Astronomy

Eclipses and shooting stars: August’s celestial spectacle

The Perseids are this month’s highlight: tiny fragments of a comet which become visible as they pass through the Earth’s atmosphere

Le Perseidi sembrano apparire tutte dallo stesso punto

3' min read

Translated by AI
Versione italiana

3' min read

Translated by AI
Versione italiana

This August promises to be a month full of spectacular celestial events: on the 12th, there will be an eclipse which, in northern Italia, will appear almost total at sunset, followed by plenty of shooting stars. This year, there is a good chance of seeing them clearly, particularly as the Moon will cause very little interference in the sky on the most favourable nights. The most famous are the Perseids, the ‘tears of St Lawrence’, which appear to come from the constellation Perseus and become more frequent as we approach the middle of the month.

You don’t need any special equipment to see them. Simply move as far away as possible from the brightest lights and choose a spot with an unobstructed view of the horizon: a beach, the mountains, the countryside – or even an urban area that isn’t too brightly lit will do.

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Tradition has it that you should make a wish when you see your first shooting star. But, beyond this charming old saying, it’s worth pausing to watch them, because behind that trail of light lies a story that is far longer and more fascinating than we realise.

What we call shooting stars are not stars like our Sun, which is thousands and thousands of kilometres across. They are tiny fragments of matter, specks of cosmic dust, which enter the Earth’s atmosphere at extremely high speeds and, as they pass through it, heat up to produce the luminous trail that we can see with the naked eye.

In most cases, these are tiny particles, sometimes no bigger than a grain of sand or just a little larger. Yet their appearance in the night sky is spectacular, because friction with the upper layers of the atmosphere and the intense heating of the surrounding air transform that almost invisible fragment into a fleeting trail of light.

Origins in a comet

The story of that particle, however, began a long way away. In the case of the Perseids, the fragments originate from Comet 109P/Swift-Tuttle, an icy body that orbits the Sun with a period of approximately 133 years and which, as it passes through the inner regions of the Solar System, leaves behind gas and dust along its path.

Comets are objects composed of ice, dust and rocky material. As they approach the Sun, they heat up and release material from their surface: it is this material that forms the comet’s coma and tail, making the comet visible and scattering a large quantity of tiny debris along its orbit.

In August, the Earth passes through one of these regions rich in particles left behind by Swift-Tuttle. In a sense, the phenomenon is similar to driving into a bank of fog: our planet moves through space, passing through that diffuse cloud of fragments, and some of them enter the atmosphere, lighting up the sky with the Perseid meteor shower.

The colour of the trail can also provide some indication of the material’s composition and the physical conditions of the phenomenon. The shades observed depend on both the elements present in the meteoroid and the atmospheric gases involved in the heating process; for this reason, the hues can vary from yellow to green, and from red to blue.

Una stella cadente sta entrando in atmosfera, vista dallo spazio

The issue, however, is not limited to August nights. The Earth is constantly receiving dust from interplanetary space: an amount which, on an annual basis, is estimated at thousands of tonnes, albeit in the form of tiny particles that are almost always invisible in everyday life.

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To give an idea of the scale, this material is very abundant overall, but broken down into tiny particles. Some of this dust settles everywhere, mixing with terrestrial dust; in some cases, with simple tools and a great deal of patience, one can even observe traces of it amongst the debris collected from an exposed surface.

The effect on the Moon

Cosmic dust is also significant on the Moon. There is no atmosphere there capable of slowing down micrometeorites, and so even the smallest fragments reach the surface directly, stirring up other material and contributing, over time, to the formation of that fine, crumbly surface layer we call regolith.

Furthermore, on the Moon, there is no wind, rain or vegetation capable of quickly erasing the tracks left on the surface. This is one of the reasons why the footprints of the Apollo astronauts, left in the lunar dust decades ago, are still there.

In short, a speck of dust can conceal a part of the history of the Solar System. And perhaps this is precisely what makes a shooting star so fascinating: the fact that, for a moment, something tiny and ancient streaks across our sky and reminds us just how far back in time and space a journey that seems so brief might have begun.

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