Ichi-ryu karate competitions were held for the first time in Serpukhov. The organizer was the Moscow Regional Karate Federation, and the gym was kindly provided by school No. 12. Since the opening of the educational institution, the director of the school, Elena Akimova, has paid special attention to the development and support of sports in general, for which many coaches and parents of young athletes are grateful to her.
The Regional Karate Federation in Serpukhov was formed quite recently - in the fall of 2011. The founders were Vladimir Balashov, Alexei Gerasimov, Mikhail Ivanov. All of them have been in the sport for a long time. Honored Coach of Russia Safronov Vitaly Anatolyevich is the first teacher of this trio of coaches. He is also the ideological inspirer of an undertaking called "ichi-ryu". "Ichi" in translation means "first, best", it can also be translated as "the spirit of victory, regardless of the type of weapon", and "ryu" - school. The leaders of the federation themselves tried themselves in different types of martial arts, but still settled on karate. They grew both on their own and on the example of the world-famous "sensei" Masao Kawazoe (the teacher is the chief technical instructor of the Traditional Karate Federation of Russia, shihan of the Japan Traditional Karate Institute (JTKI) and Masayuki Hisataka ("sensei", holder of 8 and 9 dans, president of the World Federation "Koshiki-karate") "Ichi-ryu" in one of the translations means "school", and the grand master Ali Chan, who was present at the competitions as part of a delegation from China, translated the hieroglyph as "the best karate".
About 70 young athletes from 6 to 17 years old took part in the competition: from white to black belts. These are guys from 6 city clubs - the 1st gymnasium, the 12th school, the fitness club "Strength + Beauty", ICC "Yunost", SC "Typhoon". There were fighters engaged in traditional karate, koshiki-karate, directly Ichi-ryu, hand-to-hand combat.
The Ichi-ryu rules developed by us are universal, - says Alexei Gerasimov, vice-president of the regional karate federation, - they are created on the basis of different types of martial arts that we ourselves studied - karate, taekwondo, judo, boybo. We choose the best of the best. At the same time, the main traditions of karate, such as, for example, "the first clear blow - on the spot", are observed - after all, all the techniques of traditional karate come down to this. The style is contact, so it is impossible to hold back the onslaught of an opponent in one kimono. The use of protective equipment is mandatory.
Competitions were held in two traditional disciplines, - says the president of the federation Vladimir Balashov, - these are kata (formal exercises) and kumite. In the first case, the guys demonstrated the degree of assimilation of the technique of attack and defense, as well as the movement of the body: the enemy exists only in the imagination. Well, kumite is the practical use of the basic techniques learned in kata. The guys competed until late in the evening. Each of them went out on the tatami more than once, but there was no noticeable fatigue. Our boys and girls were so good in fights and kata that it is difficult to single out anyone without fear of offending the others. Everyone is just great, especially the girls. So, there is someone with whom to develop a new direction in karate, there is someone to prepare for competitions of a higher level.
Winners of the First Open Ichi-Ryu Karate Tournament
Discipline in kata
category 6-7 years
1. Nikolay Menshaev
2. Fatyanov Dmitry
3. Makarov Gleb
category 8-9 years
1.Osmanov Timur
2. Oleg Kulikov
3. Pozdnyakov Maxim
girl category
8-9 years old
1.Redkina Masha
2.Puzankova Alexandra
3. Vasilevich Alina
category 10-11 years old
1.Eremin Nikita
2. Zylikov Danila
3. Fedechkin Nikolay
category 12-13 years old
1. Pitelin Ilya
2. Pawlak Egor
3. Glotov Sasha
Discipline in KUMITE
category 6-7 years
1. Kryuchkov Ivan
2. Makarov Gleb
3. Ponomarev Vlad
category 8-9 years
1. Kostin Danila
2. Akhmetov Tamerlane
3. Pavel Kopeikin
category 10-11 years old
1. Danila Zylikov
2. Eremin Nikita
3. Tyuriakov Ivan
category 12-13 years old
1. Pitelin Ilya
2. Glotov Sasha
3.Pavlyak Egor
category 14-15 years old
1. Afanasiev Igor
2. Andrey Galkin
3. Andrey Barnov
category 16-17 years old
1.Makarov Dmitry
2. Odinokov Alexander
3. Grandfather Philip
Since ancient times, warriors carried two swords with them. Previously, they were simply called: "long sword" - or katana, and "sword" - wakizashi. Now they are called somewhat differently: "sword" and "short sword". Without going into the reasons, I will only say that according to tradition in our country, a warrior always wears two swords on his belt. The spear and halberd are only worn outdoors. Such is the Way. This has certain advantages. Therefore, at the Nito Ichi Ryu school, they learn to wield two swords.
