Warm nights can be enjoyable times to watch for meteor showers. From Earth, streaking meteors seem to appear as shooting stars millions of miles away. But, a picture from the International Space Station clearly captures a meteor BELOW the 250 miles altitude of the space station. The visible streaks are caused by tiny particles burning up in Earth's atmosphere due to friction at altitudes of 50 miles above the surface.
Most meteors are the size of a grain of sand. The Eta Aquarids peak during early-May each year. Eta Aquarid meteors are known for their speed. These meteors are fast—traveling at about 148,000 mph (66 km/s) into Earth's atmosphere. Fast meteors can leave glowing "trains" (incandescent bits of debris in the wake of the meteor) which last for several seconds to minutes. Delta Aquarids meteor showers are visible from mid-July with peak activity on July 28 or 29.
Scientists were expecting to find an intermediate-mass black hole at the heart of the globular cluster NGC 6397, but instead they found evidence of a concentration of smaller black holes lurking there.
#space #Shorts #BlackHoles
Credit:
ESA/Hubble, N. Bartmann
Track Greta Sting, Kevin MacLeod, Creative Commons Attribution 4.0. https://creativecommons.org/licenses/by/4.0/
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This video captured by ESO’s OmegaCAM on the VLT Survey Telescope, shows a lonely galaxy known as Wolf-Lundmark-Melotte, or WLM for short, that lies in the rather faint constellation of Cetus (The Sea Monster). Although considered part of our Local Group of dozens of galaxies, WLM stands alone at the group’s outer edges as one of its most remote members. In fact, the galaxy is so small and secluded that it may never have interacted with any other Local Group galaxy — or perhaps even any other galaxy in the history of the Universe.
Credit:
ESO.
Acknowledgement: VST/Omegacam Local Group Survey
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https://www.youtube.com/watch?v=Dv3kZkx1lk4
The Universe... it appears to be a vast, cold, quiet expanse of space.
But is it?
X-ray astronomy satellite ASTRO-H will take flight to unravel the hot, violent Universe hidden deep in the night sky.
(Credit: JAXA)
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https://www.youtube.com/watch?v=eAIUP7kGIbQ
An aurora is a natural light display in the sky , predominantly seen in the high latitude (Arctic and Antarctic) regions.
Aurorae are caused by cosmic rays, solar wind and magnetospheric plasma interacting with the upper atmosphere .
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This sequence of color-enhanced images shows how quickly the viewing geometry changes for NASA’s Juno spacecraft as it swoops by Jupiter. The images were obtained by JunoCam.
Once every 53 days, Juno swings close to Jupiter, speeding over its clouds. In just two hours, the spacecraft travels from a perch over Jupiter’s north pole through its closest approach (perijove), then passes over the south pole on its way back out. This sequence shows 11 color-enhanced images from Perijove 8 (Sept. 1, 2017) with the south pole on the left (11th image in the sequence) and the north pole on the right (first image in the sequence).
The first image on the right shows a half-lit globe of Jupiter, with the north pole approximately at the upper center of the image close to the terminator -- the dividing line between night and day. As the spacecraft gets closer to Jupiter, the horizon moves in and the range of visible latitudes shrinks. The second and third images in this sequence show the north polar region rotating away from the spacecraft's field of view while the first of Jupiter's lighter-colored bands comes into view. The fourth through the eighth images display a blue-colored vortex in the mid-southern latitudes near Points of Interest "Collision of Colours," "Sharp Edge," "Caltech, by Halka," and "Structure01." The Points of Interest are locations in Jupiter’s atmosphere that were identified and named by members of the general public. Additionally, a darker, dynamic band can be seen just south of the vortex. In the ninth and tenth images, the south polar region rotates into view. The final image on the left displays Jupiter's south pole in the center.
From the start of this sequence of images to the end, roughly 1 hour and 35 minutes elapsed. #space #astrophysics #universe
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https://www.youtube.com/watch?v=ooYo0NNHByU
Engineers on the ground will remotely orchestrate a complex sequence of deployments in the hours and days immediately after the launch of the James Webb Space Telescope. This animation shows the nominal sequence for these deployments.
#WEBB #UnfoldTheUniverse #Shorts
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https://www.youtube.com/watch?v=Qo3OZ9k1K9g
With a view 100 times bigger than that of NASA’s Hubble Space Telescope, the Wide Field Infrared Survey Telescope WFIRST will aid researchers in their efforts to unravel the secrets of dark energy and dark matter, and explore the evolution of the cosmos. It also will discover new worlds outside our solar system and advance the search for worlds that could be suitable for life. Scientists participating in the mission discuss the spacecraft, the science, and its potential. Slated to launch in the mid-2020s, the observatory will operate at a gravitational balance point known as Earth-sun L2, which is located about 930,000 miles from Earth and directly opposite the sun.
Related:
https://www.youtube.com/watch?v=9Y6VPD9H0_8
Credit: NASA's Goddard Space Flight Center/Wiessinger
This video is public domain and may be downloaded at: http://svs.gsfc.nasa.gov/cgi-bin/details.cgi?aid=12153
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Since its birth, fifty years ago, ESO has helped to improve our knowledge of the Universe by means of successive generations of powerful optical ground-based telescopes. But there are other ways to collect the light from distant objects. In this episode, we discover how ESO has helped astronomers to explore the Universe at longer wavelengths, such as the infrared and radio regimes.
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https://www.youtube.com/watch?v=2xO7F6wgxgs