The brightest star in the constellation Ursa Major add your price to the comment base. Constellation Ursa Major - myths and legends about the origin

The constellation Ursa Major (Ursa Major) is seven particularly spectacular stars that are easy to find in the sky. These are stars of the second magnitude (the least one is the upper left star of the "bucket"). Excluding these stars, there are 125 more stars in the constellation brighter than the 6th magnitude.

The size of the constellation Ursa Major

The constellation Ursa Major covers an area of ​​1280 square degrees in the sky - this is one of the largest constellations. The size of the constellation significantly exceeds the boundaries of the "bucket with a handle." Measurements have revealed, for example, that the "bucket" stars are located at rather unequal distances from us: the nearest star (Aliot) is 50 light-years away from us, and the most distant (Benetnash) is 4 times more. Near the star Mizar (which means "horse" in Arabic) is an almost imperceptible asterisk Alkor ("rider") of approximately the fifth magnitude.

Ursa Major in astronomy

For beginners-lovers of astronomy, Ursa Major can serve as a special "training ground":

  1. this constellation, as a starting point, as a guide, makes it possible to search for numerous other constellations;
  2. very clearly shows the apparent diurnal rotation of the sky and the rearrangement of the view starry sky during a year;
  3. having remembered the angular distances between the stars of the "ladle", it is possible to carry out approximate angular measurements;
  4. amateur astronomers who have a barely perceptible telescope can view double and variable stars inaccessible to the naked eye in the constellation Ursa Major and even distinguish some galaxies (including the famous "exploding galaxy" M82.

Constellation Ursa Major: myths and legends

The constellation "bucket" has been known to people since ancient times. The ancient Greeks believed that constellation Ursa Major- this is the nymph Callisto, companion of Artemis, beloved of Zeus. But one day she incurred the disgrace of the goddess, transgressing the rules carried out by the companions of Artemis. And she turned her into a bear and set dogs on her. To protect his beloved, Zeus had to raise her to heaven.

Be that as it may, this event is dark: perhaps Zeus himself, hiding his own betrayals from the jealous wife of Hera, turned Callisto into a bear, and Artemis organized a hunt for her, either by mistake, or by teaching the far-sighted and vengeful Hera. Perhaps, in the end, that Hera, for the sake of revenge, herself turned Callisto into a constellation, and Callisto's son Arkad arranged a hunt for her by mistake. From time to time, some unknown girlfriend of Callisto, who at the same time turned into Ursa Minor, is also involved in this story.

Another myth, described by Philemon, tells that the baby Zeus was forced to reincarnate into a snake, and turn his nannies into bears, when his father Cron was looking for him, in order to, according to his habit, eat the newborn. From this place, Ursa Major and Ursa Minor and the constellation Serpent came from. The constellation Serpent is not in the sky, probably - this is the Dragon. This is similar to the close location of all three constellations. However, this myth is possibly just a poetic fantasy.

Constellation Ursa Major on the constellation map

Ursa Major can be admired during the day. This can easily be done by finding it on one of the interactive ones. On the maps, you can find other large and small constellations and look at them in a big approximation. All in your hands!

Constellation Ursa Major

Ursa Major is a constellation in the northern hemisphere of the sky. Seven Ursa Major make up a figure resembling a ladle with a handle. The two brightest stars, Aliot and Dubhe, have magnitudes of 1.8 apparent magnitudes. According to the two extreme stars of this figure (α and β), you can find the Polar Star. Best conditions visibility - in March-April. It can be seen throughout Russia all year round (with the exception of the autumn months in southern Russia, when the Big Dipper descends low to the horizon).

