The Evening Sky in July 2018

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Transcription:

The Evening Sky in July 2018 All five of the naked-eye planets are in the evening sky. Venus, Jupiter and Mars appear soon after sunset. Silver Venus is in the west, above where the sun set. Golden Jupiter is in the northeast at dusk, moving to due north by 8 pm. Orange Mars is in the east. As the sky gets darker Mercury appears below and left of Venus. It sets around 7 pm. Mercury keeps the same distance from Venus till mid-month, then sinks lower. Saturn also appears in the darker sky, midway between Jupiter and Mars. It is in the middle of the Milky Way and is the brightest 'star' in that part of the sky. Sirius, the brightest true star, sets in the southwest as twilight ends, twinkling like a diamond. Canopus, the second brightest star, is also in the southwest at dusk. It swings south later. South of the zenith are 'The Pointers', Beta and Alpha Centauri. They point to Crux the Southern Cross on their right. Midway down the north sky is orange Arcturus, similar in brightness to Saturn. Vega rises in the northeast around 9 pm. It is on the opposite side of the sky to Canopus: low in the north when Canopus is low in the south. Venus sets more than three hours after the sun so is a brilliant object in the dark night sky. It is bright enough to cast shadows in dark locations. In a telescope it is small and featureless, looking like the Moon after first quarter. It is 140 million km away mid-month. Mercury is tiny in a telescope. Through the month it becomes a thinner but taller crescent as it comes closer but more of its sunny side is turned away from us. Mercury is 150 million km from us at the beginning of July and 95 million km at the end. The crescent Moon will be right of Mercury on the 15th and near Venus on the 16th. We pass by Mars at the end of July. It will then be 58 million km away, the closest it has been since 2003. It is still small in a telescope. At a magnification of 75x it appears as large as the Moon does to the naked eye. Its south polar cap of ice and frozen carbon dioxide might be seen as a white spot. Dusky markings are sometimes visible, crossing slowly as the planet rotates. Jupiter and Saturn are always worth a look in any telescope. Jupiter's four 'Galilean' moons can be seen lined up on each side of the planet. Sometimes one or two may be missing as they pass in front of or behind Jupiter or are hidden in Jupiter's shadow. A small telescope shows Saturn's ring system and biggest moon Titan looking like a star about four ring-diameters from the planet. Big telescopes show fainter moons closer in. Jupiter is 740 million km away mid-month; Saturn is 1360 million km away. The Moon will be near Jupiter on the 21st and close to Saturn on the 25th..Alpha Centauri is the third brightest star. It is also the closest of the naked eye stars, 4.3 light years* away. Beta Centauri, like most of the stars in Crux, is a blue-giant star hundreds of light years away. Canopus swings down to the southern skyline before midnight then moves into the southeast sky in the morning hours. It is a 'circumpolar star': it never sets. Crux and the Pointers are also circumpolar. Canopus is a truly bright star: 13 000 times the sun's brightness and 300 light years away. Arcturus, in the north, is the fourth brightest star and the brightest in the northern hemisphere sky. It is 120 times the sun's brightness and 37 light years away. It twinkles red and green when setting in the northwest around midnight. It is an orange colour because it is cooler than the sun; around 4000 C. The Milky Way is brightest and broadest in the east toward Scorpius and Sagittarius. In a dark sky it can be traced up past the Pointers and Crux, fading toward Sirius. The Milky Way is our edgewise view of the galaxy, the pancake of billions of stars of which the sun is just one. The thick hub of the galaxy, 30 000 light years away, is in Sagittarius. The actual centre is hidden by dust clouds in space. A scan along the Milky Way with binoculars shows many clusters of stars and some glowing gas clouds. We see the beginning of a lunar eclipse around dawn on the 28th. The Moon begins to enter the outer part of the Earth's shadow at 5:15 a.m. At 6:24 is touching the inner shadow. By 7:30 it is fully immersed in the inner shadow. Southern locations will see more of the eclipse as the Moon sets later in the south. *A light year (l.y.) is the distance that light travels in one year: nearly 10 million million km or 10 13 km. Sunlight takes eight minutes to get here; moonlight about one second. Sunlight reaches Neptune, the outermost major planet, in four hours. It takes four years to reach the nearest star, Alpha Centauri. Notes by Alan Gilmore, University of Canterbury's Mt John Observatory, P.O. Box 56, Lake Tekapo 7945, New Zealand. www.canterbury.ac.nz 180521

