Explaining Different Kinds of Meteor Showers. It’s the Way the Comet Crumbles

The Universe often puts on a good show for us down here on Earth but one of the best spectacles must be a meteor shower. We see them when particles, usually the remains of comets, fall through our atmosphere and cause the atmosphere to glow. We see them as a fast moving streak of light but a new paper has suggested that the meteor showers we see can explain the sizes of the particles that originally formed the comet from where they came. 

Comets are mostly composed of ice but with a little rock mixed in for good measure. They’ve often been called dirty snowballs to describe this mix of ice and rock. They travel around the Sun in elongated, elliptical orbits which bring them close to the Sun. The intense heat from the Sun causes the ice to instantly turn into a gas in a process known as sublimation which releases the trapped dust. The pressure from the Sun known as the solar wind presses against the gas and dust released from a comet to produce the tail which always points away from the Sun. 

As the comet travels around the Solar System, it deposits debris along its orbit almost like a trail of celestial breadcrumbs. The debris at this stage is known as meteoroids but, if the Earth travels through it then they create the stunning meteors that we see streak across the sky. The Earth passes through the debris field from a number of comets on a regular, annual basis and this gives rise to the regular meteor showers we see such as he Perseids or Leonids. 

A team of 45 researchers have been studying meteor showers and have discovered something rather curious. They have found that not all comets crumble in the same way as they approach the Sun. The team studied 47 young meteor showers by using special low light video cameras all over the world. The cameras measured the path of the meteors enabling the team to work out how high up they were when they first light up and how they then slowed down in the atmosphere. They were also able to measure the composition enabling them to deduce the size of the particles.

In a paper published in the journal Icarus, the team theorised that a comet will simply crumble into the size of the ‘pebbles’ they are made of. This does seem to make complete sense given that the comets form as chunks of dust, rock and ice. More ice will slowly form as the comet orbits out in the dark cold reaches of the Solar System but as it heats on its journey inwards, it will just fall apart again as the ice sublimates. 

The results of the paper showed that longer period comets, such as those originating in the Oort Cloud generally crumble into sizes of particulates indicative of slow and gentle accretion conditions.  The resultant meteoroids have a lower density and tend to only brighten deeper into the Earth’s atmosphere. Comets from the Jupiter-family on the other hand crumble up into smaller, denser meteoroids with 8% more solid material on average.

There are a few meteor showers that originate from asteroids and these too have been studied. The team found that they tend to produce meteor showers with smaller particles that have evidence of aggressive fragmentation during their formation. The team acknowledge there will be exceptions to their findings but it their study has helped to build a more fuller picture of the early stages of the evolution of the Solar System and to the nature of comets that grant us the beauty of meteor showers.

Source : Meteor showers shed light on where comets formed in the early solar system