Stars and asterisms

Ursa Major is the third largest constellation (after Hydra and Virgo), whose seven bright stars form the famous Big Bucket; this asterism has been known since antiquity among many peoples under different names: the Rocker, the Plow, the Elk, the Wagon, the Seven Wise Men, etc. All the stars of the Bucket have their own Arabic names:

  • Dubhe (α Ursa Major) means "bear";
  • Merak (β) - "lower back";
  • Fekda (γ) - "thigh";
  • Megrets (δ) - "the beginning of the tail";
  • Aliot (ε) - the meaning is not clear (but, most likely, this name means "fat tail");
  • Mizar (ζ) - "sash" or "loincloth".
  • The last star in the bucket handle is called Benetnash or Alkaid (η); in Arabic, "al-Qaeed banat ours" means "the leader of the mourners." This poetic image is taken from the Arab folk interpretation of the constellation Ursa Major.

In the system of naming stars with Greek letters, the order of the letters simply corresponds to the order of the stars.

Another interpretation of asterism is reflected in the alternative name Hearse and Wailers. Here, asterism is thought of as a funeral procession: in front of the mourners, led by a leader, behind them are a funeral stretcher. This explains the name of the star η Ursa Major "the leader of the mourners."

5 inner stars of the Bucket (except for the extreme α and η) really belong to a single group in space - the moving cluster Ursa Major, which moves quite quickly across the sky; Dubhe and Benetnash are moving in the opposite direction, so the shape of the Dipper changes significantly in about 100,000 years.

The stars Merak and Dubhe, which form the wall of the Bucket, are called pointers, since the straight line drawn through them rests on the North Star (in the constellation Ursa Minor). Six stars of the Bucket have a shine of the 2nd magnitude, and only Megrets is of the 3rd magnitude.

Near Mizar, which was the second among those discovered with a telescope (Giovanni Riccioli in 1650; according to the early 2000s, it was probably observed as a double as early as 1617 by Galileo). A keen eye sees a star of magnitude 4 Alcor (80 Ursa Major), which in Arabic means “forgotten”, or “insignificant”. It is believed that the ability to distinguish the star Alcor has been a recognized test of vigilance since ancient times. The pair of stars Mizar and Alcor is often interpreted as an asterism " horse and rider».

Peculiar asterism Three gazelle jumps of Arabic origin consists of three pairs of closely spaced stars, and the pairs are on the same straight line and separated by equal distances. Associated with hoofprints of a gazelle moving by jumps. Includes stars:

  • Alula North and Alula South (v and ξ, first jump),
  • Taniya North and Taniya South (λ and μ, second jump),
  • Talita North and Talita South (ι and κ, third jump).

Aliot, Mizar and Benetnash form an extended arc that points to Arcturus, the brightest star north of the celestial equator, and also the brightest star visible in the spring in the mid-latitudes of Russia. As this arc extends further south, it points to Spica, the brightest star in the constellation Virgo.



The constellation of this month is familiar to any inhabitant. northern hemisphere. Throughout history, Ursa Major has been an easily recognizable figure in the night sky. She seemed to be a bear, then a plow, they recognized in her both three hunters with a bear, and a bear with a cart. (Did I remember to mention that she looked like a bear? :-) In the asterism - the Big Dipper - one guesses, probably, the largest number of figures for the night sky. The bucket serves as a reference point for finding many of the constellations of the Northern Hemisphere, and in itself is an open cluster. Designated Collinder 285, or the Ursa Major Moving Group of Stars, it includes the five central stars of the Bucket and is located just 70 light-years from Earth. Cr285 is best viewed with the naked eye.

