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Let's start by discussing something that humans may not fully understand.
For example, let's talk about "Orion Constellation."
This topic is all about space: facts, our dreams, and our experiences.
Orion Constellation

IC 434 Nebula - Horsehead Nebula
The famous dark nebula, "Horsehead" (official designation Barnard 33), was first discovered over a hundred years ago – in 1888 on a photographic plate obtained at the Harvard University Observatory (USA). Its remarkably expressive shape has made it one of the most famous astronomical objects.
The bright pink glow of the hydrogen cloud, against which the dark outlines of the Horsehead Nebula stand out, is caused by the ultraviolet radiation of Sigma Orionis, a young, bright O-type star. A map of the polarization of the cloud's glow indicates that Sigma Orionis is the only source of hot radiation illuminating this area (the bright star Zeta Orionis, located nearby, is closer to us than the cloud and is therefore not related to it). The presence of a single powerful source of radiation makes the Horsehead Nebula an excellent, unique laboratory for testing existing models of photodissociation processes, which describe the interaction of gas and dust immersed in a "sea" of ultraviolet quanta.
IC 434 or the Horsehead Nebula in the Orion Constellation

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M42 Nebula (NGC 1976) - Great Orion Nebula
Below Orion's Belt, you can find the bright gas and dust nebula M42 (NGC 1976) - the Great Orion Nebula, with an integrated magnitude of 4.0m. With the naked eye, the nebula appears as an inconspicuous small spot, resembling a comet. In a telescope, however, the nebula appears in all its glory. In the center of the nebula, you can see four hot stars - the Orion Trapezium. Around the Orion Trapezium is an area of active star formation, which consists of an extremely dense young star cluster and T Tauri-type variables. Nearby are dense molecular clouds, which are the closest giant molecular clouds to the Sun: Orion A and Orion B, located 400-500 pc away.
The nebula is located at a distance of 1500 light-years from Earth, and the reddish color in the photograph is explained by the strong glow at the wavelength of hydrogen, which makes up the main mass of the gas in the Great Orion Nebula.

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M43 (NGC 1982) - De Mairan Nebula in the Orion Constellation
M43 is a diffuse nebula (NGC 1982) that reflects and scatters light. It is now considered part of the Orion Nebula, being separated from M42 by a strip of dark dust. It was first described by de Mairan in 1733 and was long known by his name.
The stars NU Orionis (HD 37061), with a magnitude of 6.5m-7.6m and a spectral class of B4, are immersed in M43. Most likely, M43 glows due to these stars, which formed in this part of the Orion Nebula. The nebula shines with reflected light, as the energy of the radiation from nearby stars is not enough to cause emission radiation. In addition to the usual gases for nebulae (hydrogen and helium), the M43 nebula contains oxygen and even some molecular compounds, including organic ones.

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Flame Nebula (NGC 2024) in the Orion Constellation

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Large Magellanic Cloud

Large Magellanic Cloud
In long-exposure images, the LMC begins to resemble a spiral galaxy with a bar. The Large Magellanic Cloud is located at a distance of only 180 thousand light-years in the constellation Dorado, and its size is about 15 thousand light-years. SN1987A, the brightest and closest of all supernovae of our time, erupted in the LMC.
Together with the Small Magellanic Cloud (SMC), the LMC can be seen from the southern hemisphere with the naked eye.
Source - astronet.ru
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Supernova Outburst Threatens Earth with Powerful Gamma-Ray Burst
Astronomer Peter Tuthill from the University of Sydney has discovered that a supernova may erupt in the relatively near future in the binary system WR 104, which will lead to a powerful gamma-ray burst directed straight at Earth, Fox News reports, citing an article in The Astrophysical Journal.
WR 104 is located only eight thousand light-years from Earth (approximately towards the center of the Galaxy). One of the stars in it belongs to the Wolf-Rayet class (in particular, it has a very high temperature and luminosity) and, according to Tuthill's data, is likely nearing the end of its life. At the end of the life of such a star, a supernova eruption occurs.
A Wolf-Rayet supernova eruption could destroy life on Earth

During a supernova eruption of this type, the core of the star collapses into a black hole, and the shell is ejected into space. The complex interaction of fields and matter around the hole often leads to the formation of a gamma-ray burst: the release of two beams of very high energy directed in opposite directions into space. Such bursts have been observed repeatedly.
Being directly in the path of a beam generated at such a small distance is dangerous for life on Earth: gamma rays can, for example, destroy the ozone layer that protects us, and subatomic particles will create potentially dangerous cascades of particles in the atmosphere. Tuthill's calculations show that such a probability exists. However, it is unclear how high it is, especially since there may still be hundreds of thousands of years before the supernova explosion.
Source - internet
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So, what do you think? When will we fly to Mars?
Let's start by discussing something that humans may not fully understand.
For example, let's talk about "Orion Constellation."
This topic is all about space: facts, our dreams, and our experiences.
Orion Constellation

