Post Archives: Watchers of the Skies

For live links, click to: riverhouses.org/2019-alpheratz

October is the middle month of Cygnus Term in the River Houses, and as our monthly star calendar will show you, October’s Great Star is blue-white Alpheratz, the brightest star in the constellation Andromeda, the chained maiden of Greek mythology who was rescued by the hero Perseus. Its formal designation is α Andromedae — “alpha of Andromeda.” Andromeda and Alpheratz are high in the east at sunset now, passing directly overhead around midnight and then off to the west as the night goes on.

Although Alpheratz is officially part of Andromeda, it lies on the border of the adjacent constellation Pegasus and can be most easily recognized as the top left star (when you’re facing south) of the asterism called the Great Square of Pegasus. Its name derives from an Arabic phrase meaning “the navel of the horse,” reflecting its position in adjacent Pegasus.

If you want to introduce your students to Alpheratz and Andromeda, you can start with some basic astronomical mythology from your backyard star guide (riverhouses.org/books):

“In ancient Greek myth, Princess Andromeda of Ethiopia was chained to a rock as a sacrifice to the gods. In the sky, Andromeda is a faint V-shaped constellation that is most often seen upside down. To locate her on fall evenings, trace a line northeast from [the 2.1-magnitude star Alpheratz,] the northeast corner of the Great Square of Pegasus….

“Andromeda’s mother, Cassiopeia, claimed that her daughter’s beauty surpassed that of the daughters of Nereus, a god of the sea and father-in-law of Poseidon. Angered by her boasting, Poseidon sent the monster Cetus to destroy the kingdom of Ethiopia unless Cassiopeia and her husband Cepheus sacrificed their daughter. The princess was rescued by Perseus, who used the head of Medusa to turn Cetus to stone. The whole cast of the tale — her father Cepheus, Cassiopeia, Cetus, Perseus, and the hero’s winged horse Pegasus — are all nearby in the sky.“ (Backyard Guide to the Night Sky, pages 248–249)

That’s plenty for beginning students — your little lesson is done. If you want to get more advanced, the Wikipedia page on Alpheratz is packed with additional information on everything from astrometry to cultural history.

The blue-white star we see as Alpheratz is actually a close double star — two suns orbiting each other — but they are so close that they cannot be resolved even with a sizeable telescope. The double nature of Alpheratz was first detected by close examination of the way the star’s light spectrum changes from week to week. These spectroscopic measurements suggest the two Alpheratz companions circle each other once every 97 days. (Compare this to the earth’s orbit around the sun, which takes 365 days.)

The Alpheratz system is fairly close to us in astronomical terms: a little less than 100 light years away. (The light you see from it tonight was emitted in the early twentieth century and has been traveling toward us for nearly a hundred years until the moment it strikes your eye.) The larger of the two Alpheratz companion stars is almost three times the diameter of the sun, and it’s quite young: only about 60 million years old, in contrast to more than 4.5 billion for our old yellow sun.

Sometime this month, take your homeschool students out at dusk and introduce them to this great nearby star, and teach them its name, and so give them a new friend for life.

What stellar observations have you made in your homeschool lately? 😊

❡ 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 Latin name of the constellation in its 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 speaking, its apparent magnitude. The scale of star magnitudes was developed centuries ago, 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 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 (riverhouses.org/books) 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. 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 monthly “Great Star” 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 (riverhouses.org/calendars) 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. 🌟

For live links, click to: riverhouses.org/2019-deneb

(This is the first of our monthly “Star Bright” posts for the 2019–2020 homeschool year. Print your own River Houses Star Calendar and follow along with us, and add your name to our free weekly mailing list to get great homeschool teaching ideas delivered right to your mailbox all through the year.)

September is the first month of Cygnus Term in the River Houses, and as our monthly star calendar will show you, September’s Great Star is Deneb, the brightest star in the constellation Cygnus the Swan. Its formal designation is α Cygni — “alpha of Cygnus.” Cygnus and Deneb are high in the east at dusk now, passing overhead in the early evening and flying to the west as the night goes on.

