@spacetelescope@astrodon.social
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spacetelescope

@spacetelescope@astrodon.social

Mission Operations Center for NASA's Webb Space Telescope. Also operating the Hubble Space Telescope and upcoming Roman Space Telescope.

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Did you miss last week’s public lecture? Learn about how advancements in Hubble observation techniques have improved our understanding of dark matter's nature, marking a significant step forward in the study of our universe: https://youtu.be/17SWrVCoh_Y

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Congratulations to STScI assistant astronomer John Wu on being named 2024 Outstanding Young Scientist by the Maryland Academy of Sciences! He has pioneered the discovery of low-mass galaxy candidates: https://bit.ly/3QLkP2w

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in 2009, the final servicing mission launched. SM4 had an ambitious list of tasks designed to bring Hubble to the apex of its scientific capabilities and ensure it would operate for many years to come. (1/3) 🧵

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During SM4 astronauts conducted five spacewalks to install two new instruments, repair two other instruments, and replace key components like gyroscopes and batteries. They also prolonged its life by boosting Hubble to a higher orbit. (2/3)

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SM4 left Hubble at the peak of its scientific capability, and prepared it for many years of further scientific discovery. Hubble is now expected to continue science operations well into the 2030s. Credit: NASA (3/3)

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This pair of galaxies, NGC 2292 and NGC 2293, is beginning to collide, which has started the formation of new stars. These new stars appear like blue pearls in the dusty arm along the bottom.

Discover more about their interaction: https://bit.ly/3TK5wru

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Still under construction in Chile, Rubin Observatory was designed to understand the nature of dark matter and dark energy, and map the Milky Way. The observatory (first image) will have a fast-moving telescope—mount shown in the second image: https://rubinobservatory.org

In the middle of a large round room that is lined with teal-colored steel is a large round telescope mount. Below the mount, humans are standing, dwarfed by the size of the mount.

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This video tours areas of the James Webb Space Telescope’s near-infrared light view of the Pillars of Creation. This area is brimming with gas and dust—which are essential ingredients for star formation.
https://youtube.com/shorts/U2v6jBDslj0

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NASA's Roman Space Telescope could help researchers detect the universe’s FIRST STARS using the wide field of view and rapid survey speed of the upcoming observatory. (1/6) 🧵

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The universe’s earliest stars, known as Population III stars, are notoriously hard to detect with even our most powerful observatories due to their great distance and short lifetime. They were made almost entirely of hydrogen and helium. (2/6)

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will not seek intact stars. Instead, astronomers will hunt for signs of Pop III stars that have been shredded by black holes, creating a bright and energetic phenomenon known as a tidal disruption event (TDE). (3/6)

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TDEs generate light in many wavelengths. The further we look into the early universe, where these early stars primarily reside, the more the optical and UV light is redshifted, into near-infrared wavelengths visible to Roman. (4/6)

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“Roman can go very deep and yet cover a very big area of the sky. That's what's needed to detect a meaningful sample of these TDEs,” said Jane Dai, professor of astrophysics at the University of Hong Kong. (5/6)

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With this proposed strategy for identifying Pop III stars, there’s an opportunity to explore more of the universe’s mysteries, opening up numerous opportunities to better understand not only the early universe, but also galaxies closer to home. (6/6)
https://www.stsci.edu/contents/news-releases/2024/news-2024-204

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A new approach from astronomers seeks to use tidal disruption events—bright and fleeting phenomena—to locate and study the universe’s first stars, known as Population III stars, using the upcoming : https://bit.ly/3JP2spx

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Researchers using may have detected atmospheric gases surrounding 55 Cancri e, a hot rocky exoplanet 41 light-years from Earth. This is the best evidence to date for the existence of any rocky planet atmosphere outside our solar system. (1/6) 🧵

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The much thinner blankets of gas that almost certainly surround some small, rocky exoplanets have remained elusive. Researchers think they may have finally caught a glimpse of a volatile-rich atmosphere surrounding a rocky planet—55 Cancri e. (2/6)

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Light emitted by the hot, highly-irradiated exoplanet 55 Cancri e shows compelling evidence for an atmosphere, probably rich in carbon dioxide or carbon monoxide, which may be bubbling from a vast ocean of lava covering the planet’s surface. (3/6)

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James Webb Space Telescope may have caught a glimpse of an elusive rocky exoplanet atmosphere. Super-hot 55 Cancri e shows compelling evidence for atmospheric gases that may be bubbling up from a vast ocean of lava covering the planet’s surface: https://webbtelescope.pub/3JNwVEa

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STScI is offering a 10-week paid IT internship supporting premiere NASA missions. Interested candidates must be pursuing a degree in information technology, computer science, or software engineering. Application deadline is June 9, 2024. More information: https://lnkd.in/e8HpGuGr

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Black holes are among the most mysterious and fascinating features of the universe, piquing the interest of scientists like Albert Einstein and Stephen Hawking.

These resources help you learn, and educate others, about black holes: https://universe-of-learning.org/informal-educators/science-resources/black-holes

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: While studying one of the most distant galaxies ever observed with the James Webb Space Telescope, astronomers found evidence that GN-z11 hosts a central, supermassive black hole. It is the farthest active supermassive black hole spotted to date: https://webbtelescope.pub/3IiTZtG

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Dwarf galaxy UGC 5340 shines with thousands of ultraviolet-bright stars (colored blue), making it a perfect target for a Hubble survey of 50 nearby, star-forming galaxies. A particularly active pocket of rapid star birth appears in the lower right corner: https://bit.ly/4aq6HU2

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