Name Type The size Sound led
Objects NGC 2841 Galaxy 8.1"x3.5" 9,3
NGC 2976 Galaxy 5.9"x2.7" 10,1
M81 Galaxy 24.9"x11.5" 7
M82 Galaxy 11.2"x4.3" 8,6
NGC 3077 Galaxy 5.2"x4.7" 10
IC 2574 Galaxy 13.2"x5.4" 10,2
M 108 Galaxy 8.6"x2.4" 9,9
M97 planetary nebula 2,8 9,9
NGC 3718 Galaxy 8.1"x4" 10,6
NGC 3729 Galaxy 2.9"x1.9" 11
NGC 3953 Galaxy 6.9"x3.6" 9,8
M 109 Galaxy 7.5x4.4 9,8
Cr285 cluster of stars 1400" 0,4
M 101 Galaxy 28.8"x26.9" 7,5
NGC 5474 Galaxy 4.7"x4.7" 10,6
Complex objects Hickson 56 cluster of galaxies 14,5
Hickson 41 cluster of galaxies 13,9
Many of this month's targets are visible through binoculars. Bucket is a cornucopia of deep sky entertainment. Located in the Milky Way and spanning 1280 degrees of the sky, this vast stretch of space is visible far into the intergalactic limits. Not surprisingly, Ursa Major is rich in galaxies and clusters of galaxies. But there are many other interesting targets as well. Thousands of galaxies with magnitudes above 20 (in practice, 812 are available with magnitude 15 and brighter, of which 56 are brighter than magnitude 12), 7 Hickson groups, 327 Abel galaxy clusters, 641 quasars (the brightest is MKN 421, magnitude 13, 5, 11:05, +38 degrees 11 minutes), two planetary nebulae, 9 diffuse nebulae and one globular cluster (Palomar 4) - and that's not all.
In the Big Dipper (BM) there are several famous stars that are not included in the Bucket. It contains Lalande 21185- a red dwarf with a magnitude of 7.49, which is the fourth closest to solar system star and is located only 8.1 light years away. Lalande 21185 is the brightest red dwarf visible in the Northern Hemisphere. BM also hosts the 6.45 magnitude Groombridge 1830 star, which is 28 light-years away and is moving at the third fastest speed of any known star. Groombridge 1830 is a class II star and is no younger than many globular clusters. Another famous star in Ursa Major - 47 Ursa Major, which is one of many sun-like stars and may have inhabited planets.
There are a total of 7 Messier objects in Ursa Major, 6 of which are of visual interest. (We'll leave out M40, although double-star observers might want to look at it.)
The first ultra-deep image of Hubble was also taken in Ursa Major, Hubble Deep Field: 12:36:49.4000s +62d 12" 58.000". This tiny window (like a grain of rice at arm's length) allowed the Hubble telescope to look beyond our galaxy and capture at least 1500 galaxies with a 10-day exposure. Almost everything you see in the image below is galaxies. (If you have high speed internet, be sure to check out "Hubble Deep Field Enlargement".)
Before we go any further, let's take a closer look at the stars that make up the Bucket. If you start from the handle, here is Alkaid, then on the bend of the handle is the double Alcor and Mizar visible to the naked eye. Going down the bucket below, we get to Aliot, and a little further we find the first of the stars of the bucket itself - Megrets. Below we come across first Fekda, then Merak and Dubhe. One of the first things any beginner learns is to draw a line through Merak and Dubhe to find the North Star, the north star of Ursa Minor.
I have read in various sources that many civilizations and cultures use Alcor and Mizar as a test of visual acuity, but this puzzles me a little, since I myself have never found it difficult to separate them. Frankly, Ursa Major is an intimidating constellation to write a guide to: it's gigantic and holds a dozen targets even for an observer with the most modest telescope. So I focused on those objects that I myself consider the brightest and most exciting. But I left one area aside - Walter Scott Houston called it the "goblet of the night" - the bowl of the Ladle itself. I recommend that after this month's tour you take some time to look at the area inside the bowl: several targets are suitable for an average telescope. I will provide you with a search map, and at the end of the article you will find a list of bright galaxies in and around the bowl.
Let's start the evening tour at the bottom of the bowl, on the line between Fekda and Merak. Exactly southeast of Phekda (the star on the side of the bottom, which is closer to the handle), we will find Messier's first target for today: M 109.
Méchain's discovery of M 109 was known to Messier, but did not appear on "his" list until the middle of the 20th century. Messier's original list consisted of 103 targets, including several dubious ones (M40 - a double star, and the "missing" messier - M 102). M 109 Photographer Jason Blaschka
Jason Blaschka's picture of M 109 is striking, but not too similar to what I see even in the largest telescopes. A few features: even in 4-inch apochromat (under good skies), the galaxy bears a noticeable resemblance to the fighter jet from " star wars» (TIE-fighter) - the central bridge is often visible, but on a rare night I can catch a hint of spiral arms through a small aperture.
Jay Michaels did an excellent sketch - a great example of what can be seen with an 8-10" telescope on a good night. While you're here, take some time to find NGC 3953, about a degree south of M 109. Then move to the middle of the bottom of the bowl, go down a little to the south and find a nice cluster of objects - NGC 3718,NGC 3729 and one of the complex objects of this month Hickson 56.