Strategy students at Ichi School always practice with both swords in hand. The meaning of this approach lies in the fact that if a warrior is ready to give his life at any moment in battle, then he must use his combat potential to the maximum. In this case, to do otherwise and die with an undrawn weapon is simply unwise.
The position with one long sword in both hands carries with it a certain stiffness that prevents it from being freely and easily moved to the right and left. It is all the more inconvenient to hold the sword with both hands if you are sitting in the saddle, running on stony or swampy soil, when you have to defend yourself from attacks from different sides. A long sword in both hands does not allow any other weapon to be used. It is much more convenient to wield a sword if you hold it in one hand, this is my method - in each hand a sword. This method is not suitable for halberds and spears. They are too long and heavy. But the sword and companion sword are quite comfortable to hold with one hand. And if you are fighting in a crowd or want to capture a prisoner, then this position will be the only correct one. Thus, the sword should be held in both hands only in those cases when it is necessary to strike especially powerful blows. The goal of a warrior on the path of strategy is to become fluent in the use of two long swords. Without the habit of this kind of exercise, it seems too difficult, exactly.
but just as difficult for the first time to draw a bow or turn a halberd. But in the process of training, your will will become stronger, you will gain the power of the Way and will be able to easily wield them.
In The Book of Water, I will explain how the technique of wielding long and short swords differs. The long sword moves in a wide arc, it is difficult for them to make short and fast movements, but it is easy to attack from a long distance. A short sword - on the contrary, is intended for close combat. This must be well understood.
In the Strategy of the Ichi school, it is believed that the ability to win is determined by the state of the spirit of a warrior, and not by the length of his weapon. If you have the spirit of victory, you will not depend on the type of weapon and will be able to win, fighting with both long and short blades. In other words, the spirit of the Ichi school is the spirit of victory.
The book cannot explain everything. Theory without practice is dead. By practicing, you will know ten thousand things. Studying with full devotion, you will comprehend the Way of Strategy, and then nothing will remain hidden for you.
The constellation Sails is geographically located in the southern hemisphere of the starry sky.
The closest neighbors of the constellation Sail are Pump, Korma, Compass, Centaurus, and also Carina. The area occupied by the considered constellation in the sky is 499.6 square degrees. Of the entire abundance of stars in the Sails, an observer can distinguish about 195 from the Earth without the use of additional optical devices.
The constellation Sails, as seen in the Stellarium planetarium program
On the territory of Russia, this constellation is difficult to observe. Part of it can be seen only in the southern regions of the country, and the further south the observer, the more likely it is to consider the constellation. The best conditions for contemplating at least some of the components of this constellation come in February.
Astronaut's lucky joke gives name to star
Speaking about the stars of the constellation Sails, it is worth starting with the brightest - the star Gamma. Other names for this luminary are Suhail (Suhail al Mulif) and Regor (sometimes "Roger" due to the humor of the astronaut aboard Apollo 1). Often the star is called the Illusory Pearl of the Southern Sky. The long and mysterious name is explained by radiation instead of dark and absorbing rays of incredibly bright, due to which the spectrum of the star Gamma is very exotic.
Remote from us at 800 St. years, this star of the second magnitude is a multiple system, which includes at least six components. The brightest among all is considered to be Gamma-2 Sails, which in itself is also, and includes an O9 class supergiant and a Wolf-Rayet type star. The last star is special in that it is recognized as the heaviest among those ever found to date. Secondary after Gamma-2, it is supposed to consider the Gamma-1 component - a white-blue subgiant of the fourth magnitude of class B. The Regor star system has several more faint stars that have only 8, 9 and 13th magnitudes.
Another multi-star system of Sails
It turns out that the Delta star is not far from Gamma Sails in terms of the number of components. Delta Sails is the second brightest in the constellation and is another multiple system in its composition. Unfortunately, the star does not have any common name. It is 80 light years away from Earth.