Interesting Objects North and East of Overhead in July 2018 Saturn is the brightest 'star' in the region just left of the lid of 'the teapot'. Well above it and to the left is orange Antares, the brightest star in the Scorpion. Saturn is off-white to cream in colour. The near-full Moon crosses the chart region over July 22-26, hiding the Milky Way and the marked interesting objects as it goes. It will be just below Saturn on the 25th. Antares is a 'red giant' star. It is 550 light years away, 20 000 times brighter than the sun, and bigger than Earth's orbit. Its mass or weight is about 12 times that of the sun, so most of the star is very thin gas spread around a hot dense core. Red giants are the last stage in the evolution of stars. The dense core of the star has shrunk and heated up. The outer regions of the star have expanded to a thin red-hot gas. The core is wringing the last of the thermo-nuclear energy out of elements like helium, carbon, oxygen and neon. When that fuel is used up the core of Antares will collapse, triggering a spectacular supernova explosion. Estimates of when range from a few thousand years to two million years. (The sun will become a red-giant in about seven billion years time but it ends up as a white dwarf star, not a supernova.) Antares marks the body of Scorpius. In the evening at this time of year the scorpion is on its back with its tail on the right, curving upward then turning down and curling clockwise. In Maori star lore the tail's hook is the 'fish hook of Maui'. By midnight the scorpion's tail is directly overhead. At the right-angle bend in the tail is a large and bright cluster of stars, NGC 6231, looking like a small comet. It is around 6000 l.y. away. Its brightest stars are 60 000 times brighter than the sun. The cluster is about 8 light years across, similar in size to the Pleiades/Matariki cluster in our summer sky. Were it as close at the Pleiades (440 l.y.) then its brightest stars would be as bright as Sirius. Below the Scorpion's sting is M7, a cluster obvious to the eye and nicely seen in binoculars. M7 is about 800 l.y. away and around 260 million years old. (The older a star cluster, the fewer bright stars it has.) Below M7 and fainter is M6, the 'butterfly cluster'. M6 is around 1300 l.y. away and is half the age of M7. Other clusters worth a look in binoculars are M21, M23, NGC 6167, and NGC 6193. The 'M' objects were listed by the 18 th Century French astronomer Charles Messier. He hunted comets, so made a catalogue of fuzzy objects that could be mistaken for comets. The NGC (New General Catalogue) objects shown are bright enough to have been seen by Messier but are too far south to be seen from Paris where he worked. Above Saturn is the glowing gas cloud M8, the 'Lagoon Nebula'. It is a star-forming region where gas and dust have recently gathered into new stars. ('Recently' in astronomical time scales is the past million years or so.) Ultraviolet light from one particularly hot star is lighting up the leftover gas, making it glow. On colour photos it appears pink due to hydrogen atoms fluorescing in the UV light. Below M8 is M20, the Trifid Nebula, small glowing patch in binoculars, also a pink hydrogen region in photos. Right alongside it is a blue reflection nebula where starlight is scattered by dust. Other nearby nebulae (gas and dust clouds) are M16 and M17. Globular clusters, spherical clusters of ancient stars, are found throughout the region. The brightest is M4 by Antares. It is also one of the closest at 10 000 l.y. away. In binoculars and small telescopes 'globs' appear as round fuzzy spots. Others marked on the chart are M9, M10, M12, M14, M19, M22, M55, M54, M62, M80 and NGC 6541. The concentration of globular clusters in this area was an early clue that the centre of the galaxy lay in this direction. This part of the Milky Way is broad and bright