At an average magnification, 3718 and 3729 are in the same field of view. I would say that 3718 is about three times the size of 3729, but the galaxies are quite similar to each other in my opinion. In large telescopes, I see that both have prominent (albeit faint) cores, and diffuse outer halos. A little further south you will find Hickson 56 - but we will return to it later.
Move towards the star at the base of the bucket (Meraku) with a wide-angle eyepiece at low power, and you will stumble upon a random celestial pair. First in the field will be M97 - Owl Nebula, a planetary nebula discovered by Pierre Méchain in 1781. I believe that this is one of the few objects that actually resembles its nickname. Even with a small telescope (under good conditions) I can catch a glimpse of the outlines of dark spots - owl eyes. The nebula is quite large, so its surface brightness is rather low. Some observers claim to have seen blue or green on the disc's surface. On a superb observing night, I picked up shades of green with a large telescope, but usually the disk looks just grey.

The M97 shot by Rick Krejecki is amazing. Check out the high resolution version on his website (http://www.ricksastro.com/DSOs/owl_XT_xscope.shtml) - a lot of time can be spent just counting the tiny background galaxies. I wonder if any of them have been visually identified by observers with giant telescopes?
If you have a desire to look at extragalactic targets, you don’t have to go far - a little closer to Merak you will find a spiral galaxy M 108, located edge to us. Experiment a little with different magnifications - see if you can make out the mosaic structure and if you can detect any presence of an external halo.

A superb shot by Tom Nicolades shows a shattered and swaying electric blue M 108 and M 97 in one shot. At a low magnification of the wide-angle eyepiece (the field of view of the telescope + eyepiece system, TFOV, must be greater than 1 degree), both objects are easy to catch in the same field of view.

While we're here, let's jump over Ursa's forepaws and take a quick look at NGC 2841. This 9.2-magnitude galaxy is like a beacon of hope for medium-sized telescopes. The bright core region is surrounded by a slightly fainter halo. If you have a large telescope, look for a strip of dust i.e. abrupt fading of the halo on one side of the galaxy.

M 81/M 82 - Photographer John Moody
Having finished with 2841, we move on to a pair of real pearls of the Big Dipper, M81 and M82.
M 81 and 82 make up an exciting pair of galaxies that can be seen even with small binoculars. They are separated by only 3/4 degrees, are visible through wide-angle eyepieces and are a wonderful pair. They were discovered by Bode in 1774 and are an illustration of a galactic morphology that at first glance does not allow for great differences. Both galaxies are members of a small cluster of galaxies called the M 81 group (which is located nearby, 10 million light years away), so it would be appropriate to discuss M 81 first. In small telescopes, M 81 is a bright oval, but large telescopes begin to show it spiral structure. Of the two, M 81 is by far the larger and brighter, and looks like a classic spiral galaxy in long-exposure photographs. M 82, on the other hand, is not curled properly and looks like it has been defeated in some huge celestial conflict. In an 18" telescope, I see it curved at one end, with distinct mottling, and an almost distinct septum about a third of the way from one of the edges. It is slightly dimmer than M 81, but visually I find it much more impressive.
It is worth noting that this is one of the few DSOs in which visualists observe color, but so far not even in 80mm telescopes. A friend of mine in Arizona, who has access to a 30" telescope, describes seeing red or pink color, and I see nothing of the kind, although I observe this object with telescopes up to 25” in diameter. I think that this will require excellent night, good optics and the maximum aperture that you can afford. But don't despair! In my opinion, M 82 is one of the most beautiful targets in the night sky, with or without color. Even in small telescopes, this pair is stunning and can be picked out in dark skies with minimal help from optics.