The composite star system contains two binary stars. The first visual binary star is represented by the components Delta Sails A and B. The luminary Delta A is located on the main sequence and appears to be a white dwarf of the second magnitude. Component A's companion, Delta B, is a fifth-magnitude yellow dwarf.
At 69 arc seconds from this system, there is another, much dimmer system. It is represented by Delta C and Delta D - stars of the eleventh and thirteenth magnitudes, respectively. The distance between these two components is 6 arc seconds. It is worth noting that the Delta Sails star system is the brightest among all eclipsing-variable luminaries in the sky. And after some 7,000 years, she is predicted to play the role of the South Pole Star as a result of the precession of the earth's axis.
Objects of deep and distant space
First of all, it is worth saying a few words about the False Cross asterism as part of the constellation under consideration, which is formed by its stars Delta, Kappa, Yot and Epsilon of the Carina constellation. Asterism got its name for its resemblance to the constellation. However, unlike the latter, the specified asterism is not an indicator of the South Pole of the world. This erroneous judgment previously often led to a variety of navigational errors.
Here in Sails, at a distance of 2 thousand St. years from us, the planetary nebula of the Eight Flares or the South Rim is located. In the center of the nebula is a rather hot color that illuminates the entire nebula with ultraviolet rays.
There is also a Gama Nebula in the constellation, which is considered to be a remnant that occurred about 11-12 thousand years ago. The nebula is also called Gam 12. It extends to the constellation Puppis and is an emission nebula.
Story
To this day, many consider Sails to be part of another larger constellation called the Argo Ship, known to all thanks to ancient Greek mythology. However, back in 1752, Lacaille proposed dividing such a large constellation into smaller ones, thanks to which three new constellations appeared in the sky. In addition to, in fact, Sails, constellations were also formed under the names Korma and Kiel. However, the names of the stellar components have not changed, so there are no stars in the Sails marked with alpha or beta - these stars have retained the names assigned during their stay in the constellation Ship Argo.
| List of constellations in the spring sky | |
|---|---|
> Sails
| An object | Designation | Meaning of the name | Object type | magnitude |
| 1 | Gamma Sails | "Main Star of the Oath" | multiple star | 1.83 |
| 2 | Delta Sails | "Beam and Arrow" | triple star | 1.99 |
| 3 | Lambda Sails | "Smooth Plain" | Orange supergiant | 2.21 |
| 4 | Kappa Sails | "Ride" | double star | 2.48 |
| 5 | Mu Sails | Not | double star | 2.69 |
| 6 | Phi Sails | "Star Map" | Blue-white supergiant | 3.52 |
| 7 | Psi Sails | Not | double star | 3.60 |
Story constellation Sails in the southern hemisphere: part of the Argo Ship, description with photo, diagram, star map, myth and legend, facts, bright stars, asterism.
Sails - constellation, which is located in the southern sky and from Latin "Vela" is translated as "Sails".
It was once part of the larger constellation Argo Ship, which is the ship of the Argonauts. It was first recorded by Ptolemy in the second century. And in the 1750s, Nicolas Louis de Lacaille divided it into three: Sails, Keel and Stern.
The constellation Sails contains several notable objects: the Eight Flare Nebula (NGC 3132), the Gum Nebula, the Sails supernova remnant, the Pencil Nebula (NGC 2736) and the Sails omicron cluster (IC 2391).
Facts, position and map of the constellation Sails
| Sail | |
|---|---|
| Lat. title | Vela |
| Reduction | Vel |
| Symbol | Sail |
| right ascension | from 8 h 00 m to 11 h 00 m |
| declination | -56° 30' to -36° 45' |
| Square | 500 sq. degrees (32nd place) |
| brightest stars (value< 3 m ) |
|
| meteor showers |
|
| neighboring constellations |
|
| The constellation is visible at latitudes from +34° to −90°. The best time for observation is February. |
|
Contains 5 stars with planets and no Messier objects. The brightest star is Gamma Parus, whose apparent visual magnitude reaches 1.75. There are three meteor showers: Delta Velida, Gamma Velida and Puppida Velida. Included in the Heavenly Waters group along with, and. Consider the scheme of the constellation Sails on the map of the starry sky.
The myth of the constellation Sails
The constellation depicts part of the Argo Ship, on which Jason and the Argonauts sailed from Iolkos to obtain the Golden Fleece. It was created by Argus, who used the help of Athena. When the expedition ended, they dedicated the ship to Poseidon, who placed it in the sky.
