This image captures the bright central remnant surrounded by stunning expanding rings of gas and dust from the stellar explosion.
Credit: NASA, ESA, R. Kirshner
This image showcases the dense center of the Milky Way, filled with millions of stars, nebulae, and cosmic phenomena. It provides a glimpse into the active and vibrant core of our galaxy.
Credit: ESA/Hubble, NASA, Maximilian Häberle (MPIA)
RS Puppis is a Cepheid variable star surrounded by intricate dust patterns. Its pulsations cause dramatic changes in brightness, offering valuable insights into star behavior and cosmic structures.
Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
M80 is a dense, spherical star cluster located in Scorpius. It reveals thousands of stars packed closely together, offering a glimpse into the evolution of stellar environments.
Credit: The Hubble Heritage Team (AURA/STScI/NASA)
AG Carinae is a massive star surrounded by a nebula of gas and dust. This image reveals the star's brilliant white core, encased in a glowing pink and white shell, showing the interaction between the star and its environment.
Credit: NASA, ESA, STScI
NGC 346 is a star-forming region in the Small Magellanic Cloud, filled with bright, hot stars and ionized gas. It’s a dynamic site of ongoing stellar birth.
Credit: NASA, ESA, and A. Nota (STScI/ESA)
The Bubble Nebula, created by the wind of a massive star, displays a stunning spherical structure formed by gas and dust. It offers a striking view into the powerful processes which shape space.
Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)