Carol Lakomiak's sketch of this area gives a great idea of ​​what can be seen with large binoculars or a small telescope.
As you can see from the map, there are many other targets in this region. Take some time and scout everything around - follow NGC 3077, 2976 and IC 2574. In my opinion, NGC 3077 and 2976 in large telescopes are similar in brightness to M 81 in small apertures. If you use the "star trail method" in search of M81 and linger on one of them, embarrassment can happen. Your expectations should always match the aperture.
We haven't even begun to really explore the possibilities of the Big Dipper, and yet we will make one more stop, and then we will move on to two complex objects.
Go around the top of the Bucket and keep moving away from the handle to find M 101- galaxy pinwheel (Pinwheel)*. It was discovered by Méchain in 1781 and looks really spectacular in a large telescope, showing an obvious spiral structure and patchiness in the arms.
M101 has a large, loose surface that can be confusing and difficult to see with a small telescope. Remember when you're looking for this large object: it's about 2/3 the size of a full moon, but the surface shininess is very low, so be careful to gradually separate it from the background. The galaxy is huge - reference books indicate from 170,000 to 190,000 light-years across. It is approximately 25 million light-years distant and contains some of the most spectacular and vast star-forming regions known.
Many of these stellar birth centers are bright enough to merit their own NGC numbers: NGC 5441, 5447, 5450, 5449, 5451, 5453, 5458, 5461, 5462, and 5471.
NGC 5471 is the largest and brightest HII region in M101, much larger than anything comparable in the Milky Way (5471B is presumed to contain a hypernova). It is visible in large telescopes, and while I often recommend viewing galaxies at high magnification (my favorite galactic horse, the Nagler 13t6 eyepiece and the Obsession 18” provide about 180x magnification and a nice wide field of view), the detailed structure of M101 my advice would be to explore at high and low magnifications and see what works best for you personally. Be sure to take a look at the brightest HII regions. Note that the image below does not capture 5450 and 5447 - 5447 is south of 5450.
Region II. Galaxy M 101 Like M81, M101 is the main member of the eponymous group of galaxies, so while you are in this area, keep a close eye on other robbers as well. The brightest are NGC 5474 and NGC 5473, but there are many others.

M101. Photographer James Jacobson
Complex objects In the Big Dipper there are several objects worthy of being called complex. The first thing that comes to mind is the 7 Hickson groups, the Palomar 4 globular cluster, and a fairly bright quasar. Quasars are interesting on their own, not what you see in the eyepiece, and the Palomar 4 can certainly be handled in a large telescope and in dark terrain, so in general I lean towards a group of galaxies. Given the above, I present as complex objects the two "brightest" Hicksons in Ursa Major: Hickson 56 and Hickson 41.
Hickson 56 lies directly south of a pair of galaxies we visited earlier - NGC 3729 and 3718.
Note that the marker marking the position of Hickson 56 is slightly offset in the image above. Hickson 56 has 5 components (although not all of them can be seen) whose brilliance ranges from 16.2 to 15.8, and they are all tiny (the largest takes 1.3x2 arcseconds), so be sure to handle them in good conditions and with a large aperture.
Iiro Sairanen from Finland observed a Hickson 56 with a 16" newton at 292x and provided the following sketch:
Another tricky object of the month - Hickson 41. Hickson 41 is a bit harder to get to, but slightly brighter. Again, note that it does not match perfectly with the maps shown. Rely on DSS images. There are 4 components with magnitudes from 14.6 to 18.1, where the largest element is only 1.5x2 arcseconds in size. Alvin Huey, observing at 377x and 528x, wrote in his excellent Hickson Group Observer's Guide that he failed to catch the fourth member of the group in a 22” f4.1 dobson.