In 1752, Nicolas Louis de Lacaille divided the giant constellation into three smaller ones: Sails, Carinae and Korma. He used one set of Greek letters for all the constellations, so the Sails are devoid of Alpha and Beta (departed to Carina).
The main stars of the constellation Sails
Explore carefully the bright stars of the constellation Sails of the southern hemisphere with a detailed description and characteristics.
Suhail(Gamma Sails) is a multiple star system (6 stars) with an apparent magnitude of 1.7 and a distance of 336 light years.
The main object (A) is a spectroscopic binary consisting of a blue supergiant (O7.5) and a massive Wolf-Rayet star (developed, extremely hot, massive, rapidly losing mass due to a powerful stellar wind). The Wolf-Rayet star is one of the closest supernova candidates and is likely to end in a Type Ic supernova explosion. The orbital period is 78.5 days, and the distance between them is 1 AU.
The closest satellite to them (B) is a blue-white subgiant (B). Other objects include C (a white star of visual magnitude 8.5) and a binary star composed of D and E.
D is a class A white star with an apparent magnitude of 9.4, and E is a 13th magnitude star.
Delta Sails is a multiple star system with an apparent visual magnitude of 1.96 and a distance of 80.6 light years. It is located near the border with the constellation Carina.
Represented by stars A and B, whose orbital period is 142 years. Visual magnitude A is 1.97 and B is 5.55. The primary component is a spectroscopic binary with a rotation period of 45.15 days. It is the brightest eclipsing star system. Both evolved away from the main sequence. Age - 400 million years.
At 69 arc seconds, there is another binary system, represented by stars of the 11th and 13th magnitude, divided by 6 arc seconds.
The star is also called Ku-She, which means "bow and arrow" in Chinese.
Lambda Sails- an orange star between a giant and a supergiant (K4.5Ib-II) with an apparent visual magnitude of 2.21 and a distance of 545 light years. It is a slow irregular LC type variable star whose brightness ranges from 2.14 to 2.30.
It is 8.5 times more massive than the Sun, 207 times larger in radius, and 10,000 times brighter. Age - 32 million years. Also called Suhail (like Gamma Sails). In China, it is known as pinyin - "the judge for judging the age of animals."
Kappa Sails is a spectroscopic binary star located 572 light years away. The visual magnitude is 2.48. The combined stellar classification is B2 IV, making it a blue-white subgiant. The orbital period is 116.65 days.
Mu Sails- a double star located 117 light years away. Objects are separated by 1.437 arcseconds and have an orbital period of 116.24 years. The total apparent visual magnitude is 2.69, and individual stars are 2.7 and 6.4.
The brighter object is a yellow giant (G5 III), which is 3.3 times as massive, 13 times larger in radius, and 107 times brighter. The companion is a yellow dwarf (G2V) of the main sequence.
HD 82668- an orange giant (K5 III) with an apparent magnitude of 3.16 and a distance of 239 light years. Located between Sails and Kiel. Twice as massive as the Sun and 29 times larger in radius.
Phi Sails- a blue-white supergiant (B5 Ib) with an apparent visual magnitude of 3.52 and a distance of 1590 light years. The traditional name Tsei Ke means "heaven's record" in Chinese.
Omicron Sails- a blue-white subgiant (B3 IV) with an apparent visual magnitude of 3.60 and a distance of 490 light years to us. It is 5.5 times more massive than the Sun, 4.3 times larger in radius, and 1000 times brighter. It is a variable star whose luminosity ranges from 3.55 to 3.67 over 2.78 days.
Psi Sails- a binary star with an apparent magnitude of 3.60 and a distance of 60.5 light years. Among the stars of the constellation, this is the closest one to our planet.
It is represented by a yellow-white subgiant (F3IV) with a visual magnitude of 4.1 and a yellow-white dwarf (F0V), whose apparent magnitude reaches 4.6. Divided by 0.68 arcseconds, and the orbital period is 33.99 years.
WISE 1049-5319- a binary system of brown dwarfs, distant 6.6 light years from the Sun (closest to our system). It was the closest to the Sun before the discovery of Barnard's Star (Ophiucus).
The main component has a stellar classification of L8 ± 1. The orbital period is 25 years, and the distance is 3 AU.
