Sometimes I complain about the earthly weather, but mostly I like to post about astronomy and space events. Hope you enjoy the articles.
By: Susie77 , 5:02 PM GMT on January 17, 2014
Courtesy of EarthSky
As seen during Northern Hemisphere winter (or Southern Hemisphere summer), the stars seem brighter. Why? It’s partly because – on December, January and February evenings – the part of Earth you’re standing on is facing into the spiral arm of the galaxy to which our sun belongs.
Consider the sky at the opposite time of year. In June, July and August, the evening sky seen from the entire Earth is facing toward the center of the Milky Way galaxy. The galaxy is about 100,000 light-years across, and its center is some 25,000 to 28,000 light-years away. We don’t see into the exact center of the Milky Way, because it’s obscured by galactic dust. But during those Northern Hemisphere summer months (Southern Hemisphere winter months), as we peer edgewise into the galaxy’s disk, we’re gazing across some 75,000 light-years of star-packed space (the distance between us and the center, plus the distance beyond the center to the other side of the galaxy). Thus, at that time of year, we’re looking toward the combined light of billions upon billions of stars.
On June, July and August evenings, we look toward the galaxy’s center as indicated by the red arrows. On December, January and February evenings, we look away from the center, as indicated by the blue arrows. Other features, including our galaxy’s primary spiral arms and the sun’s location in the Orion Spur, are also shown. Artist’s illustration via NASA/JPL/Caltech/R.Hurt. View larger.
In northern winter, we’re looking the opposite way – into the suburbs of the galaxy and into the spiral arm of the galaxy in which our sun resides. There really are some gigantic stars located in this direction, and they are relatively close to us – in our own neighborhood, so to speak, our own spiral arm. So we’re seeing fewer stars on Northern Hemisphere winter evenings (or Southern Hemisphere summer evenings), as we look across only about 25,000 light-years of Milky Way, toward the deep space beyond our galaxy’s boundaries.
And that’s why, while the combined light of so many distant stars visible on June, July and August evenings gives the sky a hazy quality, the evening sky in December, January and February looks clearer and sharper.
Our spiral arm of the galaxy is called the Orion Arm, or sometimes the Orion Spur. It’s not one of the primary spiral arms of the Milky Way but only a “minor” spiral arm. Our local Orion Arm is some 3,500 light years across. It’s approximately 10,000 light years in length. Our sun, the Earth, and all the other planets in our solar system reside within this Orion Arm. We’re located close to the inner rim of of this spiral arm, about halfway along its length.
Perhaps you know the bright stars of the prominent constellation Orion the Hunter? This constellation is visible in the evening during Northern Hemisphere winter (Southern Hemisphere summer). The stars of mighty Orion also reside within the Orion Arm of the Milky Way. In fact, our arm of the galaxy is named for this constellation.
Bottom line: During the Northern Hemisphere winter months (Southern Hemisphere summer months), everyone on Earth is looking away from the star-rich center of the galaxy, toward the outskirts of our Milky Way galaxy, during the evening hours. We are looking into the spiral arm of the galaxy to which our sun belongs. That’s why we see so many bright stars; they are neighbors of sorts to our sun in our local spiral arm. And it’s one reason why this part of the sky has a sharp and clear quality; we are seeing fewer stars, surrounded by the inky depths of space beyond our galaxy’s boundaries.
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