0608 GMT September 17, 2019
Though humans have named a few constellations of stars, from Orion to the Big Dipper, in reality, there are many more stars in the Universe than could ever be given names, according to livescience.com.
Just how many is not exactly clear, but it's a lot. A whole lot.
One way to get at this number is to figure out the average number of stars in a typical galaxy and multiply that by the estimated number of galaxies in the Universe.
"Deep-field images from the Hubble Space Telescope suggest there are 10 times more galaxies in the Universe than scientists previously thought, with about two trillion galaxies in total," according to a study published in October 2016 in the journal Science by Christopher Conselice, a professor of astrophysics at the University of Nottingham in the UK, and his colleagues.
"About 100 million stars inhabit the average galaxy, according to one of the best estimates," Conselice said.
But getting to that number was not just a matter of aiming a telescope at the sky and counting up all the twinkly bits. Only the most luminous stars in a galaxy shine brightly enough to be detected by a telescope.
In 2008, for instance, the Sloan Digital Sky Survey (which maps all observable celestial objectsin one third of the sky), detected about 48 million stars, or just half of the number estimated to exist, according to a 2008 study in the Astrophysical Journal.
A star as bright as our own Sun in the neighboring Andromeda galaxy would not even be detected by traditional telescopes such as those used by the Sloan Digital Sky Survey, Space.com reported.
Instead, most people estimate the number of stars in a galaxy based on galactic mass. Because the Universe is expanding and galaxies are moving farther apart, the light from other galaxies is, on average, slightly 'red-shifted', meaning its wavelength is stretched.
But because galaxies are rotating, some parts of the galaxies are actually moving closer to Earth, which means some of the light is 'blue-shifted', according to Space.com.
By using these light-based measurements, astronomers can make a rough estimate of how fast the galaxy is rotating, which in turn reveals its mass.
From there, scientists have to filter out all the dark matter, or matter that exerts a gravitational pull but reflects no light.
David Kornreich, an assistant professor at Ithaca College in New York, previously SAID, "In a typical galaxy, if you measure its mass by looking at the rotation curve, about 90 percent of that is dark matter."
Conselice said, "Multiplying the number of galaxies — which is about two trillion — by the 100 million stars in the galaxy suggests there could be about 10 raised to the19th power stars in the Universe.
"But this could easily be a factor of 10 higher."