BREAKING NEWS: #NASAWebb ushers in a new era of exoplanet science with the first unequivocal detection of CARBON DIOXIDE in a planetary atmosphere outside our solar system. (1/5) 🧵
After years of preparation and anticipation, exoplanet researchers are ecstatic! The James Webb Space Telescope has captured an astonishingly detailed rainbow of near-infrared starlight filtered through the atmosphere of a hot gas giant 700 light-years away. (2/5)
The transmission spectrum of exoplanet WASP-39 b, based on a single set of measurements made using Webb’s Near-Infrared Spectrograph and analyzed by dozens of scientists, represents a hat trick of firsts ⬇️. (3/5)
1) #NASAWebb’s first official scientific observation of an exoplanet; 2) the first detailed exoplanet spectrum covering this range of near-infrared colors; and 3) the first indisputable evidence for carbon dioxide in the atmosphere of a planet orbiting a distant star. (4/5)
The results are indicative of #NASAWebb’s ability to spot key molecules like carbon dioxide in a wide variety of exoplanets providing insights into the composition, formation, and evolution of planets across the galaxy. (5/5) #UnfoldTheUniversewebbtelescope.pub/WASP39b
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#NASAWebb will soon reveal unprecedented and detailed views of the universe, with the upcoming release of its first full-color images and spectroscopic data! Below is the list of objects that Webb targeted for these first observations, which will be released on July 12. (1/8)
Carina Nebula: One of the largest and brightest nebulae in the sky, located approximately 7,600 light-years away in the southern constellation Carina. Nebulae are stellar nurseries where stars form. The Carina Nebula is home to many massive stars. (2/8)
WASP-96b (spectrum): A giant planet outside our solar system, composed mainly of gas. The planet, located nearly 1,150 light-years from Earth, orbits its star every 3.4 days. It has about half the mass of Jupiter, and its discovery was announced in 2014. (3/8)
Bright stars create unique patterns called diffraction spikes, which are produced as light bends around the sharp edges of a telescope. Most reflecting telescopes—including #NASAWebb—show spikes as light interacts with the primary mirror and struts that support the mirror. (1/5)
Light—which has wave-like properties—tends to radiate from a point outward. When light waves interact, they can either become more amplified or cancel each other out. These areas of amplification and cancellation form the light and dark spots in diffraction patterns. (2/5)
Primary mirrors in reflecting telescopes cause light waves to interact as they direct light to the secondary mirror. So, even if a telescope had no struts, it would still create a diffraction pattern. The shape of the mirror and any edges it has determine its pattern. (3/5)
#NASAWebb will revolutionize our understanding of the lifecycles of stars, starting at the very beginning. Protostars like HH 47 eject light-year-long jets even while accumulating the hydrogen needed to begin nuclear fusion and shine. (1/4)
Credit: NASA.
With its powerful infrared sensitivity and resolution, #NASAWebb is capable of peering into star-forming regions across our entire galaxy—like R136—where previous infrared telescopes were limited to dust clouds within our own galactic neighborhood. (2/4)
Credit: NASA/ESA.
Sunlike stars end their lives by gently ejecting their outer layers to form what’s known as a planetary nebula. #NASAWebb will look at NGC 6302 and nebulas like it to learn how chemical elements are recycled throughout our galaxy. (3/4)
Who is ready to be “thrown” through a loop? A supermassive black hole’s feedback loop to be exact! Decoder: In these images, RED indicates COLD and TEAL indicates HOT. (1/7)
Supermassive black holes, which lie at the centers of galaxies, are voracious! They periodically “sip” or “gulp” from COLD swirling disks of gas and dust that orbit them. Where there’s lots of very cold gas, stars can begin to form—but it also falls onto the black hole. (2/7)
As a result of “nom, nom, noming” on all that delicious cold gas, supermassive black holes launch outflows in the form of radiation, jets, and wind! (It’s gettin’ hot in here!) (3/7)
This was definitely the selfie seen around the world! But HOW was #NASAWebb able to take a selfie? Joe DePasquale, senior science visuals developer at @stsci, digs in! 🧵 <1/9>
DePasquale: The press release states that there is a specially designed pupil imaging lens (PIL) in one of Webb’s main imaging instruments known as NIRCam. What is a PIL anyway? <2/9>
DePasquale: PIL then is a specially designed lens whose sole purpose is to provide a clear image of that aperture allowing you to see where light enters the system. You can see it on the lower left side in this diagram of NIRCam. <3/9>
As they die, massive stars—at least 8 times bigger than our sun—populate the universe with new elements. How does that happen? We’ll show you each step! 👇🏼 (1/7)
Credit: NASA, ESA, and L. Hustak (STScI).
Stars don’t normally explode 💥 because they balance two forces: gravity, which wants to crush all of the gas towards the center, and pressure from fusion, which pushes outward.
The first stage of a star’s life is fueled by hydrogen-to-helium fusion. (2/7)
Over a star’s lifetime, the core will run out of fuel, contract and heat up, and begin new fusion reactions.
This creates a multi-layered core, with heavier elements fusing in the hot, dense center and shells of lighter elements fusing at cooler temperatures. (3/7)