The rate of formation of new stars in the Milky Way galaxy is estimated to be about 1-2 stars per year.
To find the average rate of formation of HCl, divide the change in concentration of HCl by the time interval over which the change occurs. This will give you the average rate at which HCl is being formed.
The rate of formation of iodine can be calculated by measuring the change in concentration of iodine over time. This can be determined using the equation Rate = Δ[I2]/Δt, where Δ[I2] is the change in concentration of iodine and Δt is the change in time. This rate can be expressed in units such as M/s.
At equilibrium, the formation of products from reactants will be faster.
To calculate the initial rate, you need to know the rate law for the reaction. From there, you can plug in the initial concentrations of A and B to determine the rate constant. Without the rate law, it's not possible to calculate the initial rate.
Competitive inhibitors decrease the maximum reaction rate (Vmax) of an enzyme by competing with the substrate for the enzyme's active site, which reduces the efficiency of the enzyme-substrate complex formation and slows down the rate of the reaction.
Higher, as the increased star formation rate increases the population of massive stars that can lead to supernovae explosions. Starburst galaxies have a higher concentration of gas and dust, leading to more frequent and intense supernova events compared to a galaxy like the Milky Way.
New stars are being born all the time. The rate of star formation in the Milky Way is about 7 new stars a year.
It is estimated that on average, around 1 star is formed per year in the Milky Way galaxy. This equates to less than 0.000114 STARS/day per galaxy. However, the rate at which stars are formed can vary depending on the galactic environment.
A small galaxy with those characteristics would be a dwarf elliptical galaxy, such as M32 (a companion to Andromeda). Most elliptical galaxies are larger than average galaxies, and some are among the largest, containing as many as a trillion (1012) stars.Elliptical galaxies generally have few young stars and more dust when compared to spiral galaxies such as the Milky Way or Andromeda.
400 billion seconds. (almost thirteen thousand years) By the way there are probably no more than 200 billion stars in our galaxy...
The "baby boom galaxy" was named the "baby boom galaxy" because of the surprising amount of new stars being "born", created within it. At over 4,000 new stars per year it is the "mother" of all stellar births. In comparison, our Galaxy, the Milky Way, only one to two new stars are formed each year.
As with all space questions about speed, it all depends on your point of reference. Within the Milky Way, the orbital rate of the stars increase as you move away from the centre of the galaxy.
A Starburst Galaxy is a galaxy with an exceptionally high rate of star formation, compared to other galaxies.Galaxies usually have a burst of star formation after a collision or close encounter between two galaxies.Because of the rate of star formation and the amount of available hydrogen, starburst galaxies are presumed to be temporary.M82 (Cigar Galaxy) is a well known starburst galaxy [See related link]
Oh, look at that! Galaxies are like big families filled with stars twinkling together in the vast universe. There can be thousands to billions of stars in one galaxy, creating gorgeous and glowing views that truly inspire the imagination. Just picture yourself painting a whole galaxy filled with stars shining bright like diamonds in the sky.
The Milky Way contains somewhere around 200 billion stars. These stars account for about 20% of the visible mass of the galaxy, the other 80% being interstellar gas. However, most of the matter in our galaxy is of a form we have not yet identified, and we call it "dark matter." We don't know what it is, but we can measure its effect on the rotation rate of the stars, and we can calculate the distribution of the dark matter.
For sure. The current rate of star formation is about one a year.
Yes, relative to other celestial bodies. Indeed by observing common movement factors of these other galaxies, we may deduce the rate of movement of our home Milky Way galaxy.