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New observations from the NASA/ESA Hubble Space Telescope have provided the first spectroscopic observations of two of these super-puffy planets, which are located in the Kepler-51 system.
Resembling a nightmarish beast rearing its head from a crimson sea, this celestial object is actually just a pillar of gas and dust.
Fomalhaut system
This diagram compares observations made with the NASA/ESA Hubble Space Telescope of two 'hot Jupiter'-class planets orbiting very closely to different sunlike stars. Astronomers measured how light from each parent star is filtered through each planet's atmosphere.
These images, taken a year apart by the NASA/ESA Hubble Space Telescope, reveal a shadow moving counterclockwise around a gas and dust disc encircling the young star TW Hydrae.
This illustration from a hypothetical planet in a distant ultra-dense galaxy reveals a sky packed with thousands of stars. There are 200 times more stars in this sky than in our Earth's night-time sky. The ultra-dense galaxies existed about 11 billion years ago