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Could We Save The Earth From An Asteroid Impact?

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Space debris, coronal mass ejections from the sun, and UAP’s are just some of the known hazards of the final frontier.

As we learn more about the fabric that makes up the universe all around us, we are becoming increasingly aware of the many dangers which lurk in the vastness of the space all around us.

Near earth objects are among the most concerning of these threats, as it becomes more apparent that we need adequate defenses for the planet.

According to recent reports, an asteroid identified as 1994 PC1 flew by at approximately 1.2 million miles away from our planet.

While this is a comfortable distance from our perspective, in cosmic terms it was fairly close, and it begs the question: are we prepared to deflect large objects from outer space?

Finding a solution to this problem was touted as one of the main objectives of the newest branch of the U.S. military—Space Force.

Plans to develop and test methods of asteroid deflection and planetary defense are underway, but these efforts are still in their infancy.

The recent near earth object was recorded by NASA:

Daily Caller provided a deeper look into the near earth object 1994 PC1:

The asteroid is categorized as a “potentially hazardous” object by If it were to hit the planet, it would carve out a crater over nine miles wide and 2,000 feet deep, according to an impact calculator developed by Imperial College London and Purdue University.

A previous report from NBC News highlights NASA plans to stop asteroids before they impact:

In the third objective, NASA is asked to come up with new ways to deflect an asteroid heading toward Earth.

This involves developing technologies for “rapid-response NEO reconnaissance missions,” in which a spacecraft could launch toward an Earth-bound asteroid and somehow change the space rock’s course so that it no longer posed a threat.

NASA had plans to attempt this with the Asteroid Redirect Mission (ARM) in 2021, but the Trump administration scrapped that mission in 2017.

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