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Cosmic Bedchamber @UCx8LTjlTDpeJ5kf1BFS7-vg@youtube.com

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Welcome to Cosmic Bedchamber ! Immerse yourself in the soot


Welcoem to posts!!

in the future - u will be able to do some more stuff here,,,!! like pat catgirl- i mean um yeah... for now u can only see others's posts :c

Cosmic Bedchamber
Posted 3 months ago

During its 61st close flyby of Jupiter on May 12, 2024, NASA’s Juno spacecraft captured this color-enhanced view of the giant planet’s northern hemisphere. It provides a detailed view of chaotic clouds and cyclonic storms in an area known to scientists as a folded filamentary region. In these regions, the zonal jets that create the familiar banded patterns in Jupiter’s clouds break down, leading to turbulent patterns and cloud structures that rapidly evolve over the course of only a few days.

Citizen scientist Gary Eason made this image using raw data from the JunoCam instrument, applying digital processing techniques to enhance color and clarity.

At the time the raw image was taken, the Juno spacecraft was about 18,000 miles (29,000 kilometers) above Jupiter’s cloud tops, at a latitude of about 68 degrees north of the equator.

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Cosmic Bedchamber
Posted 3 months ago

Which planet is known as the "Red Planet"?

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Cosmic Bedchamber
Posted 3 months ago

Hubble Images NGC 3810
Measuring the distance to truly remote objects like galaxies, quasars, and galaxy clusters is a crucial task in astrophysics, particularly when it comes to studying the early universe, but it’s a difficult one to complete. We can only measure the distances to a few nearby objects like the Sun, planets, and some nearby stars directly. Beyond that, astronomers need to use various indirect methods; one of the most important examines Type Ia supernovae, and this is where the NASA/ESA Hubble Space Telescope excels. NGC 3810, the galaxy featured in this image, was the host of a Type Ia supernova in 2022. In early 2023, Hubble focused on this and a number of other galaxies to closely examine recent Type Ia supernovae. Type Ia supernovae are the result of a white dwarf exploding, and their peak brightness is very consistent. This attribute allows astronomers to use Type Ia supernovae to measure distances: we know how bright a Type Ia supernova should be, so we can tell how far away it must be by how dim it appears. One snag with this method is intergalactic dust. Because intergalactic dust blocks some of the supernova’s light, astronomers need to determine how much light the dust reduces to accurately measure the supernova’s brightness and calculate its distance. Hubble’s unique capabilities offer them a clever way of doing this. Astronomers use Hubble to take images of the same Type Ia supernovae in ultraviolet light, which the dust almost completely blocks out, and in infrared light, which passes through dust nearly unaffected. By carefully noting how much light comes through at each wavelength, astronomers can determine how much dust lies between Hubble and the supernova, letting them confidently calibrate the relationship between a supernova’s brightness and its distance. Hubble’s unique capability to observe in ultraviolet and infrared wavelengths of light in great detail with the same instrument makes it the perfect tool for these types of observations. Indeed, some of the data used to make this beautiful image of NGC 3810 focused on its 2022 supernova. You can see it as a point of light just below the galactic nucleus. There are many ways to measure cosmic distances, but Type Ia supernovae are one of the most useful and accurate tools because they are so bright. Astronomers must use other methods as well, either as an independent check against other distance measurements, or to measure at much closer or farther distances. One such method, that also works for galaxies, is comparing their rotation speed to their brightness; based on that method, NGC 3810 is about 50 million light-years from Earth.

Credits: ESA/Hubble & NASA, D. Sand, R. J. Foley

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Cosmic Bedchamber
Posted 4 months ago

*Hubble: Draco Dwarf Spheroidal*


A team of astronomers analyzed observations by NASA's Hubble Space Telescope taken over a span of 18 years to measure the dynamic motions of stars within the Draco dwarf galaxy. The telescope's extensive baseline and data archive enabled the team to build the most accurate three-dimensional map of the stars' movements within the system. These improved measurements are helping to shed "light" on the mysterious qualities and behavior of dark matter, the universe's invisible "glue." The left image is from the Digitized Sky Survey (DSS). It presents a wider view of the region. The two right-side images are Hubble views.

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Cosmic Bedchamber
Posted 4 months ago

Do You Like Sleeping on a Spaceship? Share Your Thoughts!

As humanity sets its sights on the stars and space travel becomes more of a reality than a fantasy, one intriguing aspect of interstellar life that captures our imagination is sleeping on a spaceship. Whether it’s the serene silence, the lack of gravity, or the futuristic surroundings. But would you actually enjoy it? We want to hear your thoughts!

Please share your thoughts by participating in our poll and leaving a comment below:

Poll Question: Do You Like Sleeping on a Spaceship?
Feel free to elaborate on your choice in the comments. We are excited to hear about your views, concerns, and the aspects you find most appealing or daunting. Whether you’re an avid space enthusiast or a curious dreamer, your input is invaluable in exploring this fascinating aspect of future space travel.


Join the conversation and let’s discuss the future of sleeping in space. Your insights could help shape the way we approach this aspect of long-term space missions, ensuring a comfortable and restful experience for future space travelers.

Thank you for participating in our community poll. Keep dreaming, keep exploring, and maybe one day, you'll find yourself drifting off to sleep among the stars!

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