Maisons of Tomorrow

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)

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..

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..

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..

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..

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..

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..

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..

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...

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...

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...

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...

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...

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...

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...

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...

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...

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...

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...

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...

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...