This image shows just a small part of the region; the full N159 complex spans more than 150 light-years from end to end.
(Credit: ESA/Hubble & NASA, R. Indebetouw)
This image shows just a small part of the region; the full N159 complex spans more than 150 light-years from end to end.
(Credit: ESA/Hubble & NASA, R. Indebetouw)
Dun Briste provides us with a rare glimpse of the Carboniferous. (A 60-million-year-long period lasting from about 359 million to 299 million years ago)
Dun Briste provides us with a rare glimpse of the Carboniferous. (A 60-million-year-long period lasting from about 359 million to 299 million years ago)
Almost every object you see here is a whole galaxy - each with billions of stars of its own!
Credit: ESA/Webb, NASA & CSA, G. Rihtaršič (University of Ljubljana, FMF), R. Tripodi (University of Ljubljana, FMF)
Almost every object you see here is a whole galaxy - each with billions of stars of its own!
Credit: ESA/Webb, NASA & CSA, G. Rihtaršič (University of Ljubljana, FMF), R. Tripodi (University of Ljubljana, FMF)
(Credit: NASA, ESA, and STScI)
(Credit: NASA, ESA, and STScI)
(Credit: ESA/Hubble & NASA, J. Dalcanton, Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA)
(Credit: ESA/Hubble & NASA, J. Dalcanton, Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA)
A physiologist explains how to keep your body feeling warm: www.universal-sci.com/headlines/20...
A physiologist explains how to keep your body feeling warm: www.universal-sci.com/headlines/20...
(Credit: NASA, ESA, CSA, STScI)
(Credit: NASA, ESA, CSA, STScI)
At about 76 million light-years away, it is considered nearby, making it ideal for studying details like star clusters and gas clouds.
(Credit: ESA/Webb, NASA & CSA, A. Leroy)
At about 76 million light-years away, it is considered nearby, making it ideal for studying details like star clusters and gas clouds.
(Credit: ESA/Webb, NASA & CSA, A. Leroy)
A dark, dusty band forms the “body,” hiding the ancient Sun-like core that makes the nebula glow.
Credit: ESA/Webb, NASA & CSA, J. Kastner, M. Zamani (ESA/Webb)
A dark, dusty band forms the “body,” hiding the ancient Sun-like core that makes the nebula glow.
Credit: ESA/Webb, NASA & CSA, J. Kastner, M. Zamani (ESA/Webb)
It has been sculpted and slowly worn away by intense winds and radiation from nearby new-born stars.
Credit: NASA, ESA, CSA, and STScI, A. Pagan (STScI)
It has been sculpted and slowly worn away by intense winds and radiation from nearby new-born stars.
Credit: NASA, ESA, CSA, and STScI, A. Pagan (STScI)
(Credit: ESO/P. Horálek)
(Credit: ESO/P. Horálek)
(Credit: NASA, ESA, CSA, STScI)
(Credit: NASA, ESA, CSA, STScI)
(Credit: Nobuyuki Kayahara)
(Credit: Nobuyuki Kayahara)
(Credit: Nobuyuki Kayahara)
(Credit: Nobuyuki Kayahara)
(Credit: ESA/Hubble & NASA, J. Dalcanton)
(Credit: ESA/Hubble & NASA, J. Dalcanton)
A neutron star, 500,000 times heavier than Earth, is so compact that its diameter doesn't exceed that of New York City.
(Credits: NASA's Goddard Space Flight Center)
A neutron star, 500,000 times heavier than Earth, is so compact that its diameter doesn't exceed that of New York City.
(Credits: NASA's Goddard Space Flight Center)
This celestial structure features a diagonal, bipolar, cylindrical flow of gas, driven outward by intense radiation and stellar winds from a scorching white dwarf at its core
Credit: NASA, ESA, STScI, N. Bartmann (ESA/Hubble)
This celestial structure features a diagonal, bipolar, cylindrical flow of gas, driven outward by intense radiation and stellar winds from a scorching white dwarf at its core
Credit: NASA, ESA, STScI, N. Bartmann (ESA/Hubble)
(The planets and the moon have been enlarged 20 times for visibility).
(Credit: James O’Donoghue / NASA)
(The planets and the moon have been enlarged 20 times for visibility).
(Credit: James O’Donoghue / NASA)
Located 6,300 light-years away in the constellation Hercules, the Blue Ring Nebula is thought to be a short-lived phase after the merger of two stars
(Credit: NASA/JPL-Caltech/NASA/JPL-Caltech/M. Seibert (Carnegie Institution for Science)/K. Hoadley (Caltech)/GALEX Team)
Located 6,300 light-years away in the constellation Hercules, the Blue Ring Nebula is thought to be a short-lived phase after the merger of two stars
(Credit: NASA/JPL-Caltech/NASA/JPL-Caltech/M. Seibert (Carnegie Institution for Science)/K. Hoadley (Caltech)/GALEX Team)
In its core, stars are typically older and smaller; cooler, lower-mass stars appear redder, while hotter stars shine bluer
(Credit: ESA/Hubble & NASA, A. Filippenko - Acknowledgement: M. H. Özsaraç)
In its core, stars are typically older and smaller; cooler, lower-mass stars appear redder, while hotter stars shine bluer
(Credit: ESA/Hubble & NASA, A. Filippenko - Acknowledgement: M. H. Özsaraç)
Webb reveals a restless scene: young, massive stars are chiselling away at gas and dust, while their intense light floods the region with a blue-tinted glow.
(Credit: NASA, ESA, CSA, STScI)
Webb reveals a restless scene: young, massive stars are chiselling away at gas and dust, while their intense light floods the region with a blue-tinted glow.
(Credit: NASA, ESA, CSA, STScI)
Planetary nebulae like the Red Spider Nebula form when ordinary stars like the Sun reach the end of their lives
Credit: ESA/Webb, NASA & CSA, J. H. Kastner (Rochester Institute of Technology)
Planetary nebulae like the Red Spider Nebula form when ordinary stars like the Sun reach the end of their lives
Credit: ESA/Webb, NASA & CSA, J. H. Kastner (Rochester Institute of Technology)
(Credit: ESA/Hubble & NASA, W. Keel)
(Credit: ESA/Hubble & NASA, W. Keel)