HD 78004 is an orange giant (K2III) with an apparent visual magnitude of 3.75 and an absolute magnitude of -1.14. Located at 309 light years.
HD 74180 is a binary star (F3Ia), whose visual magnitude reaches 3.77. It is located 3,100 light years from us. The main object is a yellow-white supergiant (irregular variable) with variations in brightness from magnitude 3.77 to 3.91. The companion is a star of 10th magnitude, separated by 37.5 arc seconds.
HD 92139 is a triple star system 86.5 light-years distant from Earth. The total apparent magnitude is 3.84. The main component is a yellow-white subgiant (F3IV) with an apparent magnitude of 4.5. It is a spectroscopic binary with two objects orbiting in 10.21 days.
The third star is a main sequence white dwarf (A6V) with a visual magnitude of 5.1 and a distance of 0.3 arcseconds. It completes a revolution around the pair in 16.3 years.
HD 75063- a white giant (A1III) with a visual magnitude of 3.87 and a distance of 1550 light years. The absolute value is -4.54.
HD 73526 is a main sequence yellow dwarf (G6V) with an apparent visual magnitude of 9.00 and a distance of 310 light years. Reaches the solar mass, 1.49 times larger in radius and 1.77 times brighter.
Two planets revolve around it. The first one was found in 2002 with an orbital period of 187.5 days, and the second one was found in 2006 with an orbital period of 376.9 days. The planets form a 2:1 resonance. HD 73526 b is 2.07 times the mass of Jupiter, and HD 73526 c is 2.30 times.
WASP-19 is a main sequence yellow dwarf (G8V) with an apparent magnitude of 12.3 and a distance of 815 light years.
In 2009, a hot Jupiter, WASP-19 b, was found, with the shortest orbital period of 0.78884 days.
V390 Sails is an old, massive red giant (F3e). The star evolved from a red giant and began to shed layers, forming a dust disk. Eventually, it will create a planetary nebula. It is located 2600 light years away and has a visual magnitude of 10.48. 5000 times brighter than the Sun. This is a variable of type RV Taurus. A satellite revolves around it with a frequency of 499 days.
Asterism
false cross is an asterism created by the stars Delta Sails, Kappa Sails, Iota Carinae, and Epsilon Carinae. It is called "false" because it is often confused with the Southern Cross (used in navigation to find the south).
Celestial objects of the constellation Sails
Eight Flare Nebula(NGC 3132, Caldwell 74) is a bright planetary nebula spanning half a light year in diameter. The apparent visual magnitude is 9.87, and the distance is 2000 light years.
It got its name because, when observed through amateur telescopes, it resembles a figure eight. It contains two stars: a star of the 10th magnitude and a white dwarf of the 16th magnitude, blowing away the outer layers. It is the ultraviolet radiation from the second object that causes the nebula to glow.
(Gum 16) is a supernova remnant with an apparent visual magnitude of 12 and a distance of 815 light years. Occupies 8 degrees in diameter. The precursor star is believed to have exploded 11,000-12,300 years ago.
The remnant includes the Pencil Nebula (NGC 2736) and is associated with the Vela pulsar. It is also 4 times larger than the supernova remnant in Korma and overlaps it. Both are among the brightest and largest X-ray objects.
In 1998, another supernova was discovered in the direction of the Sails remnant - RX J0852.0-4622, 650 light-years distant from us.
Pulsar in Sails(PSR B0833-45) is a pulsar associated with a supernova remnant. It is located 959 light years away and has an apparent magnitude of 23.6. It is a source of radio, optical, gamma and X-ray radiation.
An association formed by astronomers at the University of Sydney in 1968 testified that supernovae form neutron stars.
Nebula Pencil(NGC 2736) is a nebula located near the Pulsar in Sails. It is 815 light years away from us. The apparent magnitude is 12. It is believed that it was formed from part of the shock wave of the supernova remnant.
(Gum 12) is an emission nebula spanning 40 degrees in the Sails and Stern. Located 400 parsecs from us. It contains the remnants of the Sails supernova and is thought to be a greatly expanded supernova remnant that exploded a million years ago.
In the 1950s, it was discovered by Australian astronomer Colin Gum.
Gum 19 A star-forming region located 22,000 light years away. It is illuminated by the large, bright blue supergiant V391 Parusov. Surface temperature - 30000 °C.
