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Bima Sakti: Our Galaxy with Dark Doors and Star-Clad Layers

Bima Sakti is not just a faint band of light in the night sky—it is a barred spiral galaxy that is home to the Sun and 100–400 billion other stars. With a diameter of more than 87,000 light-years but only a thousand light-years thick in its spiral arms, its structure resembles a dusty glass disc spun by dark gravity. The location of the Solar System on the edge of the Orion arm makes us limited distant observers—while reminding us how small our place is in the vast cosmos.

26 Jun 20264 min read128,425 viewsBy Redaksi KhatulistiwaWikipedia — Milky Way
Bima Sakti: Our Galaxy with Dark Doors and Star-Clad Layers
Image: Foto: Wikipedia — Milky Way (CC BY-SA 4.0)
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A Band of Light Hiding a Giant Galaxy

In a dark night sky far from light pollution, human eyes can see a faint glowing band—a silvery white with a slight blue at the edges, like spilled milk on an endless black canvas. This is the origin of the name Milky Way, or in traditional Malay: Bima Sakti. However, this appearance is merely an optical illusion due to perspective: the light is not a single object, but a combination of light from billions of stars in our galaxy's spiral arm, too far away to be seen individually. The average distance between stars in this area reaches 5–10 light-years—imagine: if the Sun were a grain of sand in Kuala Lumpur, the nearest star, Proxima Centauri, would be in Singapore. And there are still thousands of grains scattered across the peninsula. That is the scale of Bima Sakti: not just a 'galaxy,' but a coordinated gravitational system containing gas, dust, stars, black holes, and—most mysterious of all—dark matter.

Barred Spiral Structure: Not an Ordinary Disc

Bima Sakti is classified as a barred spiral galaxy—a spiral galaxy with a dense stellar bar stretching from its center. This bar, which is about 27,000 light-years long, functions like a 'cosmic highway': it channels gas and dust toward the center of the galaxy, triggering the formation of new stars in material-rich areas such as the Orion Nebula. Its spiral arms—Orion, Sagittarius, Perseus, and Scutum-Centaurus—are not static structures, but density waves moving slowly through the galactic disc, like ripples on the surface of a pond. The Solar System is located in the Orion arm, approximately 27,000 light-years from the galactic center—roughly at the position of the 'outer edge' of the main disc. The thickness of these arms is only about 1,000 light-years, while the total diameter of the disc reaches 87,400 ± 3,600 light-years. Imagine a CD with a diameter of 30 meters—but only 3 millimeters thick. That is the ratio of thickness to diameter of Bima Sakti.

The Dark Ring That Binds: The Role of Dark Matter

If all the stars, gas, and dust in Bima Sakti were combined, their total mass would not be enough to explain the galaxy's rotational speed—especially in the outer regions. Stars on the edge of the disc rotate much faster than predicted by Newton's laws based on visible mass. The solution? A 'corona' of dark matter extending up to nearly 2 million light-years—more than 20 times the diameter of the visible disc. This region does not emit, absorb, or reflect light, but its existence is proven through its gravitational effects on the movement of stars and satellite galaxies such as the Magellanic Clouds. Within this corona, there are also several old stars that have 'escaped' from the disc—like gravitational exiles still bound to the galaxy through an invisible pull.

Cosmic Neighbors and Our Place in the Cosmic Hierarchy

Bima Sakti is not an isolated entity. It has at least 60 satellite galaxies—most of them dwarf galaxies rich in dark matter—and is one of the main members of the Local Group, a group of galaxies that also includes Andromeda (M31) and Triangulum (M33). The Local Group itself is a small component of the Virgo Supercluster, which in turn is part of the Laniakea Supercluster—a massive cosmic structure spanning 500 million light-years, containing about 100,000 galaxies. In this hierarchy, Bima Sakti is like a small island in an ocean made up of other oceans. This fact reminds us: the existence of Earth is not only dependent on the exact distance from the Sun, but also on the stability of our galaxy's orbit within the local group—because large gravitational disturbances from neighboring galaxies could disrupt planetary orbits or trigger massive stellar explosions.

Unanswered Questions: What Does 'Home' Mean in the Universe?

We call Bima Sakti 'our galaxy'. But what does 'home' mean when the home itself is moving—spinning at a speed of 230 km/s around the galactic center, taking 225–250 million years for a full orbit (known as a cosmic year)? What is 'home' when more than 99.9% of its mass is invisible? And what are the implications for the search for extraterrestrial life, when we know that Bima Sakti contains at least a billion potentially habitable planets—yet most are in complex gravitational zones near the galactic center or in the barren outskirts? These questions are not just philosophical speculations. They drive missions such as Gaia (ESA), which has mapped the positions and movements of over 1.8 billion stars—enabling scientists to build simulations of galactic evolution over 13.6 billion years. In the process, we are not only learning about our galaxy, but also testing the limits of human understanding of space, time, and existence itself.

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Reference: Milky Way — Wikipedia

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