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Speeding Stars

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I have always admired the night sky, especially on a hot summer night when the sky reveals its most beautiful face adorned with the infinite dots of gentle illumination that light up the sky. That is the “star.” No matter how old, millions or billions of years, they are all born in nebulae, the clouds of dust, and mostly hydrogen gas.

Looking at the sky, have you ever wondered if they ever move? We’ve all learned that the stars rise and set each night, but that’s just Earth’s rotation. The star never moved. What about actual movement across the vast canvas of space?

Despite appearances, stars are constantly on the move, traversing the cosmos at tremendous speeds (thousands of km/hr). While their immense distances make this motion imperceptible to our naked eyes. That’s because they are billions and billions of miles away from us. If you’re thinking why does it matter if it’s far, we should still be able to see something moving that fast even from far away. If you’re thinking that, then you’re wrong. You do experience this when moving in a car or a train; you will notice that the farther a tree or an object is, the slower it seems to move, and the closer the tree or the object is, it just goes right by us so fast.

Eons of Change: From Fixed to Moving

For centuries, astronomers believed stars held fixed positions. But in 1718, Edmond Halley, famed for his discovery of the eponymous comet, brought to light the reality of stellar motion. Comparing ancient star charts to his own observations, he found that three prominent stars – Sirius, Arcturus, and Aldebaran – had shifted positions since their cataloging by the Greek astronomer Hipparchus around 130 BC. This revelation shattered the illusion of a static universe and unveiled the concept of “proper motion” – the stars’ unique movements through space. A deeper understanding of celestial dynamics.

A Balancing Act of Distance and Perception

Our Sun, for example, hurtles through the Milky Way galaxy at a speed of 800,000 kilometers per hour! That is like crossing the United States in just 20 seconds – that’s the mind-boggling speed of our star! Yet, due to their immense distances (trillions of kilometers!), this stellar motion appears incredibly slow from our vantage point.
The closer a star is to us, the faster its perceived movement. Just like nearby trees seem to whiz by while driving compared to distant mountains, closer stars exhibit a more noticeable “proper motion.”

Barnard’s Star: The Speedy Champion

The current record holder for the fastest “proper motion” is Barnard’s Star, a red dwarf star only 6 light-years away. Even with its impressive speed, it would take this star almost 200 years to move just half the width of a full moon in the night sky. However, this motion is enough to be tracked by telescopes over a few years.

Mapping the Stellar Waltz: Unveiling the Universe’s Secrets

By studying “proper motion,” astronomers can unravel various cosmic mysteries. It helps:

Distinguish between nearby objects and distant imposters: A true companion star will have the same “proper motion” as its host star, while a background galaxy will remain stationary.

Weigh black holes: By observing the motions of stars orbiting Sagittarius A* (the Milky Way’s central black hole), astronomers have estimated its mass to be around 4 million times that of our Sun!

Build 3D maps of the galaxy: By tracking stellar movements over time, astronomers can create a three-dimensional map of our Milky Way neighborhood, revealing stellar associations and clusters.

The Grand Encounter: Andromeda and the Milky Way

The European Space Agency’s Gaia mission is meticulously charting the proper motions of billions of stars in our galaxy and beyond. This data is helping us understand the future of our cosmic neighborhood.

Our closest galactic neighbor, Andromeda, is hurtling towards us at over 100 kilometers per second. While a collision seems inevitable, its sideways motion (which “proper motion” helps us measure) is uncertain. A slow sideways motion could lead to a grand collision in 4 billion years, while a faster motion might see Andromeda gracefully miss us.

Unveiling the Future

While the verdict on the Andromeda-Milky Way collision is still out, one thing is certain: the stars hold the answers. As time unfolds, their “proper motion” will become even more evident, revealing the secrets of our galactic dance. So, the next time you gaze up at the night sky, remember – the seemingly static stars are actually engaged in a magnificent cosmic ballet, whispering tales of the universe’s.

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