as we are looking to the centre of the galaxy. The actual centre, 27 000 light years away, is hidden from our view by intervening dust clouds. The nearer clouds make gaps and slots along the Milky Way. The hub of the galaxy is a great sphere of stars, called the 'central bulge'. Some of the central bulge is glimpsed in gaps between the dust clouds. At the very centre lies a black hole four million times the sun's mass but only the size of our solar system. Infra-red telescopes, peering through the dust, show stars orbiting the invisible black hole at high speed. Notes by Alan Gilmore, University of Canterbury's Mt John Observatory, P.O. Box 56, Lake Tekapo 7945, New Zealand. www.canterbury.ac.nz 180613

Interesting Objects in the Winter Southern Sky Centaurus, with the bright 'Pointers', and Crux, the Southern Cross are south of overhead, the tightest grouping of bright stars in the whole sky. Originally Crux was the hind legs of the Centaur, the horse-man of Greek mythology. The complete Centaur, with bow, is outlined at left. It was only in the 17 th Century that Crux was split off as a separate constellation. The slow wobble of Earth's axis allowed this part of the sky to be seen from more northerly places in ancient times. The fainter Pointer and the three bluish-white stars of the Crux are all super-bright stars hundreds of light years away. Alpha Centauri is just 4.3 light years* away and the reddish top star of Crux is 90 light years from us. Omega Centauri is a globular cluster, a ball-shaped cluster of millions of stars. Its total mass is six million times the sun s. It is 17 000 light years away and 200 light years across. Globular clusters are very ancient, around 10 billion years old, twice the age of the sun. Omega Centauri is the biggest of the hundred-odd globulars randomly orbiting our galaxy. It may originally have been the core of a small galaxy that collided with the Milky Way and was stripped of its outer stars. 47 Tucanae, near the SMC, is a similar but smaller cluster about 16 000 light years away. Coalsack nebula, left of Crux, looks like a hole in the Milky Way. It is a cloud of dust and gas 600 light years away, dimming the distant stars in the Milky Way. Many dark nebulae can be seen along the Milky Way, appearing as slots and holes. These clouds eventually form new stars. The Jewel Box is a compact cluster of young bright stars about 7000 light years away. The cluster formed about 16 million years ago. To the eye it looks like a faint star close by the second-brightest star in Crux. A telescope is needed to see it well. Eta Carinae nebula, a luminous spot in the Milky Way to the right of Crux and lower, is a glowing gas cloud about 8000 light years from us. The thin gas glows in the ultra-violet light of nearby hot young stars. The golden star in the cloud, visible in binoculars, is Eta [Greek e ] Carinae. It is estimated to be to be 80 times heavier than the sun. It is four million times brighter than the sun but is dimmed by dust clouds around it. It is expected to explode as a supernova in the next few thousand years. Many star clusters are found in this part of the sky. Large & Small Clouds of Magellan (LMC & SMC) appear as two luminous clouds, easily seen by eye in a dark sky. They are galaxies like the Milky Way but much smaller. Each is made of billions of stars. The LMC contains many clusters of young bright stars seen as spots of light in binoculars. The LMC is 160 000 l.y away; the SMC 200 000 l.y. Both are very close by for galaxies. Tarantula nebula is a glowing gas cloud in the LMC. The gas glows in the ultra-violet light from a cluster of very hot stars at the centre of the nebula. The cloud is about 800 light years across. It is easily seen in binoculars and can be seen by eye on moonless nights. This nebula is one of the brightest known. If it was as close as the Orion nebula then it would be as bright as the full moon. *A light year (l.y.)is the distance that light travels in one year: nearly 10 million million km, or 10 13 km. Sunlight takes eight minutes to get here; moonlight about one second. Sunlight reaches Neptune, the outermost major planet, in four hours. It takes four years to reach the nearest star, Alpha Centauri. Text and photos by Alan Gilmore, Mt John Observatory of the University of Canterbury, P.O. Box 56, Lake Tekapo 8770, New Zealand. www.canterbury.ac.nz 120803