If you want to introduce your students to Deneb and Cygnus, you can start with some basic astronomy from your backyard star guide (riverhouses.org/books):

“Cygnus lies in what for observers is a dense and fascinating part of the sky. The bird’s wings span the Milky Way at a location packed with stars and an assortment of deep-sky objects. Owing to the positions of its bright stars it is sometimes called the Northern Cross — the northern parallel to the brilliant Southern Cross constellation in the Southern Hemisphere. You will see Cygnus highest in the sky in late summer and early fall, with its head pointing south like a bird on its migratory path toward warmer climates.

“Deneb, the alpha star and tail of the bird, is a brilliant magnitude-1 star that joins Altair and Vega to form the Summer Triangle. Deneb is 25 times more massive than our sun and 60,000 times more luminous.“ (Backyard Guide to the Night Sky, page 216)

That’s plenty for beginning students — your little lesson is done. If you want to get more advanced, the Wikipedia page on Deneb is packed with additional information on everything from astrometry to cultural history.

Deneb is an enormous blue-white supergiant, about 200 times the diameter of our sun. If it were placed at the center of our solar system it would extend out to engulf the orbits of Mercury, Venus, and the Earth. Deneb is estimated to be about 2,600 light years away, so the photons striking your eye when you gaze upon it were actually emitted by the star 2,600 years ago — when the ancient Greek poet Sappho was composing her lyrics in the eastern Aegean — and they have been traveling at the speed of light to greet us ever since. The name Deneb is Arabic for tail — it’s the tail of the swan for us, but for medieval Arabic astronomers it was usually imagined as the tail of a heavenly hen.

Some time during this first month of Cygnus Term, take your homeschool students out at dusk and introduce them to this giant sun, and teach them its name, and so give them a new friend for life.

What stellar observations have you made in your homeschool lately? 😊

❡ 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 Latin name of the constellation in its 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 speaking, its apparent magnitude. The scale of star magnitudes was developed centuries ago, 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, 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 has imaged distant stars and galaxies below magnitude 30, the dimmest celestial objects humans have seen so far. 🔭

❡ 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 (riverhouses.org/books) 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. 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 monthly “Great Star” 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 (riverhouses.org/calendars) 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. 🌟

For live links, click to: riverhouses.org/2019-vega

August is the last 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 from your homeschool star atlas (riverhouses.org/books):

“Lyra is easily identified because of Vega, a brilliant white star of magnitude 0.0, the fourth brightest star in the sky and the second brightest visible from northern latitudes. Four smaller stars lie in a faint but conspicuous parallelogram just to the southeast of Vega. Although a small constellation, Lyra is rich in stars; sweep slowly with binoculars, particularly the area between β [beta] and γ [gamma] Lyrae. Do not fail to observe β [beta] Lyrae, an eclipsing binary whose light changes are visible to the naked eye, the magnitude varying from 3.4 to 4.3. ε [epsilon] Lyrae is the famous “double double”; persons with very keen eyesight can see the two components. They are easily split with binoculars. In a telescope, each of the components itself becomes a double.“ (Celestron Sky Maps, page 12)

The planisphere on the front of your star atlas will help you locate Vega, and 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.

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 times the diameter of the sun, but it is rotating so rapidly that it bulges out at the equator, making it more egg-shaped than spherical. It’s also quite a bit younger than the sun, with an estimated age of only 455 million years (compared to the sun’s age of more than 4.5 billion).

This month, take your homeschool students out at dusk and introduce them to this great nearby sun, and teach them its name, and so give them a new friend for life.

What stellar observations have you made in your homeschool lately? 😊

❡ 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 Latin name of the constellation in its 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 be the top star 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 speaking, its apparent magnitude. The scale of star magnitudes was developed centuries ago, 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, 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 has imaged distant stars and galaxies below magnitude 30, the dimmest celestial objects humans have seen so far. 🔭

❡ Watchers of the skies: Teaching your students to recognize the constellations is one of the simplest and most enduring gifts you can give them. The planisphere on the front of your River Houses star atlas (riverhouses.org/books) will let you dial up the northern hemisphere sky for any night of the year, and the descriptions and maps of each constellation will point out the highlights, including the names and characteristics of the brightest stars. Your general world atlas also has beautiful maps of the whole northern and southern hemisphere night skies on plates 121–122. 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 monthly “Great Star” 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 (riverhouses.org/calendars) 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. 🌟