NGC 2670- an open cluster with an apparent visual magnitude of 7.8 and a distance of 3200 light years. Contains 50 moderately bright stars.
NGC 2899 is a planetary nebula located 6500 light years away. John Herschel found her in 1835.
NGC 2547 is an open cluster located 1500 light years away and has a visual magnitude of 4.7. The age of the stars is 20-35 million years.
It was discovered in 1751 by Nicolas Louis de Lacaille.
(Caldwell 79) is a globular cluster with a visual magnitude of 8.24 and a distance of 16,300 light years. Age - 10.24 billion years. It contains mostly old stars dominated by red giants. The radius covers 40 light years.
HH 47(Herbig-Haro 47) – Herbig-Haro object. It is a patch of nebula formed after a young star ejected narrow jets of gas that collided with nearby gas and dust clouds. Located 1500 light years away.
Sails omicron cluster(IC 2391, Caldwell 85) is a young open cluster located 500 light years away. Apparent magnitude - 2.5 (can be seen without the use of technology). It contains 30 stars and extends over 50 arc minutes.
You have the opportunity to study the constellation Sails of the southern hemisphere more closely if you use not only our photos, but 3D models and an online telescope. For independent search, a star map is suitable.
The sails are part of the ancient constellation Ship Argo. The southern part of the constellation is located in the most star-filled regions of the Milky Way. Up to hundreds of stars can be seen in a constellation with the naked eye. After the division of the Ship Argo into three constellations at the initiative of Lacaille in 1752, there were no alpha and beta stars in the Sails. Therefore, gamma (Regor), delta, lambda (Al Suhail) became the brightest.
On the border of Sails and Carina is the asterism False Cross, which is often mistaken for the constellation of the Southern Cross. Unlike the real one, the false cross is not directed to the south pole of the world. The double star Gamma Sails is clearly visible through binoculars. Its components, which have magnitudes 2 and 4, are separated by a distance of 40 arcseconds. In this case, the main component of the pair is itself a close binary system in which two stars are adjacent. One of them is a Wolf-Rayet type star. The masses of the stars are respectively 38 and 20 solar masses. The orbital period of the pair is 78.5 days.
The smaller star is losing matter from its surface at a high rate. For the first time stars of this type were described in 1867 by French astronomers Charles Wolf (1827-1918) and Georges Rayet (1839-1906). The spectrum of this star shows broad multi-colored lines against a fairly bright continuous background. Astronomers call this star the “spectral pearl of the southern sky.”
The planetary nebula NGC 3132, located on the border with the Pump, is similar to the Ring Nebula in Lyra. However, it is noticeably brighter, and much brighter than its central star, which can be easily seen in a small telescope. The glow of the nebula itself is excited by its small companion with a surface temperature of about 100,000°K.
In Sails there is one of the most unusual objects of optical astronomy - the neutron star-pulsar Vela, blinking at a frequency of 11 pulses per second. This is the second optical pulsar, discovered in 1977, 10 years after the first one discovered in the Crab Nebula (the constellation of Taurus). Both of them are also radio pulsars, radiating radio waves into outer space. Vela was formed as a result of a supernova explosion that occurred in Parus about 12,000 years ago. He left behind a rapidly rotating neutron star with a gas envelope flying in all directions from it. Its diameter today has already reached 6 degrees. This very beautiful openwork structure lies on the galactic equator, between the stars Gamma and Lambda Sails.
Looking for a constellation in the sky
The constellation is visible at latitudes from -90° to +34°. The constellation Sails lies far south of the celestial equator and therefore is not observed on the territory of Russia. Neighboring constellations: Pump, Compass, Korma, Carina, Centaurus.
In autumn, Sails are on the southeast side of the horizon. At midnight, the constellation is still partly invisible. Above the sails is Korma with its bright star Canopus, which helps to find the constellation in the sky. To the right of the Sails, the Southern Cross rises from the horizon.
In winter, the Sails rise high into the sky and are visible all night on the southeast side of the sky. They are followed by the conspicuous Southern Cross and the Centaurus, easily identified by its two bright stars. Canopus (alpha Kipya) is located to the right and above the Sails.
In the summer at midnight, the Sails set beyond the horizon a little to the right of the south point. Above them, a part of the setting Kiel is also visible. Bright Canopus has already disappeared over the horizon. The main reference point here will be the Southern Cross, which is located above the Sails.
