Приклади вживання Universe's expansion Англійська мовою та їх переклад на Українською
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New method may resolve difficulty in measuring universe's expansion→.
The universe's expansion means that it was once much denser and hotter.
Studies suggest that the speed of the universe's expansion is increasing.
One of the goals of the ELT is thepossibility of making a direct measurement of the acceleration of the Universe's expansion.
In 1998, scientists discovered that the universe's expansion is accelerating.
One of the most exciting goals of the ELTis the possibility of directly measuring the acceleration of the Universe's expansion.
It was recently discovered that the universe's expansion is accelerating, not slowing, as was previously thought.
By putting all the pieces together, we then can calculate the universe's expansion rate.
The data is then used to measure the universe's expansion rate, which is also called the Hubble constant.
However, data collected from the 1990sforward has indicated that rather than slowing down, the universe's expansion is actually speeding up.
Or, there is the possibility that dark energy will cause the universe's expansion to accelerate faster and faster, evolving into a runaway process known as the Big Rip.
Observations from NASA's Hubble and ESA's Gaia telescope have givenresearchers the most precise measurements to date of the universe's expansion rate.
This data is then used to measure the universe's expansion rate, known as the Hubble constant.
Riess and his colleagues don't have any answers yet to this vexing problem,but his team will continue to work on fine-tuning the universe's expansion rate.
And at this moment in time, cosmologists believe that the Universe's expansion will outpace the more modest growth of the Hubble volume.
The calibration of these mile markers is crucially important,because there are disagreements between different methods for determining the universe's expansion rate.
This led to the astonishing discovery in the late-1990s that the universe's expansion is currently speeding up due to the repulsive effect of a mysterious“dark” energy.
Cosmologists believe that we are actually living at a time when H0 is decreasing; but because of dark energy,the velocity of the Universe's expansion is increasing.
In 1998, two independent teams of astronomers discovered that the universe's expansion was faster, consistent with the existence of a uniform contribution from Dark Energy.
In the 1930s Richard C. Tolman of the California Institute of Technology showed that thetemperature of the cosmic background would diminish because of the universe's expansion.
Riess andhis team members have been refining their measurements of the universe's expansion rate since 2005, under an initiative known as Supernova H0 for the Equation of State(SHOES).
Planck measures the size of the ripples, which shows information such as how much dark matter there is, how much normal matter there is,and the trajectory of the universe's expansion.
Cosmologists characterise the universe's expansion in a simple law known as Hubble's Law(named after Edwin Hubble- although in fact many other people preempted Hubble's discovery).
That corresponds to a possible future in which the force of gravity brings the universe's expansion to a halt- and then reverses it.
Hubble's discovery led to a clearer understanding of what dark energy is- an invisible force that opposes gravity,causing the universe's expansion to speed up.
That may sound counterintuitive,but as long as H0 decreases at a slower rate than that at which the Universe's expansion velocity is increasing, the overall movement of galaxies away from us still occurs at an accelerated pace.
The Saraswati supercluster was formed in an era when it is thought that darkenergy was just starting to accelerate the universe's expansion, making it a product of the delicate balance between dark energy and dark matter.
As a result the likelihood that thisdiscrepancy between measurements of today's expansion rate of the Universe and the expected value based on the early Universe's expansion is a fluke is just 1 in 100,000, a significant improvement from a previous estimate last year of 1 in 3,000.
This expansion of the universe, with nearby galaxies moving away more slowly than distant galaxies, is what one expects for a uniformly expanding cosmos with dark energy(an invisible force that causes the universe's expansion to accelerate) and dark matter(an unknown and invisible form of matter that is five times more common than normal matter).