IC 434 Nebula - Horsehead Nebula
The famous dark nebula, "Horsehead" (official designation Barnard 33), was first discovered over a hundred years ago – in 1888 on a photographic plate obtained at the Harvard University Observatory (USA). Its remarkably expressive shape has made it one of the most famous astronomical objects.
The bright pink glow of the hydrogen cloud, against which the dark outlines of the Horsehead Nebula stand out, is caused by the ultraviolet radiation of Sigma Orionis, a young, bright O-type star. A map of the polarization of the cloud's glow indicates that Sigma Orionis is the only source of hot radiation illuminating this area (the bright star Zeta Orionis, located nearby, is closer to us than the cloud and is therefore not related to it). The presence of a single powerful source of radiation makes the Horsehead Nebula an excellent, unique laboratory for testing existing models of photodissociation processes, which describe the interaction of gas and dust immersed in a "sea" of ultraviolet quanta.
IC 434 or the Horsehead Nebula in the Orion Constellation

*******************************************
M42 Nebula (NGC 1976) - Great Orion Nebula
Below Orion's Belt, you can find the bright gas and dust nebula M42 (NGC 1976) - the Great Orion Nebula, with an integrated magnitude of 4.0m. With the naked eye, the nebula appears as an inconspicuous small spot, resembling a comet. In a telescope, however, the nebula appears in all its glory. In the center of the nebula, you can see four hot stars - the Orion Trapezium. Around the Orion Trapezium is an area of active star formation, which consists of an extremely dense young star cluster and T Tauri-type variables. Nearby are dense molecular clouds, which are the closest giant molecular clouds to the Sun: Orion A and Orion B, located 400-500 pc away.
The nebula is located at a distance of 1500 light-years from Earth, and the reddish color in the photograph is explained by the strong glow at the wavelength of hydrogen, which makes up the main mass of the gas in the Great Orion Nebula.

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M43 (NGC 1982) - De Mairan Nebula in the Orion Constellation
M43 is a diffuse nebula (NGC 1982) that reflects and scatters light. It is now considered part of the Orion Nebula, being separated from M42 by a strip of dark dust. It was first described by de Mairan in 1733 and was long known by his name.
The stars NU Orionis (HD 37061), with a magnitude of 6.5m-7.6m and a spectral class of B4, are immersed in M43. Most likely, M43 glows due to these stars, which formed in this part of the Orion Nebula. The nebula shines with reflected light, as the energy of the radiation from nearby stars is not enough to cause emission radiation. In addition to the usual gases for nebulae (hydrogen and helium), the M43 nebula contains oxygen and even some molecular compounds, including organic ones.

*********************************************
Flame Nebula (NGC 2024) in the Orion Constellation

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Large Magellanic Cloud

Large Magellanic Cloud
In long-exposure images, the LMC begins to resemble a spiral galaxy with a bar. The Large Magellanic Cloud is located at a distance of only 180 thousand light-years in the constellation Dorado, and its size is about 15 thousand light-years. SN1987A, the brightest and closest of all supernovae of our time, erupted in the LMC.
Together with the Small Magellanic Cloud (SMC), the LMC can be seen from the southern hemisphere with the naked eye.
Source - astronet.ru
************************************************
Supernova Outburst Threatens Earth with Powerful Gamma-Ray Burst
Astronomer Peter Tuthill from the University of Sydney has discovered that a supernova may erupt in the relatively near future in the binary system WR 104, which will lead to a powerful gamma-ray burst directed straight at Earth, Fox News reports, citing an article in The Astrophysical Journal.
WR 104 is located only eight thousand light-years from Earth (approximately towards the center of the Galaxy). One of the stars in it belongs to the Wolf-Rayet class (in particular, it has a very high temperature and luminosity) and, according to Tuthill's data, is likely nearing the end of its life. At the end of the life of such a star, a supernova eruption occurs.
A Wolf-Rayet supernova eruption could destroy life on Earth

During a supernova eruption of this type, the core of the star collapses into a black hole, and the shell is ejected into space. The complex interaction of fields and matter around the hole often leads to the formation of a gamma-ray burst: the release of two beams of very high energy directed in opposite directions into space. Such bursts have been observed repeatedly.
Being directly in the path of a beam generated at such a small distance is dangerous for life on Earth: gamma rays can, for example, destroy the ozone layer that protects us, and subatomic particles will create potentially dangerous cascades of particles in the atmosphere. Tuthill's calculations show that such a probability exists. However, it is unclear how high it is, especially since there may still be hundreds of thousands of years before the supernova explosion.
Source - internet
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So, what do you think? When will we fly to Mars?