I was able to capture three of these four galaxies with the 18” f4.5 from my driveway, but it took a bit of tweaking - it took a good evening, I covered my head with a towel to get rid of the extraneous light, and used very high magnifications (600x), to sufficiently darken the background of the sky. Finally, I had to resort to tapping on the telescope to make sure I tracked down all three members of the group. The Hicksons, for the most part, are not casual sightings or glimpses. To get a glimpse of these tiny clusters of interacting galaxies, use every trick in the book, including high magnification and tenacity. Additional Goals
As I wrote above, Walter Scott Houston called this area "the cup of the night." Here is a map that may give you a few more reasons to travel around the bowl of the Ladle. And this is the necessary information about additional goals:

* Reference from Wikipedia: Russian name The Pinion Wheel is the result of a mistranslation from English. The pinion wheel is used in gears, it resembles a squirrel wheel of two parallel rims connected by pins - pins; in English, both the lantern wheel and the spinner (breeze) (a children's toy, a multi-blade impeller mounted on an axis (pin) and spun by the wind) are designated by the term pinwheel, however appearance the galaxy, with its spiral arms, looks exactly like a pinwheel, not a lantern wheel.

Until we meet again
Tom T.

known to people since antiquity. For example, the ancient Greeks believed that the constellation Ursa Major is the nymph Callisto, the companion of Artemis, the beloved of Zeus. But one day she incurred the wrath of the goddess by violating the rules imposed on the companions of Artemis. And she turned her into a bear and set dogs on her.

Legend

To save his beloved, Zeus was forced to take her to heaven. However, the story is dark: perhaps Zeus himself, hiding his betrayals from the jealous wife of Hera, turned Callisto into a bear, and Artemis arranged a hunt for her, either by mistake, or at the instigation of the far-sighted and vindictive Hera. It is possible, finally, that Hera, for the sake of revenge, herself turned Callisto into a constellation, and Callisto's son Arkad arranged a hunt for her by mistake. Sometimes some unknown girlfriend of Callisto, who at the same time turned into Ursa Minor, is also woven into this story. Another myth, told by Philemon, tells that the baby Zeus was forced to turn into a snake, and turn his nannies into bears, when his father Kron was looking for him, in order to, according to his habit, eat the newborn. This is where Ursa Major and Ursa Minor and the constellation Serpent came from. The constellation Serpent is not in the sky, probably - this is the Dragon. This is similar to the proximity of all three constellations. However, this myth seems to be just a poetic invention of a comedian.

In the middle latitudes, Ursa Major is one of the non-setting constellations.

Ursa Major on the star map

(area = 1280 square degrees)

The seven brightest stars of this constellation ("bucket with a handle") are easily found in the sky by everyone. These are stars of the 2nd magnitude (only one is weaker - the upper left star of the "bucket"). In addition to them, in the constellation there are 125 more stars brighter than the 6th magnitude. The boundaries of the constellation go far beyond the "bucket with a handle." The constellation Ursa Major - occupies an area of ​​​​1280 square degrees in the sky - one of the largest constellations. Measurements showed, for example, that the "bucket" stars are at very different distances from us: the nearest one (Aliot) is 50 light-years away from us, and the distance to the most distant one (Benetnash) is four times greater. Near the star Mizar (which means "horse" in Arabic), people with good eyesight see a faint star Alcor ("rider") of about 5th magnitude.

For beginner astronomy lovers, the Big Dipper can serve as a kind of "training ground": firstly, this constellation, as a starting point, as a guide, allows you to find many other constellations; secondly, it very clearly demonstrates the visible daily rotation of the sky and the change in the appearance of the starry sky during the year; thirdly, having memorized the angular distances between the "ladle" stars, one can perform approximate angular measurements; finally, amateur astronomers who have a small telescope at their disposal can observe double and variable stars inaccessible to the naked eye in the constellation Ursa Major and even see some galaxies (including the famous "exploding galaxy" M82).

Constellation Ursa Major

star formation

in the galaxy M82 is proceeding at a powerful pace - the birth (and death) of massive stars in it occurs about ten times faster than in our Milky Way. Winds from massive stars and supernova explosions created a huge cloud of gas emanating from this remarkable explosive galaxy. For the last billion years, two giant galaxies M82 and M81 have been waging a gravitational duel. The gravitational force of each of the galaxies exerts powerful impact to another during close passages that occur every hundred million years. On its last approach, M82's gravity caused density waves to propagate around M81, resulting in M81's beautiful spiral arms. In turn, M81 in M82 initiated violent star formation and the formation of colliding gas clouds with such high energy that the galaxy glows in X-rays.

