Published by Patrick Mutisya · 14 days ago
A galaxy is a massive system that contains billions to trillions of stars, together with gas, dust and dark matter, all bound together by gravity.
The Milky Way, our own galaxy, is a typical spiral galaxy. It is estimated to contain roughly \$10^{11}\$ (one hundred billion) stars.
The Sun is a G‑type main‑sequence star located in one of the Milky Way’s spiral arms, called the Orion‑Cygnus Arm. It is the star closest to Earth and provides the light and heat necessary for life.
While the Sun is only about \$1.5 \times 10^{8}\,\text{km}\$ (1 astronomical unit, AU) from Earth, the next nearest star system, Alpha Centauri, lies about \$4.37\$ light‑years away – more than \$270{,}000\$ times farther than the Sun.
Most stars that we see in the night sky are at distances of tens to thousands of light‑years, far beyond the reach of ordinary measuring tools.
Light travels at a constant speed in vacuum:
\$c = 3.00 \times 10^{8}\ \text{m s}^{-1}\$
The distance light travels in one year is called a light‑year (ly). It can be calculated as:
\$\text{1 ly} = c \times (\text{1 year}) = 3.00 \times 10^{8}\ \text{m s}^{-1} \times 3.156 \times 10^{7}\ \text{s} \approx 9.46 \times 10^{15}\ \text{m}\$
| Unit | Equivalent Distance |
|---|---|
| 1 AU (Astronomical Unit) | \$1.5 \times 10^{8}\ \text{km}\$ |
| 1 Light‑Year | \$9.46 \times 10^{12}\ \text{km}\$ (≈ \$63{,}240\$ AU) |
| 1 Parsec | \$3.26\$ light‑years |
Using light‑years allows astronomers to express the vast distances between stars and galaxies in a convenient way.