Human biosphere and the 100 years of 1 life span as related to the size of the star at that size.
We are getting closer and closer to the point when we are over the 6 meter marker. So we are all representing the same age and the same Earth.
The question being: "What defines the age 100" as related to some Star "out there in the universe?".
The 100 years indicate the amount of motion that the whole Earth does so that this displacement fits into the size of the star Mu Cephei. Meaning that the whole Earth will move in the increasing size until it reaches the volume of that star.
the age of 100 and the size of the star that encompasses it.
by Henryk Szubinski
defining the star as the life span of one human as 100 years
as the size of some large star that has the
100 light year (human life span) / 360 as the number of the degrees rotation
light year=0.27777778
kilometer=2627980707852 km
star size 2627980707852 kilometer
Canis Majoris is one of the largest stars in our galaxy. .... a bit larger, measuring in at a staggering size of 93 billion light-years across.
radius=41857750033 km
diameter =83 715 500 066 billion km
Circumference=263 billion km.
Here's Canis Majoris size at diameter =93 billion light years.
The question being: "What defines the age 100" as related to some Star "out there in the universe?".
The 100 years indicate the amount of motion that the whole Earth does so that this displacement fits into the size of the star Mu Cephei. Meaning that the whole Earth will move in the increasing size until it reaches the volume of that star.
the age of 100 and the size of the star that encompasses it.
by Henryk Szubinski
defining the star as the life span of one human as 100 years
as the size of some large star that has the
100 light year (human life span) / 360 as the number of the degrees rotation
light year=0.27777778
kilometer=2627980707852 km
star size 2627980707852 kilometer
Canis Majoris is one of the largest stars in our galaxy. .... a bit larger, measuring in at a staggering size of 93 billion light-years across.
radius=41857750033 km
diameter =83 715 500 066 billion km
Circumference=263 billion km.
Here's Canis Majoris size at diameter =93 billion light years.
Mu Cephei as smaller than the Canis Majoris as close to the 93 billion light years diameter as about the 83.7 billion light years(shown as the red star in the center).
from
Wikipedia
date 2017
November 9
Mu Cephei (μ Cep, μ Cephei), also known as Herschel's Garnet Star, is a red supergiant star in the constellation Cepheus. It appears garnet red and is located at the edge of the IC 1396 nebula. Since 1943, the spectrum of this star has served as the M2 Ia standard by which other stars are classified.[11]
Mu Cephei is visually nearly 100,000 times brighter than the Sun, with an absolute visible magnitude of Mv = −7.6. Summing radiation at all wavelengths gives a luminosity of around 283,000 L☉ (bolometric magnitude −8.8[8]), making it one of the most luminous red supergiants in the Milky Way. It is also one of the largest stars so far discovered.
The deep red color of Mu Cephei was noted by William Herschel, who described it as "a very fine deep garnet colour, such as the periodical star ο Ceti".[12] It is thus commonly known as Herschel's "Garnet Star".[13] Mu Cephei was called Garnet sidus by Giuseppe Piazzi in his catalogue.[14] An alternative name, Erakis, used in Antonín Bečvář's star catalogue, is probably due to confusion with Mu Draconis, which was previously called al-Rāqis [arˈraːqis] in Arabic.[15]
In 1848, English astronomer John Russell Hind discovered that Mu Cephei was variable. This variability was quickly confirmed by German astronomer Friedrich Wilhelm Argelander. Almost continual records of the star's variability have been maintained since 1881.[16]
A very luminous red supergiant, Mu Cephei is likely to be the largest star visible to the naked eye, and one of the largest known. It is best seen from the northern hemisphere from August to January.
This is a runaway star with a peculiar velocity of 80.7 ± 17.7 km/s.[7] The distance to Mu Cephei is not very well known. The Hipparcos satellite was used to measure a parallax of 0.55 ± 0.20 milliarcseconds, which corresponds to an estimated distance of 1,333–2,857 parsecs. However, this value is close to the margin of error. A determination of the distance based upon a size comparison with Betelgeuse gives an estimate of 390 ± 140 parsecs,[18] so it is clear that Mu Cephei is either a much larger star than Betelgeuse or much closer (and smaller and less luminous) than expected.
The star is approximately 1,260 R☉ (880,000,000 km; 540,000,000 mi) in radius, and were it placed in the Sun's position it would reach between the orbit of Jupiter and Saturn.[8] Mu Cephei could fit around 2 billion Suns into its volume. Other estimates vary between 650 R☉[9] and 1,420 R☉[6].
