes to build a treasure trove that'll fuel discoveries for years to come. More about Swift: t.co/ABePiPT5Ra
Say Betelgeuse three times and its companion may appear! Scientists thought that the 10th brightest star had a companion, and a @NASAAmes scientist spotted it using @NOIRLabAstro’s Gemini North telescope in Hawaii and a @NASA-built camera: t.co/YASGVKgVNB 🔗 go.nasa.gov/4yGatoj
#OTD in 2000, the High Energy Transient Explorer (HETE-2) launched from Kwajalein Atoll. An international collaboration, it was launched to help detect and unravel the mystery of gamma-ray bursts. Learn more about HETE-2 here: t.co/Xp1ZFQ1eos 🔗 go.nasa.gov/4y7NJfX
Most TESS planets were discovered by catching dips in starlight from orbiting planets. But it recently identified a planet through another method called microlensing, where light from a distant star is magnified by a nearer star passing in front of it: t.co/W3bZkG7HOs
We’ve only scratched the surface of TESS discoveries — there are thousands of additional exoplanet candidates awaiting confirmation! Learn more about our search for distant worlds: t.co/ymLMXge902
Puffy, Jupiter-sized WD 1856 b is the first intact planet found closely orbiting a much smaller white dwarf star. The process of forming these compact cool stars usually destroys nearby planets, so scientists were surprised to find one: t.co/mxYF3cYvlP 🔗 go.nasa.gov/4zi3JwP
Not all planets are solo acts! TESS helped find a family of six exoplanets smaller than Neptune in synchronized orbits around their star. Their repetitive orbital dance can teach us about planet formation and evolution … and be set to music: t.co/zyDKOmk5qK
TESS stares at wide patches of the sky, watching for changes that might indicate a planet orbiting a star. Within its first three months of observations, TESS confirmed three exoplanets … and also spotted supernovae, comets, flaring stars, and more: t.co/q8UuxdOH7K 🔗 go.nasa.gov/4yGZjzS
In 2020, the TESS team announced its first discovery of an Earth-sized world orbiting within its star’s habitable zone, the range of distances where conditions may be just right for liquid water to exist on a planet’s surface: t.co/FAmjFraWRv
The universe is better with friends. As our Swift Observatory approaches the end of its mission, we’re celebrating its 21+ years in orbit — and the friends it's made — with some new galactic images. Check out this thread for more, or download yours here: t.co/5... 🔗 chandra.si.edu/photo/2026/s...
The universe is better with friends. As our Swift Observatory approaches the end of its mission, we’re celebrating its 21+ years in orbit — and the friends it's made — with some new galactic images. Check out this thread for more, or download yours here: t.co/5... 🔗 chandra.si.edu/photo/2026/s...
🎵 Twinkle, twinkle, little bat! How I wonder what you’re at! Up above the world you fly, Like a tea-tray in the sky. 🎵 Perhaps the Hatter spied this cosmic teacup, captured by @chandraxray (blue) and @NASAHubble (red and green)? More: t.co/TDRY0bE70G #MadHatterDay 🔗 chandra.si.edu/photo/2019/t...
Sometimes when we look out into the shadowy depths of the cosmos, we find it looking right back. #MondayMotivation
#OTD in 1952, the namesake for our Neil Gehrels Swift Observatory was born. He led development of Swift, a first-of-its-kind satellite designed to automatically repoint to study fleeting cosmic explosions called gamma-ray bursts. Learn more about Swift: t.co/Sy3iiYkL0G 🔗 nasa.gov/swift
Also #OTD, @NASAHubble imaged nebula N44, which is filled with glowing gas, dark dust lanes, and stars of different ages. It also hosts a dark, starry gap called a “superbubble,” whose presence is something of a mystery. What did Hubble see on your day? t.co/gWs7DGccWK 🔗 go.nasa.gov/47vxuOR
Black holes don’t emit light, but the regions around them can shine bright! Data from our NuSTAR telescope and @ESA_XMM from 13 distant and luminous supermassive black holes helped astronomers explore how their coronae produce intense X-ray light: t.co/9m77Ft936H 🔗 nustar.caltech.edu/news/nus...
Because gamma rays can’t be focused with current technology, Swift’s Burst Alert Telescope works differently than typical telescopes. The Burst Alert Telescope uses a mask made of lead tiles that stop gamma rays, casting shadows on the detectors below. t.co/004femyq7q 🔗 go.nasa.gov/4xXmEw4
Sightseeing? Don’t forget to send a postcard! 📬 We’ve got you covered if your travels take you to the edge of a black hole. Tour the universe with the Traveler on NASA+: t.co/xyGwOiLhQ2 🔗 go.nasa.gov/4dzElun
Swift’s Ultraviolet/Optical Telescope tested out its vision on galaxy M101, also known as the Pinwheel galaxy. Shortly after that, it started regular observations, including enabling Swift’s first distance determinations to gamma-ray bursts in March 2005. t.co/YCzJWzhb7z 🔗 go.nasa.gov/4dfudXq
In 2018, Swift’s Ultraviolet/Optical Telescope took its millionth image, which captured an active galaxy that appeared to exhibit some unusual behavior. To mark the occasion, this mosaic was created from images taken by the telescope. Zoom in to explore. t.co/mrzxuMymFa 🔗 go.nasa.gov/4yI8L6d
As its name suggests, the Ultraviolet/Optical Telescope detects both UV and optical (or visible) light. When it spots a burst, the telescope goes through a preprogrammed series of observations, turning its filter wheel to capture specific wavelengths. t.co/BDPTI05WUC 🔗 go.nasa.gov/4hlPocP
Swift’s X-Ray Telescope caught X-rays from a gamma-ray burst Swift detected on Jan. 17, 2005, while the burst was still going on! It was the first time any X-ray telescope had seen such an early stage of a burst. Learn more: t.co/52Em7FGsPO 🔗 go.nasa.gov/4hz21js
During its 20+ years in orbit, Swift has observed much, much more than gamma-ray bursts. And just a couple years ago, Swift learned a new trick: Astronomers developed an automated search of Swift’s view of the X-ray sky to find sudden changes. t.co/4KCtkFgMQi
Though the commercial mission to boost our Swift observatory ended without an attempt to raise the spacecraft’s orbit, NASA and Katalyst Space have gained valuable experience that will benefit future in-space servicing programs. 🧵
Innovative operation of Swift extended the time it was at a serviceable altitude, an approach that could be adapted for other missions. Katalyst also performed demonstrations of their satellite-servicing technology. More lessons learned: t.co/WzmoYW0xt5 🔗 go.nasa.gov/3Vg9m04