Spiraling Stars Help Explain Early Universe

Spiraling stars in the Small Magellanic Cloud are the subject of a recent study in ‘The Astrophysical Journal.’ Find out how their spiral motions help explain the “baby boom” of star formation shortly after the Big Bang.

At this time of the year, I enjoy looking up at the sky toward the constellations Andromeda and Cassiopeia. It’s the ideal time for me to try to spot the Andromeda Galaxy, also known as M31.

It’s the brightest galaxy we can see with the naked eye, and it’s also the closest full galaxy to the Milky Way. Since I live in the Northern Hemisphere, I’ve never had the chance to look at a couple of other easily visible neighbouring galaxies called the Large and Small Magellanic Clouds.

Astronomers classify the Magellanic Clouds as irregular dwarf galaxies, and they’re only visible south of Earth’s equator. Both Magellanic Clouds orbit our Milky Way galaxy as part of the same local group of galaxies that includes Andromeda.

Spiraling Stars in the Small Magellanic Cloud

Fortunately, the Hubble Space Telescope and the European Southern Observatory’s Very Large Telescope don’t have my…