The photosphere of Mu Cephei has an estimated temperature beteween 2,595 K and 3,750 K. It may be surrounded by a shell extending out to a distance at least equal to 0.33 times the star's radius with a temperature of 2,055 ± 25 K. This outer shell appears to contain molecular gases such as CO, H2O, and SiO.[18]
Infrared observations suggest the presence of a wide ring of dust and water with an inner radius about twice that of the star itself, extending to about four times the radius of the star.[9]
The star is surrounded by a spherical shell of ejected material that extends outward to an angular distance of 6″ with an expansion velocity of 10 km s−1. This indicates an age of about 2,000–3,000 years for the shell. Closer to the star, this material shows a pronounced asymmetry, which may be shaped as a torus. The star currently has a mass loss rate of a few times 10−7 M☉ per year.[19]
comparatives of the star sizes from Earth and upwards to the biggest star , Canis Majoris.
from
Wikipedia
date 2017
November 9
Mu Cephei (μ Cep, μ Cephei), also known as Herschel's Garnet Star, is a red supergiant star in the constellation Cepheus. It appears garnet red and is located at the edge of the IC 1396 nebula. Since 1943, the spectrum of this star has served as the M2 Ia standard by which other stars are classified.[11]
Mu Cephei is visually nearly 100,000 times brighter than the Sun, with an absolute visible magnitude of Mv = −7.6. Summing radiation at all wavelengths gives a luminosity of around 283,000 L☉ (bolometric magnitude −8.8[8]), making it one of the most luminous red supergiants in the Milky Way. It is also one of the largest stars so far discovered.
The deep red color of Mu Cephei was noted by William Herschel, who described it as "a very fine deep garnet colour, such as the periodical star ο Ceti".[12] It is thus commonly known as Herschel's "Garnet Star".[13] Mu Cephei was called Garnet sidus by Giuseppe Piazzi in his catalogue.[14] An alternative name, Erakis, used in Antonín Bečvář's star catalogue, is probably due to confusion with Mu Draconis, which was previously called al-Rāqis [arˈraːqis] in Arabic.[15]
In 1848, English astronomer John Russell Hind discovered that Mu Cephei was variable. This variability was quickly confirmed by German astronomer Friedrich Wilhelm Argelander. Almost continual records of the star's variability have been maintained since 1881.[16]
A very luminous red supergiant, Mu Cephei is likely to be the largest star visible to the naked eye, and one of the largest known. It is best seen from the northern hemisphere from August to January.
This is a runaway star with a peculiar velocity of 80.7 ± 17.7 km/s.[7] The distance to Mu Cephei is not very well known. The Hipparcos satellite was used to measure a parallax of 0.55 ± 0.20 milliarcseconds, which corresponds to an estimated distance of 1,333–2,857 parsecs. However, this value is close to the margin of error. A determination of the distance based upon a size comparison with Betelgeuse gives an estimate of 390 ± 140 parsecs,[18] so it is clear that Mu Cephei is either a much larger star than Betelgeuse or much closer (and smaller and less luminous) than expected.
The star is approximately 1,260 R☉ (880,000,000 km; 540,000,000 mi) in radius, and were it placed in the Sun's position it would reach between the orbit of Jupiter and Saturn.[8] Mu Cephei could fit around 2 billion Suns into its volume. Other estimates vary between 650 R☉[9] and 1,420 R☉[6].
The photosphere of Mu Cephei has an estimated temperature beteween 2,595 K and 3,750 K. It may be surrounded by a shell extending out to a distance at least equal to 0.33 times the star's radius with a temperature of 2,055 ± 25 K. This outer shell appears to contain molecular gases such as CO, H2O, and SiO.[18]
Infrared observations suggest the presence of a wide ring of dust and water with an inner radius about twice that of the star itself, extending to about four times the radius of the star.[9]
The star is surrounded by a spherical shell of ejected material that extends outward to an angular distance of 6″ with an expansion velocity of 10 km s−1. This indicates an age of about 2,000–3,000 years for the shell. Closer to the star, this material shows a pronounced asymmetry, which may be shaped as a torus. The star currently has a mass loss rate of a few times 10−7 M☉ per year.[19]
comparatives of the star sizes from Earth and upwards to the biggest star , Canis Majoris.
