The aurora borealis is often seen solely method up north, however two weeks in the past the evening sky was full of shimmering curtains of pink and inexperienced mild that could possibly be seen all the way in which down into the southern US. Folks in Texas and Hawaii received out of their automobiles to stare and take footage.
The reason for this mild present was an particularly strong blast of solar wind—electrically charged particles shot out from the solar at unbelievable speeds. And there is extra to return as we strategy the height of the present photo voltaic cycle, a interval of elevated photo voltaic storms that occurs each 11 years.
That is one instance of what scientists name “space weather,” which offers with the interplay between the solar and the Earth. Not all the results of house climate are fairly, and a few are outright harmful. However the physics behind it are fairly cool. Let’s test it out!
Blowin’ within the Wind
You would possibly consider the solar as an amazing ball of fireplace—nevertheless it’s not. (Fireplace is a chemical response between oxygen and carbon.) What the solar is, actually, is a huge nuclear fusion reactor. Within the core, protons are smashed collectively below excessive strain. These protons stick collectively to create the nucleus of a helium atom, with two protons and two neutrons. (Two of the protons decay into neutrons).
Illustration: Rhett Allain
However wait! The helium nucleus has much less mass than the 4 protons we began with. That mass is not misplaced—it is became vitality, in accordance with Einstein’s well-known equation E = mc2, the place E is vitality, m is mass, and c is the pace of sunshine. That final quantity is large—mild travels at 300,000 kilometers per second, and it is hugeness is squared—which implies that even a tiny lack of mass creates A LOT of vitality. That is why the solar is so scorching, with a core temperature of 27 million levels Fahrenheit. Yep, that is fairly scorching.
Below this excessive warmth, the gases within the outer a part of the solar type a plasma by which electrons are ripped away from their atoms, leaving free electrical costs (principally electrons and protons) zooming round. A few of them are shifting quick sufficient to flee the gravitational pull of the solar. These ejected particles are what we name the “photo voltaic wind.”
You’ll be able to see the impact of the photo voltaic wind when it hits a comet. Comets are mainly massive soiled snowballs that orbit the solar in lengthy ellipses. As one nears the solar, its icy physique sublimates and turns right into a gasoline. A few of this gasoline good points sufficient vitality to be ionized (electrons are free of the atoms), leaving an electrically charged gasoline. Then, when the photo voltaic wind hits, it pushes this ionized gasoline away, making a tail that may be tens of thousands and thousands of miles lengthy.
Enjoyable truth: You would possibly suppose the tail extends out behind the comet like a jet contrail, nevertheless it does not! It extends away from the solar—so mainly sideways to the path of the comet’s movement.
Why Now?
However what causes the photo voltaic wind to get so labored up each 11 years? Properly, like Earth, the solar has a magnetic discipline, nevertheless it’s extraordinarily unstable. As a result of the solar isn’t a stable object, completely different elements of it rotate at completely different speeds. This causes its magnetic discipline to twist and warp, and each 11 years or so it really flips and reverses polarity. This final occurred in 2013, and right here we’re in 2024.
These shifting magnetic discipline strains can break by way of the floor, creating solar spots and superior geysers of plasma referred to as photo voltaic flares. Why does this occur? When electrical costs are zipping round, they are often pushed and pulled by a magnetic discipline. You’ll be able to see this your self with some copper wire and a battery. Should you place the wire close to a stationary magnet after which join the ends so a present flows, the wire will transfer. Test it out:
