August is the third month of Hercules Term in the River Houses, and as our monthly star calendar will tell you, August’s Great Star is Vega, the brightest star in the constellation Lyra the Lyre. Its formal designation is α Lyrae — “alpha of Lyra.” Vega is one of my favorites and it’s almost directly overhead (near the zenith) every evening this month just after sunset, passing off to the west as the night goes on.
If you want to introduce your students to Vega and Lyra you can start with some basic astronomy and astronomical mythology from your backyard star guide:
Resembling a small jagged line hitched to a parallelogram, Lyra is one of the delights that is easy to envision and easy to spot. Its alpha star, Vega, is among the brightest stars in the sky and is directly overhead from mid-northern latitudes in summer — a handy reference point for many other constellations and objects. With Deneb [our September star] and Altair [alpha Aquilae], Vega forms the Summer Triangle.
Three times the size of our sun and 50 times more luminous, astronomers think Vega may be young and newly formed, only about 400 million years old — that’s less than 10 percent of our sun’s age. A big Vegan discovery came in 1983, when the Infra-Red Astronomical Satellite (IRAS) photographed a disk of cool dust surrounding the star. Astronomers suspect that planets may be forming out of this swirling material around Vega, creating the birth of an alien solar system in the same way that ours formed.
A chilling love story accompanies this constellation. Apollo gave his son Orpheus the lyre and taught him to play captivating music. Despite being the object of many women’s affections, Orpheus loved his wife Eurydice. She died and was sent to the underworld, but Orpheus was unyielding in his desire to bring her back to life. The gods decided to allow it, but Orpheus failed to follow their one admonition not to turn around and look back at his wife as they exited Hades. Having lost his love again, Orpheus refused all other advances and was killed by a discouraged group of young women. He was then reunited with his wife, and as a tribute to their love, Zeus sent the lyre up into the sky. (Backyard Guide to the Night Sky, page 218)
That’s plenty for beginning students — your little lesson is done. If you want to get more advanced, the Wikipedia page on Vega is packed with additional information on everything from astrometry to cultural history.
Because of its prominence in the northern hemisphere night sky, Vega has played an important role in the development of modern astronomy. It was the first star other than the sun to be photographed (by daguerreotype in 1850), and the first star other than the sun to have its spectrum analyzed (in the 1870s). When the scale of stellar magnitudes was refined during the nineteenth century, Vega was chosen as the principal reference star with a defined magnitude of 0.0. (See our note below on star magnitudes.)
Modern calculations put Vega at a distance of about 25 light-years — practically next door in astronomical terms. It’s estimated to be about two and a half to three times the diameter of the sun, but it is rotating so rapidly that it bulges out at the equator, making it more ellipsoid than spherical like our sun.
Sometime this month, take your homeschool students out after dark and introduce them to this brilliant nearby sun, and teach them its name, and so give them a new friend for life.
What astronomical observations and stellar sightings have you made in your homeschool this Hercules Term? 😊
❡ Alpha and beta and gamma, oh my: Most of the principal stars within each constellation have both old vernacular names — Vega, Sirius, Arcturus, and so on — as well as more formal scientific designations. The German astronomer Johann Bayer (1572–1625) devised the formal system of star designations that is still in common use today. In Bayer’s system, the stars in each constellation, from brightest to dimmest, are assigned a lowercase letter of the Greek alphabet: α (alpha, brightest), β (beta, second brightest), γ (gamma, third brightest), δ (delta, fourth brightest), and so on. This letter designation is combined with the name of the constellation in its Latin possessive (genitive) form: Lyra becomes Lyrae (“of Lyra”), Canis Major becomes Canis Majoris (“of Canis Major”), and so on. The brightest star in the constellation Lyra (the star Vega) thus becomes α Lyrae (“alpha of Lyra”), the brightest star in Canis Major (the star Sirius) becomes α Canis Majoris (“alpha of Canis Major”), and so on, through all 24 Greek letters and all 88 constellations. How bright would you expect, say, the σ (sigma) star of Orion to be? Not very bright — it’s far down the alphabet — but σ Orionis happens to mark the top of Orion’s sword, so even though it’s not very bright it’s still notable and easy to locate on a dark night. ✨
❡ Star bright: The brightness of a star as we see it in our night sky is its magnitude — or more properly, its apparent magnitude. The scale of star magnitudes was developed long before modern measuring instruments were invented, so it can be a little bit confusing for beginners. Originally, the brightest stars in the sky were called “first magnitude” and the less-bright stars “second magnitude,” “third magnitude,” and so on, down to the dimmest stars visible to the naked eye, which were called “sixth magnitude.” In the nineteenth century the star Vega (our August star) was chosen as the standard brightness reference and its value on the magnitude scale was defined to be zero (0.0). Five steps in magnitude (from 0.0 to 5.0 or from 1.0 to 6.0) was defined to be a change in brightness of 100 times: a star 100 times dimmer than Vega (0.0) was defined to be a magnitude 5.0 star. Vega is not quite the brightest star is the sky, however, so the scale also had to be extended into negative numbers: Sirius (our March star), for example, is magnitude –1.5, about three times brighter than Vega (at 0.0). The planet Venus at its brightest is about magnitude –4.2; the full moon is about magnitude –12.9; the sun is magnitude –26.7. By contrast, the dimmest stars visible to the naked eye in a populated, light-polluted area are about magnitude 3.0; the dimmest stars visible under very dark conditions are about magnitude 6.5. The Hubble Space Telescope in orbit around the earth has photographed distant stars and galaxies below magnitude 30, the dimmest celestial objects humans have seen so far. 🌃
❡ And all dishevelled wandering stars: How far away are the stars? Do they all occupy a single celestial “dome” that rotates through the heavens (as some ancient and medieval astronomers believed), or are they scattered through space at different individual distances? Astronomers had long suspected that the “fixed” stars existed at different distances from us, but early attempts to measure those distances failed. It was not until the early 1800s that instruments and measuring techniques became precise enough to allow the first stellar distances to be calculated using the technique of parallax. Parallax is the displacement in the apparent position of an object with respect to the background when an observer moves from side to side. It’s an ordinary phenomenon you experience every day — it’s how we judge distances as we move through the landscape. Stellar parallaxes are extremely small — fractions of an arc-second (one 3600th of a degree) — and they are calculated by measuring a star’s position against the background at opposite sides of the earth’s orbit, six months apart. (That’s the astronomical equivalent of taking one step to the side.) Vega, our August star, was one of the first stars to have its parallax measured; modern estimates put it at about 0.13 arc-seconds. Apply some trigonometry, and that yields a distance of about 25 light-years. 🔭
❡ Watchers of the skies: Teaching your students to recognize the constellations is one of the simplest and most enduring gifts you can give them. We recommend the handy Backyard Guide to the Night Sky as a general family reference — it will help you identify all the northern hemisphere constellations and will point out many highlights, including the names and characteristics of the brightest stars. Your recommended world atlas also has beautiful maps of the whole northern and southern hemisphere night skies on plates 121–122 (10th and 11th eds.). Why not find a dark-sky spot near you this month and spend some quality homeschool time beneath the starry vault. 🌌
❡ First star I see tonight: This is one of our regular Homeschool Astronomy posts featuring twelve of the most notable stars of the northern hemisphere night sky. Download and print your own copy of our River Houses Star Calendar and follow along with us as we visit a different Great Star each month — and make each one of them a homeschool friend for life. 🌟
❡ This is a printable lesson: Down at the bottom of this post you’ll find a “Print” button and icon, along with several social-media share buttons. The Print button will let you create a neat and easy-to-read copy of this little lesson, and it will even let you resize or delete elements that you may not want or need (such as images or footnotes). Give it a try today! 🖨
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