In a few billion years, only one of the two galaxies will remain. M81 itself, also referred to as NGC 3031, is one of the brightest galaxies in the sky. In this galaxy, the second most powerful supernova of the present time SN 1993J (the flash was observed on March 28, 1993), which could be observed from Earth, broke out. The star SN 1993J is part of a binary system and, after the explosion, left a surviving huge satellite star in its orbit. Astronomers study the remnant of SN 1993J using a companion star. scientists have long sought to detect a neutron stellar or black hole forming in real time. Supernovae are the main sources of heavy elements in the Universe and play an important role in the evolution of galaxies. Supernova SN 1993J, which initially seemed quite ordinary, puzzled scientists a lot when it turned out that its ejection was too rich in helium, and instead of gradually fading, the explosion products began to increase in brightness in a strange way. Astronomers guessed that an ordinary red supergiant star could not turn into such an unusual supernova. Then there was an assumption that the flared supergiant was paired with another star, the gravity of which shredded the outer shell of the dying neighbor shortly before the explosion.

Archival images of the M81 galaxy before the supernova explosion showed a red supergiant star, which subsequently exploded as SN 1993J. During the 250 years before the explosion of SN 1993J, about 10 solar masses of gas were blown off the surface of the red supergiant by its companion, which in the future should also become a supernova with the formation of a neutron star or black hole. The galaxy is comparable in size to the Milky Way. A careful study of the variable stars M81 made it possible to very accurately determine the distance to the galaxy - it turned out to be equal to 11.8 million light years.

Facts

With an area of ​​1280 square degrees, it is in third place in terms of size. Covers the second quadrant in the northern hemisphere (NQ2). Can be found in latitudes from +90° to -30°. Adjacent to Bootes, Giraffe, Veronica's Hair, Dragon, Lion, Lesser Lion, Hounds and Lynx.

It contains 7 Messier objects: Messier 40, Messier 81 (NGC 3031), Messier 82 (NGC 3034), Messier 97 (NGC 3587), Messier 101 (NGC 5457), Messier 108 (NGC 3556) and Messier 109 (NGC 3992).

Also contains 13 stars with planets. The brightest is Epsilon Ursa Major, whose apparent magnitude reaches 1.76. There are two meteor showers: Alpha Ursa Majorids and Leonids-Ursids. Included in the Ursa Major group along with Bootes, Giraffe, Hounds, Veronica's Hair, Dragon, Lesser Lion, Lynx, Ursa Minor and Northern Crown.

MYTHOLOGY

Callisto(Greek Καλλιστώ) - in Greek mythology, the Arcadian, the daughter of Lycaon, was among the companions of Artemis the huntress, was turned into a bear because she did not retain her virginity and gave birth to Arkad and Pan. According to another version, she was turned into a beast by Zeus, who tried to hide her from the jealousy of Hera.

When Arkad, who did not know her and was brought up by Maya or Hermes, wanted to kill her, Zeus transferred both to the sky in constellations: Callisto- Big Dipper, Arcade- Arktofilakom (Keeper of the bears, now) or the star Arcturus in this constellation. Hera, who pursued her with her anger, deprived her of the opportunity to refresh herself part of the day in the waves of the ocean; therefore the Big Dipper never sets.

In the picture - a painting - Francois Boucher "Callisto and Jupiter Zeus assumes the image of Artemis"

In Chinese astronomy, the seven bucket stars are called the Northern Dipper (Beidou). In ancient times, the ladle handle pointed almost to the pole and was used by the Chinese to keep time.

