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Milky Way Shakes: The Cosmic Collisions That Made Our Galaxy

Milky Way Shakes: The Cosmic Collisions That Made Our Galaxy

By suresh crouchPublished 2 years ago 4 min read
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Milky Way Shakes: The Cosmic Collisions That Made Our Galaxy
Photo by John Benitez on Unsplash

The magnificent new "Cosmic Collisions" offers an amazing and unprecedented understanding of these events - both catastrophic and creative - that shape the Earth, our galaxy, and the changing atmosphere. Then, moving billions of years into the future, a spectacular new cosmic collision predicts the collision of amazing galaxies when two galaxies collide. Then, the glorious new “Earth Collision” takes viewers from the earth's orbit around our galaxy, the Milky Way, to see the dense stars in a distant globular galaxy.

The glorious new Cosmic Collisions also showcased the creation of the bright Moon nearly five billion years ago when the evil planetoid collided with the Earth; a strong collision of two stars at the edge of the galaxy; and the coming collision of our Milky Way galaxy with our immediate neighbor, the Andromeda hurricane, a cosmic catastrophe that will create an elliptical galaxy for billions of years, our Milky Way galaxy, the closest Andromeda galaxy. Incorporating amazing images from space and amazing visuals backed by modern science, a brilliant new cosmic collision reveals the unimaginable collision and explosion that shaped our solar system, changed the course of life on Earth, and continues to transform our galaxy. a dynamic universe. For the first time, Cosmic Collisions also incorporate unusual phenomena that are often invisible, either because they occur in a surprisingly wide area that spans billions of years and billions of miles (as in a galaxy collision) or because they occur rapidly in space. subatomic scale (as in the proton collision at the heart of the Sun).

Starting with this one-dimensional series, each second observing the passing of 40 million years, observers can see how the cosmic collapse has transformed billions of galaxies into the universe and how the Milky Way has shaped many small galaxies during a vast period. . Using the latest astrophysical experiments to create amazing 3D visuals of intergalactic ballet, the two closest galaxies are circular and spontaneous before reconnecting.

With more than 100 billion times the infrared light of the Sun (about three times the total mass of all the stars in the sun), these elements often combine galaxies. When galaxies merge, their black holes “sink” to the center of the newly formed galaxy and eventually merge to form an even larger black hole. The researchers found in a new study that two large black holes were bound by gravity as they inevitably swerved into collisions. An international team of astronomers has observed for the first time the cosmic ballet of two rotating black holes every two years.

Conflict is the amazing and inevitable result of the interaction of gravity with such things as planets, stars, and galaxies. The collision of the atmosphere ended the era of the dinosaurs and changed the very map of the area, changed galaxies, and produced new stars and a new earth. Iron-rich stars are the offspring of stars from a distant galaxy that collapsed on the Milky Way, and their orbits still point to the strange orbit of this cosmic earthquake. The long-running collision shook the air to the point that the stars were scattered throughout the Milky Way.

As the Milky Way grew, developed, and continued its business nearly 10 billion years ago, it encountered a major collision with another small galaxy. This cosmic catastrophe permanently reversed the formation of the Milky Way, creating spirals dense out of a huge black hole in the center of the galaxy. Now a clear picture of how our galaxy, the Milky Way, came to be in the first place of its kind thanks to information collected by the European Space Agency's Gaia satellite. Astronomers have observed a galaxy as unusual as it was 11 billion years ago, and this, they say, may provoke speculations about the early formation of galaxy structures and their evolution.

Evidence suggests that the rare type of galaxy is a collision galaxy, making it one of the first to be found in the first universe. Even the rarest kind of galaxy is huge - the donut hole two thousand times the distance between Earth and Sun in diameter - and it is productive. Kazushi Sakamoto of Taiwan's Sinica Academy and Nick Scoville of the California Institute of Technology have created a molecular gas map in the center of the nearby infrared galaxy with many details using the ALMA array, indicating that it contains a few molecular gas Milky Ways centered on space. the light range of no more than 3,000 light-years - 20 times smaller than the size of a Milky Way gas disk. Designed as a giant dome and described as a “universal fire ring,” it is a rare galaxy with a mass equal to the Milky Way and 11 billion light-years across.

When most of us contemplate the shape of the Milky Way, which contains our Sun and billions of stars, our Sun, we consider the average weight of the plane of massive orbiting stars. The model helped them determine that the waves were not the result of the masses in the middle of the Milky Way. Later, when the Milky Way lost its gas and stellar potential, it could also enter adulthood — our galaxy seems to be changing for the better now, says Philip Hopkins.

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