Abstract
The invisible came into astronomy in the nineteenth century when Friedrich Bessel concluded, from tiny motions of Sirius in the sky, that it is circled by a dark body. The companion of Sirius , a white dwarf star, was discovered later, in 1862, by the talented American telescope maker Alvan Clark when he tested a new half-meter size objective lens. Bessel did not live to see the discovery, but he was convinced that the universe has its dark secrets: “There is no reason to assume that brightness is an essential property of celestial bodies. Countless visible stars do not exclude numberless invisible ones.” As we have discussed earlier, the faint high-density white dwarf companion of Sirius is not totally devoid of light, but modern astronomy speaks about genuinely dark substances whose physical nature is still unknown.
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Notes
- 1.
1The mass of stars can be estimated from the total amount of light and assuming a reasonable value for the ordinary star mass emitting a given amount of light. This is roughly the same as the light output of the Sun for a mass equal to the mass of the Sun (the mass to light ratio). The total light times the ratio gives the total ordinary star mass, a great deal less than the total mass from the orbital motions.
- 2.
2In order to see plasma, hot ionized gas, just look at the candle flame, or the Sun, or those points of light of the starry sky. Stars are giant plasma balls, so most of the ordinary matter in the universe is in the form of plasma.
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Teerikorpi, P., Valtonen, M., Lehto, K., Lehto, H., Byrd, G., Chernin, A. (2019). The Dark Side of the Universe. In: The Evolving Universe and the Origin of Life. Springer, Cham. https://doi.org/10.1007/978-3-030-17921-2_25
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DOI: https://doi.org/10.1007/978-3-030-17921-2_25
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