Kitt Peak Nightly Observing Program
Splendors of the Universe on YOUR Night!
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Andromeda was the princess of myth who was sacrificed by her parents to the sea monster Cetus. Fortunately, the hero Perseus came along to save her, and they were eventually married. The constellation Andromeda is host to the Andromeda Galaxy. Although there are smaller, dwarf galaxies that are closer to our galaxy, Andromeda is the closest big galaxy like our own; in fact, it’s bigger.
Aries is a medium-brightness constellation, but with few stars and an indistinctive shape, which makes it more challenging to recognize.
Cassiopeia is widely recognized by its characteristic W shape, though it may look like an M, a 3, or a Σ depending on its orientation in the sky, and your position on Earth. However it’s oriented, once you’ve come to know its distinctive zig-zag pattern, you’ll spot it with ease. The plane of the Milky Way runs right through Cassiopeia, so it’s full of deep sky objects—in particular, a lot of open star clusters. Cassiopeia is named for the queen form Greek mythology who angered the sea god Poseidon when she boasted that her daughter Andromeda was more beautiful than his sea nymphs.
Cygnus is a large constellation, prominent in the Northern Hemisphere. Its name comes from the Greek for “Swan” and can be imagined as a giant, celestial swan, flying overhead, with its wings fully extended. The brightest star in Cygnus is Deneb, which is one of the brightest stars in the sky, and a whopping 800 lightyears away! Deneb is one point of an asterism called the Summer Triangle—three very bright stars that form a large triangle shape prominent in the Northern hemisphere summer skies.
Lyra is a small, but notable constellation. It is host to Vega—the fifth brightest star in the sky (or sixth, counting the Sun). Not far from Vega is Messier object 57—the Ring Nebula, which is perhaps the best known planetary nebula in our sky. Lyra’s name is Greek for lyre—a kind of harp.
This constellation is named for one of the most beloved creatures of Greek mythology—the winged horse named Pegasus. Within Pegasus is a well known asterism containing the 3 brightest stars in the constellation (+ 1 in Andromeda) called The Great Square of Pegasus. Alpheratz, the brightest star in the square, actually belongs to the constellation Andromeda, but in the past, this star had been considered to belong to both constellations.
NGC 253 Sculptor Galaxy
Ngc 253: The “Silver Dollar Galaxy”. A lumpy, dusty, nearly-edge-on spiral galaxy just a bit smaller than the Milky Way. At least 75 billion solar masses, eleven million lightyears from here. It was discovered by Caroline Hershel in 1783.
M15 is a distant globular cluster, 33,000 light-years away. It has 100,000 stars, and is one of the oldest known globular clusters, having formed about 12 billion years ago.
M2 is a globular star cluster containing roughly 150,000 stars, and is located about 35,000 light-years away. It has a diameter of 170 light-years, making it one of the largest known clusters by volume.
Quick streaks of light in the sky called meteors, shooting stars, or falling stars are not stars at all: they are small bits of rock or iron that heat up, glow, and vaporize upon entering the Earth’s atmosphere. When the Earth encounters a clump of many of these particles, we see a meteor shower lasting hours or days.
That clumpy band of light is evidence that we live in a disk-shaped galaxy. Its pale glow is light from about 200 billion suns!
Human technology! There are almost 500 of these in Low Earth Orbit (we can’t see the higher ones). We see these little “moving stars” because they reflect sunlight.
M103 is one of many open star clusters in the constellation Cassiopeia. At a distance of about 10,000 lightyears, this is one of the most distant open star clusters known. The apparent brightest star in the cluster is not actually a member of the cluster at all, but actually a foreground star. The brightest star in the cluster is a red giant star; it has a redish orange tinge.
M45 The Pleiades
M45, the “Pleiades,” is a bright, nearby star cluster, in the last stages of star formation. About seven stars stand out as the brightest in the cluster, and is why the cluster is also known as the “Seven Sisters,” alluding to the Pleiades, or Seven Sisters from Greek mythology. In Japanese, the cluster is known as “スバル,” “Subaru,” and is featured as the logo of the automobile manufacturer of the same name. The Pleiades lies about 440 light-years away and is a very young (for an open star cluster) 100 million years old.
Messier 52 is an open star cluster, which was discovered in 1774 by Charles Messier. The density near the center is about 3 stars per cubic parsec. The cluster is only 35 million years old—very young for stars. The distance of this cluster from our Solar System is not very well known; estimates range between 3,000 and 7,000 light-years. M52 can be seen as a nebulous patch in a good pair of binoculars or a small telescope. In larger telescopes, it appears as a fine, rich, compressed cluster of faint stars, often described as of fan or “V” shape. M52 can be found by extending the line from Alpha over Beta Cassiopeiae by 6 1/2 degrees to the NW to 5th mag 4 Cassiopeiae; M52 is roughly 1 degree south and slightly west of this star.
M27 Dumbbell Nebula
M27: The “Dumbbell Nebula” is the ghost of a star; the ejected outer shell of gas is of gas is still illuminated by the star’s white-hot core. Hershel named this type this type of object a “planetary” nebula, just because it looks round.
M57 Ring Nebula
M57: The Ring Nebula. This remnant of a dead star looks exactly as it’s name says – a ring or doughnut shape cloud of gas. The nebula is about 2.6 lightyears across and lies about 2,300 lightyears away.
Albireo (β Cyg)
Named long before anyone knew it was more than one star, Albireo (β Cygni) comprises of a set of stars marking the beak of Cygnus, the swan. Through a telescope, we see two components shining in pale, but noticeably contrasting colors: orange and blue. The difference in color is due to the stars’ difference in temperature of over 9000°C! The brighter orange component, Albireo A, is actually a true binary system, though we can’t resolve two stars in the telescope. The fainter blue component, Albireo B, may be only passing by, and not gravitationally interacting with Albireo A at all. Albireo is about 430 light-years away.
Mesarthim (γ Arietis)
Mesarthim is one of the brighter stars making up the constellation Aries—the ram. It is actually a pair of stars—a double star—204 light-years away. It’s component stars are of similar brightness and both white. They are separated by about 500 times the distance between the Earth and the Sun, and take approximately 5,000 years to orbit each other. The apparent (slightly) dimmer star, Gamma-1, is actually the hotter and more luminous star. Much of its light is ultraviolet, and invisible to human eyes. The apparent (slightly) brighter star, Gamma-2, has some interesting characteristics that suggest not only that it may be evolving from a dwarf to a subgiant, but also that it is highly magnetized.
Struve 2470 and 2474 The Other Double Double
Struve 2470 and 2474 are a lesser known pair of double stars in the constellation Lyra. The system’s neighbor, Epsilon Lyrae, the “Double Double” is the better know pair of double stars.
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