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Keywords: supernova remnant, Tycho Brahe
![Ударная волна от сверхновой в туманности Карандаш](https://images.astronet.ru/pubd/2024/02/23/0001921228/NGC2736_Helge_Buesing1024.preview.jpg)
23.02.2024
This supernova shock wave plows through interstellar space at over 500,000 kilometers per hour. Centered and moving upward in the sharply detailed color composite its thin, bright, braided filaments are actually long ripples in a cosmic sheet of glowing gas seen almost edge-on.
![Волокна остатка сверхновой в Парусах](https://images.astronet.ru/pubd/2024/04/16/0001926417/VelaSnr_CTIO_960.preview.jpg)
16.04.2024
The explosion is over, but the consequences continue. About eleven thousand years ago, a star in the constellation of Vela could be seen to explode, creating a strange point of light briefly visible to humans living near the beginning of recorded history.
![Необычная туманность Pa 30](https://images.astronet.ru/pubd/2024/04/03/0001925079/Pa30V_NASA_960.preview.jpg)
3.04.2024
What created this unusual celestial firework? The nebula, dubbed Pa 30, appears in the same sky direction now as a bright "guest star" did in the year 1181. Although Pa 30's filaments look...
![Озвученный остаток сверхновой туманность Медуза](https://images.astronet.ru/pubd/2024/03/25/0001923985/jellyfish_payne_960.preview.preview.jpg)
25.03.2024
What does a supernova remnant sound like? Although sound is a compression wave in matter and does not carry into empty space, interpretive sound can help listeners appreciate and understand a visual image of a supernova remnant in a new way. Recently, the Jellyfish Nebula (IC 443) has been sonified quite creatively.
![Остаток сверхновой Тихо в рентгеновских лучах](https://images.astronet.ru/pubd/2019/01/14/0001454446/TychoSNR_Chandra_960.preview.jpg)
13.01.2019
What star created this huge puffball? What's pictured is the hot expanding nebula of Tycho's supernova remnant, the result of a stellar explosion first recorded over 400 years ago by the famous astronomer Tycho Brahe. The featured image is a composite of three X-ray colors taken by the orbiting Chandra X-ray Observatory.
![Остаток сверхновой в Парусах](https://images.astronet.ru/pubd/2019/01/10/0001454035/Vela-DSS-New-SS1024.preview.jpg)
10.01.2019
The plane of our Milky Way Galaxy runs through this complex and beautiful skyscape. Seen toward colorful stars near the northwestern edge of the constellation Vela (the Sails), the 16 degree wide, 200 frame...
![Туманность Гама: остаток сверхновой](https://images.astronet.ru/pubd/2022/11/29/0001859575/Gum_Lima_960.preview.jpg)
29.11.2022
Because the Gum Nebula is the closest supernova remnant, it is actually hard to see. Spanning 40 degrees across the sky, the nebula appears so large and faint that it is easily lost in the din of a bright and complex background.
![Химические элементы в остатках звезды](https://images.astronet.ru/pubd/2019/08/03/0001488042/g292chandra.preview.jpg)
1.08.2019
Massive stars spend their brief lives furiously burning nuclear fuel. Through fusion at extreme temperatures and densities surrounding the stellar core, nuclei of light elements ike Hydrogen and Helium are combined to heavier elements like Carbon, Oxygen, etc. in a progression which ends with Iron.
![Ударная волна от сверхновой в туманности Карандаш](https://images.astronet.ru/pubd/2021/04/14/0001734456/Pencil_TurgeonMishra_960.preview.jpg)
14.04.2021
This supernova shock wave plows through interstellar space at over 500,000 kilometers per hour. Near the middle and moving up in this sharply detailed color composite, thin, bright, braided filaments are actually long ripples in a cosmic sheet of glowing gas seen almost edge-on.
![RCW 86: остаток исторической сверхновой](https://images.astronet.ru/pubd/2022/05/30/0001834876/RCW86_MP1024.preview.jpg)
28.05.2022
In 185 AD, Chinese astronomers recorded the appearance of a new star in the Nanmen asterism. That part of the sky is identified with Alpha and Beta Centauri on modern star charts. The new star was visible for months and is thought to be the earliest recorded supernova.
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