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Magnetar Rotating1970-01-01T00:00:00+00:00Magnetars are rapidly spinning ultra-magnetic neutron stars with a period of between 3 and 12 seconds and are subject to "starquakes". As their phenomenal magnetic field shifts, the stellar crust breaks and emits bursts of gamma rays. These stars are a...PT21Shttps://d38zjy0x98992m.cloudfront.net/5000b36b-505a-4760-af1c-433af02863af/MAGNETAR_UHD_265_xlarge.jpghttps://d38zjy0x98992m.cloudfront.net/5000b36b-505a-4760-af1c-433af02863af/MAGNETAR_UHD_265_mp4_hd_video.mp4https://www.scientific.pictures/media/5000b36b-505a-4760-af1c-433af02863af/pricehttps://www.scientific.pictures/media/5000b36b-505a-4760-af1c-433af02863af/price
Supernova and Remnant SN1AX
This animation shows a very dense white dwarf star devouring a much larger, but less massive, red star. The matter swirls into the white dwarf via an accretion disk. The white dwarf reaches a critical mass and undergoes a thermonuclear explosion that destroys the white dwarf and flings the red star into space. Some debris from the white dwarf travels at very high speed to our region of the Milky Way and is detected by telescopes on Earth.
Animation ID: Supernova_and_Remnant_SN1AX_16sec_HQ
Duration: 00:16
Animation resolution: 1920x1080 pixels @ 30.0 fps, ~74.3 Mbits/s
Published in: ANIMATIONS, Astronomy
Supernova and Remnant SN1AX2019-05-07T06:16:33ZThis animation shows a very dense white dwarf star devouring a much larger, but less massive, red star. The matter swirls into the white dwarf via an accretion disk. The white dwarf reaches a critical mass and undergoes a thermonuclear explosion that d...PT16Shttps://d38zjy0x98992m.cloudfront.net/dc3b4dd8-1df9-44bd-8b0b-65e4cd510c45/Supernova_and_Remnant_SN1AX_16sec_HQ_xlarge.jpghttps://d38zjy0x98992m.cloudfront.net/dc3b4dd8-1df9-44bd-8b0b-65e4cd510c45/Supernova_and_Remnant_SN1AX_16sec_HQ_mp4_hd_video.mp4https://www.scientific.pictures/media/dc3b4dd8-1df9-44bd-8b0b-65e4cd510c45/pricehttps://www.scientific.pictures/media/dc3b4dd8-1df9-44bd-8b0b-65e4cd510c45/price
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