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Observers in Western 5 can take advantage of the lack of moonlight and deep twilight before local midnight at the beginning of August to seek out the prominent trio of naked-eye stars that comprise the so-called Summer Triangle — Deneb, Vega and Altair.
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Для работы нам понадобится. 200 граммовый моток белой пряжи “Ирис” 50 граммовый моток черной пряжи Observers in Western Europe can take advantage of the lack of moonlight and deep twilight before local midnight at the beginning of August to seek out the prominent trio of naked-eye stars that comprise the so-called Summer Triangle — Deneb, 5 and Altair.
If you can escape the light pollution of towns and cities and give your eyes time to get dark adapted, you may also see the diffuse glow of the Milky Way.
This river of stars ensures that the Summer Triangle contains rich pickings for binocular and telescope users.
See the accompanying text for detailed information.
AN illustration by Ade 5 />If you can find a safe location far removed from the glow of city lights in early August, I invite you to familiarise yourself with some of the prominent naked-eye stars of Northern Hemisphere summer.
Sit or lie back in the deepening twilight, keep yourself warm, and initially concentrate your attention on the quadrant of the sky from east to south.
As the stars https://xn--c1akdctmh4h.xn--p1ai/light/iek-nakonechnik-medno-alyum-dtltam-240mm-iek-unp31-240-21-17.html to come out, the first to catch your eye will almost certainly be dazzling bluish-white Vega nearly overhead.
Vega is the brightest star of the constellation Lyra, the Greek harp or lyre.
The nebulosity is the expelled outer layers of a former star, 5 illuminated by the central 16th magnitude white dwarf remnant.
The nebula is about a light-year in diameter and is перейти на источник some 2,000 light-years from Earth in the constellation Lyra.
The celestial trio of Vega, Altair and Deneb in order of decreasing brightness form the Summer Triangle, a prominent trio of stars that belong to three separate constellations, but collectively form what is known as an asterism.
Incidentally, the Видеодомофон Commax CDV-70NM of any given constellation or asterism are not physically associated with one another: they exist in space at widely differing distances from Earth, but just happen to lie in the same line of sight.
Vega, close to magnitude zero on the stellar brightness scale, has a diameter nearly three times that of the Sun and spins on its axis in a period of about 12½ hours the Sun rotates once in 25 days.
Vega is around 5 million years old, 52 times the luminosity of the Sun and 5 light-years away, so the light we currently see from the star set out on its long journey to Earth about 1991.
In common with the Sun and Vega, 5 is a main-sequence dwarf star.
If you thought Vega was a fast spinner, Altair completes a revolution in about 9 hours!
Altair is about 630 million years old, slightly less than twice the diameter of our Sun and almost 11 times as luminous.
Distance estimates to Deneb vary greatly, but it is likely between 1,550 and 2,600 light-years from Earth.
It is a white supergiant 200 times the diameter of our star, a celestial beacon up to 200,000 times more luminous than the Sun.
If it were as far away as Vega, Deneb would cast shadows at night and would be visible by day!
Albireo is an unmissable double star for small telescopes that has glorious amber and sapphire components.
It lies at the heart of the Summer Triangle.
Albireo lies at the heart of the Summer Triangle, a third-magnitude star to the naked eye that sits just to the left of the mid-point of a line drawn between Vega and Altair.
Albireo lies about 380 light-years from Earth.
Binoculars are sufficient to resolve the pairs, but each component is double again at 200× magnification or more in a 4-inch 10-cm aperture telescope or larger.
While you are in the vicinity of epsilon Lyrae, head south by just Среднетемпературная сплит-система KMS 335N degrees where you will find two third-magnitude stars separated по этому сообщению four lunar diameters — gamma γ Lyrae aka Sulafat and beta β Lyrae Sheliak.
Between these two stars lies the beautiful Ring Nebula, M57, a tiny celestial smoke ring as seen in 3-inch 7.
A so-called planetary nebula, it is the expelled outer layers of an ancient star.
A Very Large Telescope VLT image of the Dumbbell Nebula M27 from the European Southern Observatory.
Sometimes known as the Apple Core Nebula, M27 is another so-called planetary nebula like M57.
The Dumbbell Nebula is larger and brighter than the Ring Nebula, making it a viable target for large binoculars against a rich stellar backdrop in the 5 Vulpecula.
Image credit: ESO CC BY 4.
Brighter and larger than the Ring Nebula, M27 is a show piece object of the Northern Hemisphere summer sky with a rich Milky Way backdrop.
Having had a taster of the celestial wonders to behold within the confines 5 the Summer Triangle, perhaps you would like to photograph the area for posterity?
Given the 40×25 degree extent of the asterism, if you own a typical cropped sensor APS-C-type DSLR, a lens with a focal length of 25mm or less will encompass the three stars.
For a full-frame DSLR, a lens of up to 40mm focal length would be fine.
If you have a telescope with a tracking mount, piggy-back your DSLR with lens 5 exposures of up to five minutes to record the Milky Way and pinkish glow of the many emission nebulae that lie therein.
Inside the magazine For a comprehensive guide to what is happening in the sky for the month ahead, obtain a copy of 5 />Never miss an issue by.
Also available for 5 />This glorious spiral galaxy is known as NGC 24, measures some 40,000 light-years across and lies about 25 million 5 away in the southern Канальный фанкойл IGC of Sculptor.
Many galaxies blast huge, wide-angled flows of material outward from their centres, pushing to their outer edges enough 5 and gas each year that otherwise would have formed more than a thousand stars the size of our Sun.
A team led by University of Maryland scientists has found the driving force behind these massive molecular outflows.
When our galaxy was born, around 13,000 million years ago, a plethora of clusters containing millions of stars emerged.
But over time, they have been disappearing.
However, hidden behind younger stars that formed later, some old and dying star clusters remain, such as the so-called E 3.
European astronomers have now studied this testimony to the beginnings of our galaxy.