Maisons of Tomorrow

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Maisons of Tomorrow

Maisons of Tomorrow

@tomorrowmaisons

Maha Nawaz is the founder of “Maisons of Tomorrow,” a science & technology blog focused on advancing science journalism.

Katılım Ekim 2023
14 Takip Edilen436 Takipçiler
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Once again happily announced that i was the team lead which led the team to discover the faint preliminary moving object SAM2605 (Picture attached showing the data from PAN STARRS) Using data analysis on Astrometrica software for the international asteroid search campaign (IASC)
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Central region of Messier 77 is powered by a black hole surrounded by a thin accretion disc, which itself is surrounded by a thick ring of gas & dust. This thick ring completely obscures our view of the supermassive black hole; its galactic nucleus is also believed to have jets..
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Central region of Messier 77 is powered by a black hole surrounded by a thin accretion disc, which itself is surrounded by a thick ring of gas & dust. This thick ring completely obscures our view of the supermassive black hole; its galactic nucleus is also believed to have jets..
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Central region of Messier 77 is powered by a black hole surrounded by a thin accretion disc, which itself is surrounded by a thick ring of gas & dust. This thick ring completely obscures our view of the supermassive black hole; its galactic nucleus is also believed to have jets..
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Central region of Messier 77 is powered by a black hole surrounded by a thin accretion disc, which itself is surrounded by a thick ring of gas & dust. This thick ring completely obscures our view of the supermassive black hole; its galactic nucleus is also believed to have jets..
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Central region of Messier 77 is powered by a black hole surrounded by a thin accretion disc, which itself is surrounded by a thick ring of gas & dust. This thick ring completely obscures our view of the supermassive black hole; its galactic nucleus is also believed to have jets..
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Central region of Messier 77 is powered by a black hole surrounded by a thin accretion disc, which itself is surrounded by a thick ring of gas & dust. This thick ring completely obscures our view of the supermassive black hole; its galactic nucleus is also believed to have jets..
Maisons of Tomorrow tweet media
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Central region of Messier 77 is powered by a black hole surrounded by a thin accretion disc, which itself is surrounded by a thick ring of gas & dust. This thick ring completely obscures our view of the supermassive black hole; its galactic nucleus is also believed to have jets..
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Head-on collision between two galaxies fueled the unusual triangular-shaped star-birthing frenzy. The interacting galaxy duo is collectively called Arp 143. The pair contains spiral galaxy NGC 2445 at right, along with NGC 2444 at left...
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Head-on collision between two galaxies fueled the unusual triangular-shaped star-birthing frenzy. The interacting galaxy duo is collectively called Arp 143. The pair contains spiral galaxy NGC 2445 at right, along with NGC 2444 at left...
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Head-on collision between two galaxies fueled the unusual triangular-shaped star-birthing frenzy. The interacting galaxy duo is collectively called Arp 143. The pair contains spiral galaxy NGC 2445 at right, along with NGC 2444 at left...
Maisons of Tomorrow tweet media
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Head-on collision between two galaxies fueled the unusual triangular-shaped star-birthing frenzy. The interacting galaxy duo is collectively called Arp 143. The pair contains spiral galaxy NGC 2445 at right, along with NGC 2444 at left...
Maisons of Tomorrow tweet media
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Head-on collision between two galaxies fueled the unusual triangular-shaped star-birthing frenzy. The interacting galaxy duo is collectively called Arp 143. The pair contains spiral galaxy NGC 2445 at right, along with NGC 2444 at left...
Maisons of Tomorrow tweet media
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Head-on collision between two galaxies fueled the unusual triangular-shaped star-birthing frenzy. The interacting galaxy duo is collectively called Arp 143. The pair contains spiral galaxy NGC 2445 at right, along with NGC 2444 at left...
Maisons of Tomorrow tweet media
English
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Head-on collision between two galaxies fueled the unusual triangular-shaped star-birthing frenzy. The interacting galaxy duo is collectively called Arp 143. The pair contains spiral galaxy NGC 2445 at right, along with NGC 2444 at left...
Maisons of Tomorrow tweet media
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Cosmic shock waves that were generated during the collision of 2 massive galaxy clusters more than a billion years ago, forming galaxy cluster Abell 3667. The size of the main shock wave is spanning the entire width of galaxy cluster for a total size of 6.5 million light-years...
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Cosmic shock waves that were generated during the collision of 2 massive galaxy clusters more than a billion years ago, forming galaxy cluster Abell 3667. The size of the main shock wave is spanning the entire width of galaxy cluster for a total size of 6.5 million light-years...
Maisons of Tomorrow tweet media
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Cosmic shock waves that were generated during the collision of 2 massive galaxy clusters more than a billion years ago, forming galaxy cluster Abell 3667. The size of the main shock wave is spanning the entire width of galaxy cluster for a total size of 6.5 million light-years...
Maisons of Tomorrow tweet media
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Cosmic shock waves that were generated during the collision of 2 massive galaxy clusters more than a billion years ago, forming galaxy cluster Abell 3667. The size of the main shock wave is spanning the entire width of galaxy cluster for a total size of 6.5 million light-years...
Maisons of Tomorrow tweet media
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Cosmic shock waves that were generated during the collision of 2 massive galaxy clusters more than a billion years ago, forming galaxy cluster Abell 3667. The size of the main shock wave is spanning the entire width of galaxy cluster for a total size of 6.5 million light-years...
Maisons of Tomorrow tweet media
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Maisons of Tomorrow
Maisons of Tomorrow@tomorrowmaisons·
Cosmic shock waves that were generated during the collision of 2 massive galaxy clusters more than a billion years ago, forming galaxy cluster Abell 3667. The size of the main shock wave is spanning the entire width of galaxy cluster for a total size of 6.5 million light-years...
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