Glossary of Common Astronomy Terms
Astronomy - The scientific study of objects and events beyond Earth, including stars, planets, galaxies, and the universe.
| Term | Definition | Learn more |
|---|---|---|
| Astronomy | The scientific study of objects and events beyond Earth, including stars, planets, galaxies, and the universe. | In AstroGuide: Learn |
| Astrophotography | The practice of photographing objects in space. It uses cameras, telescopes, and image processing to reveal details that are too faint for our eyes to see. | |
| Aperture | The diameter of a telescope's main lens or mirror. A larger aperture collects more light and can potentially reveal more detail. | |
| Bortle Scale | A nine-level scale used to describe the brightness of the night sky caused by light pollution. Lower numbers represent darker skies. | |
| Celestial Object | Any natural object found in space, such as stars, planets, moons, asteroids, nebulae, and galaxies. | |
| Deep-Sky Object (DSO) | Objects outside our solar system, such as nebulae, star clusters, and galaxies. | |
| Exposure | The amount of time a camera collects light. Longer exposures allow more faint details to be recorded. | |
| Field of View (FOV) | The amount of sky visible through a telescope or camera system. A wider field of view captures larger areas of the sky. | |
| Focal Length | The distance between a telescope's optical system and the point where light is focused. It determines image scale and field of view. | |
| Focal Ratio | The relationship between a telescope's aperture and focal length, expressed as an f-number (such as f/4 or f/10). It affects light-gathering speed and imaging characteristics. | |
| Galaxy | A massive collection of stars, gas, dust, and dark matter held together by gravity. Our home galaxy is the Milky Way. | |
| Light Pollution | Artificial light that brightens the night sky and reduces the visibility of faint astronomical objects. | |
| Light-Year | The distance light travels in one year. It is used to describe distances between stars and galaxies. | In AstroGuide: Learn |
| Magnification | How much larger an object appears through a telescope compared to viewing it with the naked eye. | |
| Nebula | A large cloud of gas and dust in space. Some nebulae are regions where new stars are forming. | In AstroGuide: Learn |
| Narrowband Filter | A filter that allows only specific wavelengths of light to pass through. It is commonly used to capture emission nebulae. | In AstroGuide: Learn |
| Pixel Scale | The amount of sky covered by each pixel of a camera image. It affects the level of detail that can be recorded. | |
| Seeing | The stability of Earth's atmosphere. Good seeing allows sharper views, especially for planets and high-resolution imaging. | In AstroGuide: Learn |
| Signal-to-Noise Ratio (SNR) | The amount of useful information compared to unwanted noise in an image. Higher SNR usually results in cleaner and more detailed images. | |
| Stacking | Combining multiple images together to improve signal quality and reduce noise. | In AstroGuide: Learn |
| Star Cluster | A group of stars held together by gravity. The two main types are open clusters and globular clusters. | |
| Telescope | An optical instrument that collects and focuses light to observe distant objects. | |
| Transparency | The clarity of the atmosphere and how easily light from space can pass through it. | |
| Tracking | The movement of a telescope mount to follow objects as Earth rotates, keeping them centred during observation or photography. | In AstroGuide: Learn |