The constellations Ursa Major, and are associated with one myth, which even today excites us with the tragedy described in it. Long ago, King Lycaon ruled Arcadia. And he had a daughter, Callisto, known throughout the world for her charm and beauty. Even the lord of heaven and earth Thunderer Zeus admired her divine beauty as soon as he saw her. Secretly from his jealous wife - the great goddess Hera - Zeus constantly visited Callisto in her father's palace. From him she gave birth to a son Arkad, who quickly grew up. Slender and handsome, he skillfully shot from a bow and often went hunting in the forest. Hera learned about the love of Zeus and Callisto. Falling into a rage, she turned Callisto into an ugly bear. When Arkad returned from hunting in the evening, he saw a bear in the house. Not knowing that this was his own mother, he pulled the bow string ... But Zeus did not allow Arkad, although unwittingly, to commit such a grave crime. Even before Arkad fired an arrow, Zeus grabbed the bear by the tail and quickly soared with her into the sky, where he left her in the form of the constellation Ursa Major. But while Zeus was carrying the bear, her tail began to lengthen, which is why the Big Dipper has such a long and curved tail in the sky. Knowing how much Callisto was attached to her maid, Zeus took her to heaven and left her there in the form of a small but beautiful constellation. Zeus and Arcada moved to the sky and turned into a constellation. forever doomed to protect his mother, the Big Dipper.19 Therefore, he firmly holds the leashes of the Hounds of the Dogs, which bristled with rage and are ready to pounce on the Big Dipper and tear it apart.

There is another version of this myth. Forever young goddess Artemis, dressed in hunting clothes, with a bow, a quiver and a sharp spear long time wandered through the mountains and forests in search of good game. Following her, her companions and maids moved, resounding with laughter and songs. Mountain peaks. The girls were one more beautiful than the other, but the most charming was Callisto. When Zeus saw her, he admired her youth and beauty. But the servants of Artemis were forbidden to marry. To master it, Zeus went to the trick. One night, in the form of Artemis, he appeared before Callisto... From Zeus, Callisto gave birth to a son, Arkad, who quickly grew up and became an unsurpassed hunter. The jealous wife of Zeus Hera, who learned about her husband's love affair, unleashed her anger on Callisto, turning her into an ugly clumsy bear. One day, the son of Callisto Arkad was wandering through the forest, and suddenly a bear came out of the bushes to meet him. Not knowing that it was his mother, he pulled the string, and the arrow flew into the bear ... But Zeus, who vigilantly guarded his beloved Callisto, at the last moment took the arrow away, and she flew past. At the same time, Zeus turned Arcade into a little bear cub. After that, he grabbed the bear with the cub by the tails and carried them to the sky. There he left Callisto to shine in the form of the beautiful constellation Ursa Major, and Arcada - in the form of the constellation. In the sky, in the form of the constellations Callisto and Arkad, they became even more beautiful than on Earth. Not only people admired them, but Zeus himself. From the top of Olympus, he often looked at the constellations Big and enjoyed their beauty and continuous movement across the sky. Hera was unpleasant when she saw her husband admiring his pets. She turned with an ardent prayer to the sea god Poseidon so that he would never allow the Big Dipper to touch the sea. Let her die of thirst! But Poseidon did not heed the pleas of Hera. Could he really let the beloved of his brother, Zeus the Thunderer, die of thirst?! Ursa Major continues to circle around the pole, while once a day she descends low over the northern side of the horizon, touches sea ​​surface, quenches thirst and then rises again, attracting the eyes of people and gods with its beauty.

Interesting Facts

The constellation Ursa Major is depicted on the flag of Alaska.

The flag of Alaska (eng. Flag of alaska) is one of the symbols of the US state of Alaska.

The flag was designed in 1926 by 13-year-old Alaska Native Benny Benson, and in 1927 adopted as the official symbol of the Territory of Alaska, which became a state on January 3, 1959.

Eight gold (yellow) five-pointed stars are depicted on a blue background: seven in the image of the Big Dipper and the North Star in the upper right corner.

The Big Dipper symbolizes power, and the North Star - the north (Alaska is the northernmost territory of the United States).

Source: http://ru.wikipedia.org/wiki/Ursa Major_(constellation)