Mu Cephei is located in the IC 1396 Nebula.
from
Wikipedia
date 2017
NOvember 9
The Elephant's Trunk nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constellation Cepheus about 2,400 light years away from Earth.[1] The piece of the nebula shown here is the dark, dense globule IC 1396A; it is commonly called the Elephant's Trunk nebula because of its appearance at visible light wavelengths, where there is a dark patch with a bright, sinuous rim. The bright rim is the surface of the dense cloud that is being illuminated and ionized by a very bright, massive star (HD 206267) that is just to the east of IC 1396A. (In the Spitzer Space Telescope view shown, the massive star is just to the left of the edge of the image.) The entire IC 1396 region is ionized by the massive star, except for dense globules that can protect themselves from the star's harsh ultraviolet rays.
The Elephant's Trunk nebula is now thought to be a site of star formation, containing several very young (less than 100,000 yr) stars that were discovered in infrared images in 2003. Two older (but still young, a couple of million years, by the standards of stars, which live for billions of years) stars are present in a small, circular cavity in the head of the globule. Winds from these young stars may have emptied the cavity.
The combined action of the light from the massive star ionizing and compressing the rim of the cloud, and the wind from the young stars shifting gas from the center outward lead to very high compression in the Elephant's Trunk nebula. This pressure has triggered the current generation of protostars.[2][3]
from
Wikipedia
date 2017
NOvember 9
The Elephant's Trunk nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constellation Cepheus about 2,400 light years away from Earth.[1] The piece of the nebula shown here is the dark, dense globule IC 1396A; it is commonly called the Elephant's Trunk nebula because of its appearance at visible light wavelengths, where there is a dark patch with a bright, sinuous rim. The bright rim is the surface of the dense cloud that is being illuminated and ionized by a very bright, massive star (HD 206267) that is just to the east of IC 1396A. (In the Spitzer Space Telescope view shown, the massive star is just to the left of the edge of the image.) The entire IC 1396 region is ionized by the massive star, except for dense globules that can protect themselves from the star's harsh ultraviolet rays.
The Elephant's Trunk nebula is now thought to be a site of star formation, containing several very young (less than 100,000 yr) stars that were discovered in infrared images in 2003. Two older (but still young, a couple of million years, by the standards of stars, which live for billions of years) stars are present in a small, circular cavity in the head of the globule. Winds from these young stars may have emptied the cavity.
The combined action of the light from the massive star ionizing and compressing the rim of the cloud, and the wind from the young stars shifting gas from the center outward lead to very high compression in the Elephant's Trunk nebula. This pressure has triggered the current generation of protostars.[2][3]
The Elephant trunk nebula.
Important thing about Telomera, that they need space to move about in.So that the nebula openings in their centers may give the resulting matter around and the space within just as the human body has the matter around it and the space within.
Because the image 3 defines the time dilation of the" empty space planets" as the expansion of light, these planets are dark matter or dark energy because of the existance of gravity inside them or at the edges of the GAPS. This would be the types of planetary matter shells that exist in most of the universe.
continuing this theory
So space as 3 functions of ratios with 3 equals
1)singularity of space as not being made of matter and as the opposite of light=1
2)singularity of the opposite of the negative light -c of space as the density singularity=-1
3)the singularity of the opposite of negative -c light as the dark matter or dark energy=+1
The opposites of space and light, matter and density are singular values that may change
from +1 to -1 to +1 . This 3 equal ratio faze as the e.r.f (equal ration faze) makes the equation as the
-n
1)singularity of space as not being made of matter and as the opposite of light=1
2)singularity of the opposite of the negative light -c of space as the density singularity=-1
3)the singularity of the opposite of negative -c light as the dark matter or dark energy=+1
The opposites of space and light, matter and density are singular values that may change
from +1 to -1 to +1 . This 3 equal ratio faze as the e.r.f (equal ration faze) makes the equation as the
-n
at some c light function, the dilation of dark matter caught inside empty spheres as empty planets and stars may be defined as the dilation of time.
Emptyness may have 3 types as Intergalactic space, inner galactic space, space in planets and stars.
Emptyness may have 3 types as Intergalactic space, inner galactic space, space in planets and stars.
Space as the total emptiness of the universe may actually be turned against or away from the observer by the various layers that define the opposites of it as the m and c and density as time motion.