As of the first of May 2024 - the LVST is back on line.
A meteor is the bright trail of a meteoroid, or piece of space debris, that we might see as it enters our atmosphere and becomes a line of luminous plasma. An estimated 25 million meteoroids, micro meteoroids and other space debris enter Earth's atmosphere each day, which results in an estimated 15,000 tonnes of that material each year. Most of the meteors visible to the naked eye are no more than particles of dust.
Sometimes if a meteoroid has sufficient mass, it makes it to the Earth's surface and is classified as a 'meteorite', The picture above is of an example meteorite held at the Visitors Centre in the Jodrell Plank Observatory's collection. It is a small part of a larger meteorite that fell to earth in the Sikhote-Alin Mountains (Russia) in 1947 and is an 'iron-nickel meteorite' (part of an asteroid's core)
Micro-meteorite dust falls on the surface of the Earth at a rate of 6,000 kg per day. This sounds a lot but if you average this across the surface area of our planet it works out at only one particle per square metre per year. To maximise finding one of these micrometeorites increasing the collection area works. One place to look in urban areas is in the rain water gutters of large roofs.