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That Interstellar object that hurled past Sun last month is from another solar system

Astronomers are now certain that the mysterious object detected hurtling past our sun last month is indeed from another solar system. They have named it 1I/2017 U1(’Oumuamua) and believe it could be one of 10,000 others lurking undetected in our cosmic neighbourhood.

The certainty of its extraterrestrial origin comes from an analysis that shows its orbit is almost impossible to achieve from within our solar system.

Its name comes from a Hawaiian term for messenger or scout. Indeed, it is the first space rock to have been identified as forming around another star. Since asteroids coalesce during the process of planet formation, this object can tell us something about the formation of planets around its unknown parent star.

The latest analyses with ground-based telescopes show that ’Oumuamua is quite similar to some comets and asteroids in our own solar system. This is important because it suggests that planetary compositions like ours could be typical across the galaxy.

Quote:It is thought to be an extremely dark object, absorbing 96% of the light that falls on its surface, and it is red. This colour is the hallmark of organic (carbon-based) molecules. Organic molecules are the building blocks of the biological molecules that allow life to function.

It is widely thought that the delivery of organic molecules to the early Earth by the collision of comets and asteroids made life here possible. ’Oumuamua shows that the same could be possible in other solar systems.

[Image: 6000.jpg?w=620&q=55&auto=format&usm=12&f...0fe2c9a383]

Its characteristics have been published by two independent groups of astronomers. The first group, led by Karen Meech, University of Hawaii, also found that ’Oumuamua was extremely elongated and roughly 400 metres long. Using the European Southern Observatory’s Very Large Telescope(VLT) they also found that it rotated once every 7.3 hours.

The other group of astronomers, led by David Jewitt, University of California Los Angeles, estimated how many other interstellar visitors like it there might be in our solar system.

Surprisingly, they calculate that another 10,000 could be closer to the Sun than the eighth planet, Neptune, which lies 30 times further from the Sun than the Earth. Yet these are currently undetected.

Each of these interstellar interlopers would be just passing through. They are travelling too fast to be captured by the gravity of the Sun. Yet it still takes them about a decade to cross our solar system and disappear back into interstellar space.

If this estimate is correct, then roughly 1,000 enter and another 1,000 leave every year – which means that roughly three arrive and three leave every day.

Using robotic telescopes such as Pan-STARRS, the one that detected ’Oumuamua, to look for asteroids is a priority for astronomers as they concentrate on discovering potentially hazardous objects that could impact Earth.

Imminent upgrades to these survey telescopes and improvements in data processing techniques mean that astronomers will soon be able to detect smaller and fainter objects. They expect a number of these to be interstellar interlopers like ’Oumuamua.
I am pretty sure this is how we all die because I have seen a lot of movies.
Here is a quick summary of how they determined this is an interstellar object.

  • Aspect ratio. It has a 10:1 ratio that is unseen in any other Kuiper belt or Oort cloud object. At most, objects may have a 3:1 ratio!
  • Hue. It has a red tint to it that is also unseen in any other known local asteroid body (Kuiper Belt only. Oort bodies have documented red hues) Theories suggest this is caused by cosmic irradation after hundreds of millions of years of insterstellar travel
  • Composition and outgassing. It is mostly highly dense rock with a chance of metal, and doesn't contain water or ice. This is known because the asteroid doesn't outgas, meaning it has no visible gas vapor around it that would normally be seen as water is boiled off by solar radiation.
  • Trajectory and velocity. It is currently moving at "85,700 miles per hour (38.3 kilometers per second) relative to the Sun" and rapidly leaving our solar system. It will pass Saturn's Orbit in January 2019. It is currently just past Mars, 124 million miles from Earth
It potentially originated near the star Vega, but due to its speed while traveling through interstellar space, Vega has since moved far past where the asteroid was 300,000 years ago.
It was also traveling approximately 196,000 mph (~314,400 kph) after slingshotting past the Sun, which is really, really fast for any rocky body.
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