Observing the Sun in white light is rewarding and relatively simple to do. It's also inexpensive, especially if you already have a telescope; all you need is a white-light solar filter.
There are many different ways to make a record of white-light solar activity, including simple counts of surface features, full-disc images, generic sunspot classifications and detailed classifications. In this article we'll guide you through solar observation, from the basics to performing detailed, daily sunspot classifications. Your observations will really help solar science, and don't forget that this is a unique opportunity to study a star close up!
First, though, we have to address the issue of solar safety. Concentrating the Sun's energy through a lens or with the concave mirror of a reflecting telescope raises it to potentially dangerous levels, so never look through or point any unfiltered telescope directly at the Sun. This includes small finder telescopes too, as apart from the obvious fire risk, there's a good chance you'll burn out their crosshairs. We'd recommend capping, filtering or removing finderscopes just to be sure.
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Could We Find Aliens by Looking for Their Solar Panels?- Designed to reflect ultraviolet and infrared, the panels have a unique fingerprint
Researchers searching for life beyond Earth spend a lot of time thinking about what telltale signs might be detectable astronomically. Forms of unambiguous evidence for the presence of life on another world are known as biosignatures. By extension, techno signatures are indicators of activity by intelligent, civilisation-building life.
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The Big Bang produced a Universe filled almost exclusively with hydrogen and helium; all other elements - what astronomers call metals - were produced by stars, supernovae and everything that happens later. So if you can pick out a pristine star with no metals polluting it from among the billions in the Milky Way, then you are likely to have a star dating from our Galaxy's earliest days.
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