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What NASA saw during JO1's member,, a thread-
#SHO: ๐๐ ๐๐จ๐ซ๐๐๐ฎ๐ฌ ๐๐๐๐ฎ๐ฅ๐
This young stellar grouping is only a few million years away and resides in the 30 Doradus Nebula, a turbulent star-birth region in the Large Magellanic Cloud, a satellite galaxy of our Milky Way
This young stellar grouping is only a few million years away and resides in the 30 Doradus Nebula, a turbulent star-birth region in the Large Magellanic Cloud, a satellite galaxy of our Milky Way
#REN: ๐๐ฅ๐ฎ๐ญ๐จ ๐๐ฒ๐ฌ๐ญ๐๐ฆ
This image was taken through a red filter captures Pluto and three of his satellites. The largest object in this image is Pluto and the second largest is Charon.
This image was taken through a red filter captures Pluto and three of his satellites. The largest object in this image is Pluto and the second largest is Charon.
#RUKI: ๐๐ฎ๐ฆ๐๐๐ฅ๐ฅ ๐๐๐๐ฎ๐ฅ๐
Known as a planetary nebula, it is the result of an old star that has shed its outer layers in a glowing display of color. It was the first planetary nebula ever discovered.
Known as a planetary nebula, it is the result of an old star that has shed its outer layers in a glowing display of color. It was the first planetary nebula ever discovered.
#JUNKI: ๐๐ก๐ข๐ซ๐ฅ๐ฉ๐จ๐จ๐ฅ ๐๐๐ฅ๐๐ฑ๐ฒ
The graceful, winding arms of the majestic spiral galaxy M51 appear like a grand spiral staircase sweeping through space. They are actually long lanes of stars and gas laced with dust.
The graceful, winding arms of the majestic spiral galaxy M51 appear like a grand spiral staircase sweeping through space. They are actually long lanes of stars and gas laced with dust.
#KEIGO: ๐๐ญ๐๐ซ ๐๐ฅ๐ฎ๐ฌ๐ญ๐๐ซ ๐๐ซ๐ฎ๐ฆ๐ฉ๐ฅ๐๐ซ ๐๐
This cluster of stars is located 8K light-years away in a huge star-forming region: the Carina Nebula. The cluster is only 500K years old &has one of the highest concentrations of bright, massive stars in the entire Milky Way.
This cluster of stars is located 8K light-years away in a huge star-forming region: the Carina Nebula. The cluster is only 500K years old &has one of the highest concentrations of bright, massive stars in the entire Milky Way.
#TAKUMI: ๐๐๐ฅ๐๐ฑ๐ข๐๐ฌ ๐ข๐ง ๐ญ๐ก๐ ๐๐ซ๐จ๐ญ๐ก ๐๐ญ๐ซ๐ข๐ฉ
his field of galaxies is just a small part of a cosmic tapestry Hubble imaged as part of the All-wavelength Extended Groth Strip International Survey. In it are galaxies of all shapes, sizes, colors, and distances.
his field of galaxies is just a small part of a cosmic tapestry Hubble imaged as part of the All-wavelength Extended Groth Strip International Survey. In it are galaxies of all shapes, sizes, colors, and distances.
#SYOYA: ๐๐๐ฅ๐๐๐ญ๐ข๐ ๐๐๐ง๐ญ๐๐ซ
This infrared image of the center of our Milky Way galaxy reveals a population of massive stars and complex structures in the hot ionized gas that swirls around the galactic core.
This infrared image of the center of our Milky Way galaxy reveals a population of massive stars and complex structures in the hot ionized gas that swirls around the galactic core.
#SHOSEI: ๐๐๐ฅ๐๐ฑ๐ฒ ๐๐ฅ๐ฎ๐ฌ๐ญ๐๐ซ ๐๐๐๐ฅ๐ฅ ๐๐๐๐
The giant elliptical galaxy in the center of this image is the most massive &brightest member of galaxy cluster Abell 2261. More than a million light-years wide, the galaxy is about 10 times bigger than our Milky Way galaxy
The giant elliptical galaxy in the center of this image is the most massive &brightest member of galaxy cluster Abell 2261. More than a million light-years wide, the galaxy is about 10 times bigger than our Milky Way galaxy
#SUKAI: ๐๐ญ๐๐ซ๐ฌ ๐ข๐ง ๐ญ๐ก๐ ๐๐๐ฅ๐๐๐ญ๐ข๐ ๐๐จ๐ซ๐
These colorful stars reside at the
of Milky Way galaxy, about 26K light-years from 
.Red-giant stars coexist w/ more younger cousins, the smaller, white, sun-like stars, in this crowded region of our galaxyโs central hub
These colorful stars reside at the
of Milky Way galaxy, about 26K light-years from .Red-giant stars coexist w/ more younger cousins, the smaller, white, sun-like stars, in this crowded region of our galaxyโs central hub
#SHION: ๐๐๐ฅ๐๐ฑ๐ฒ ๐๐๐
The arms of the "grand design" spiral galaxy M81 are filled with young, bluish, hot stars. The greenish regions in the image are bright, gaseous clouds where new stars are forming.
The arms of the "grand design" spiral galaxy M81 are filled with young, bluish, hot stars. The greenish regions in the image are bright, gaseous clouds where new stars are forming.
#MAME: ๐๐ฐ๐๐ง ๐๐๐๐ฎ๐ฅ๐
This pic captures a small region in the Swan Nebula,a hotbed of star formation. The wave-like patterns of gas have been sculpted & illuminated by a torrent of ultraviolet radiation from young, massive stars, which lie outside the pic to the upper left
This pic captures a small region in the Swan Nebula,a hotbed of star formation. The wave-like patterns of gas have been sculpted & illuminated by a torrent of ultraviolet radiation from young, massive stars, which lie outside the pic to the upper left
As for #JO1 debut date: ๐๐๐ฅ๐๐ฑ๐ฒ ๐
๐จ๐ซ๐ง๐๐ฑ ๐
The dust lanes& star clusters of this giant elliptical galaxy,known as Fornax A, give evidence that the galaxy formed from a past merger of 2 gas-rich galaxies. Its also one of the strongest sources of radio emission in the sky
The dust lanes& star clusters of this giant elliptical galaxy,known as Fornax A, give evidence that the galaxy formed from a past merger of 2 gas-rich galaxies. Its also one of the strongest sources of radio emission in the sky
