Skip to main content

Depiction of the bipolar planetary nebula by the Hubble telescope.



About 32,000 light-years from Earth is a bipolar planetary nebula, known as M1-63, located in the small southern constellation of Scutum.

Astronomers believe that such a nebula is formed when the star in its center sheds a large amount of material from its outer layers, leaving a brilliant cloud of gas and dust. At the center of the dipole nebula is a binary system of stars, capable of forming butterfly-like shapes.

This is because the material of the shedding star is funneled towards its poles, with the help of a companion, the nebula forms a typical double-lobed structure, such as M1-63.

NASA / ESA Hubble Space Telescope filters image M1-63 through F200W, F350W, F502W, and F814w, new image of M1-63 shows ultraviolet, near-infrared and optical parts of the spectrum in Hubble's wide field. This is illustrated with the help of Camera 3 (WFC3) comments.

Comments

Popular posts from this blog

JWST Just Dropped a Space Banger – Meet HH 30, the Cosmic Baby Star with an Attitude!

  ๐Ÿš€Hubble Found It, Webb Flexed on It! NASA, ESA, and CSA’s James Webb Space Telescope (JWST) just hit us with another mind-blowing “Picture of the Month,” and this time, it’s all about HH 30 —a baby star with a dramatic flair! Sitting pretty in the Taurus Molecular Cloud, this young star is rocking a protoplanetary disc that’s literally glowing with potential future planets. And oh, it’s got some serious jets and a disc wind to show off!   ๐Ÿ’ซ What’s So Special About HH 30? Ever heard of Herbig-Haro objects? No? Cool, neither did most of us until now! These are glowing gas clouds marking the tantrums of young stars as they spit out jets of gas at supersonic speeds. HH 30 is one of them, but with a twist—it’s a prototype edge-on disc, meaning we get a front-row seat to the magic of planet formation!   ๐Ÿ“ก Webb, Hubble & ALMA—The Ultimate Space Detective Team.   To break down HH 30’s secrets, astronomers went full detective mode using:   ✔️...

Solar Storm Shocker: Earth Gets a Cosmic Makeover with Two New Radiation Belts!

  The May 2024 solar storm formed two new radiation belts between the Van Allen Belts, with one containing protons, creating a unique composition never observed before. Picture this: May 2024, the Sun throws a massive tantrum, sending a solar storm hurtling toward Earth. The result? Stunning auroras light up the skies, GPS systems go haywire, and—wait for it—Earth gets two brand-new *temporary* radiation belts! That’s right, our planet just got a cosmic upgrade, thanks to the largest solar storm in two decades. And no, this isn’t a sci-fi movie plot—it’s real science, folks!   Thanks to NASA’s Colorado Inner Radiation Belt Experiment (CIRBE) satellite, scientists discovered these new belts, which are like Earth’s Van Allen Belts’ quirky cousins. Published on February 6, 2025, in the *Journal of Geophysical Research: Space Physics*, this discovery is a game-changer for space research, especially for protecting satellites and astronauts from solar storm shenanigans. ...

NASA/ESA Hubble Telescope Captures Image of Supernova to Aid Distance Measurements.

  The Hubble Space Telescope has recently captured a striking image of a supernova-hosting galaxy, located approximately 600 million light-years away in the constellation Gemini. This image, taken about two months after the discovery of supernova SN 2022aajn, reveals a bright blue dot at the center, signifying the explosive event. Although SN 2022aajn was first announced in November 2022, it has not yet been the subject of extensive research. However, Hubble's interest in this particular supernova lies in its classification as a Type Ia supernova, a type that is key to measuring cosmic distances. Type Ia supernovae occur when a star's core collapses, and they are particularly useful for astronomers because they have a predictable intrinsic brightness. No matter how far away a Type Ia supernova is, it emits the same amount of light. By comparing its observed brightness to this known luminosity, astronomers can calculate how far away the supernova — and its host galaxy — are from...