**Astronomy Picture of the Day**

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2026-06-02T04:10:00Z

Astronomy Picture of the Day

02 June 2026

The Vela Supernova Remnant

Image: https://apod.nasa.gov/apod/image/2606/Vela_Mtanous_2900.jpg

Credit: Not provided

The explosion is over, but the consequences continue. About twelve thousand years ago, a relatively normal star in the constellation Vela suddenly exploded , creating a strange point of light briefly visible to humans living near the beginning of recorded history . The outer layers of the star crashed into the interstellar medium , driving a shock wave that is still visible today. The featured image , taken piecemeal over 60 hours from the Khomas Region of Namibia , captures some of that filamentary and gigantic shock in visible light , with details highlighted by hydrogen (red) and oxygen (blue) emissions. As gas flies away from the detonated star, it decays and reacts with the interstellar medium , producing light in many different colors and energy bands. Remaining at the center of the Vela Supernova Remnant is a pulsar , a star as dense as nuclear matter that spins around more than ten times in a single second.

#APOD #VelaSupernova #VelaSupernovaRemnant #VelaConstellation #SupernovaRemnant #StellarExplosion

https://apod.nasa.gov/apod/ap260602.html

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  "content": "**Astronomy Picture of the Day**\n\n02 June 2026\n\n**The Vela Supernova Remnant**\n\nImage: https://apod.nasa.gov/apod/image/2606/Vela_Mtanous_2900.jpg\n\nCredit: Not provided\n\nThe explosion is over, but the consequences continue. About twelve thousand years ago, a relatively normal star in the constellation Vela suddenly exploded , creating a strange point of light briefly visible to humans living near the beginning of recorded history . The outer layers of the star crashed into the interstellar medium , driving a shock wave that is still visible today. The featured image , taken piecemeal over 60 hours from the Khomas Region of Namibia , captures some of that filamentary and gigantic shock in visible light , with details highlighted by hydrogen (red) and oxygen (blue) emissions. As gas flies away from the detonated star, it decays and reacts with the interstellar medium , producing light in many different colors and energy bands. Remaining at the center of the Vela Supernova Remnant is a pulsar , a star as dense as nuclear matter that spins around more than ten times in a single second.\n\n#APOD #VelaSupernova #VelaSupernovaRemnant #VelaConstellation #SupernovaRemnant #StellarExplosion\n\nhttps://apod.nasa.gov/apod/ap260602.html\n",
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