The earth undergoes a number of motions. The motion around the polar
axis accounts for the length of days and nights. The motion around the sun accounts for
the length of the year. Of interest here is the rotation of earth on the polar axis. The primary contributor to the differences we see in the length of periods of daylight is the tilt in earth's axis. You have noticed that globes of the earth are virtually always set on frames with the north-south pole oriented at an angle (of about 22.4 degrees). This is not because the tilt is more visually appealing. The earth is actually tilted that way, measured against the plane that contains the earth's whole orbit. When people in the south are experiencing summer around December-March, the south pole is tilted toward the sun. In the middle of the south temperate zone, more than half of your line of latitude will be in the sun at any moment. This is because of the tilt. As the earth rotates anyone at that latitude will spend more than half the day in sunlight. At the related latitude in the north, less than half the day will be in the sun. This all cycles back and forth as the earth orbits the sun, the axis maintaining its point almost exactly in the same direction.
Because the earth is tilted at 23.5° and as it orbits the sun different parts of the earth are nearer to the sun, making it seem higher in the sky or lower in the sky. The closer you are to the the equator, the less of a difference there is in the length of the day throughout the year. By the December 21st, the northern hemisphere is tilted as far away as it can be, making the days shortest in the northern hemisphere and longest in the southern hemisphere. by June 21st, the northern hemisphere is tilted at the maximum towards the sun and the longest days are in the northern hemisphere.
No, they are not. Regarding Universal Coordinated Time (UTC), what used to be called Greenwich Mean Time, there are occasional leap seconds added to a day, meaning that even relative to UTC not all days are the same length. Of course, periods of sunlight vary according to season depending on your latitude. Even with regard to solar days, the period of time between successive transits of the sun at a given spot, days are not the same length. This is because of the earth's changing orbital velocity over the course of a year.
No, near the longest and shortest days of the year in December and June, the length of the day from day to day varies by a very small amount. Near the Equinoxes, during October or March, the length of the day from day to day varies a lot. If you plotted day length on a graph for the year, it would look like a sine wave.
Because the earth is tilted at 23.5° and as it orbits the sun different parts of the earth are nearer to the sun, making it seem higher in the sky or lower in the sky. The closer you are to the the equator, the less of a difference there is in the length of the day throughout the year. By the December 21st, the northern hemisphere is tilted as far away as it can be, making the days shortest in the northern hemisphere and longest in the southern hemisphere. by June 21st, the northern hemisphere is tilted at the maximum towards the sun and the longest days are in the northern hemisphere.
The Universe is expanding at an accelerating rate.
An updraft tower is the place in a Cumulus cloud in which an updraft goes up at a constant rate, until the dissipation process occurs or either the entire cloud, or just a part of a cloud itself.
The solar constant of Mercury varies as the intensity of the sun changes. This rate of variation is greater than on earth. However, the mean solar constant for Mercury is 9130 W/m^2 or 9.13 kW/m^2.
Hubbles Law shows that the radial velocity of a galaxy is proportional to its distance. this can be explained by the " raisin bread model", which states that a person standing on a certain raisin as the bread expands with baking ,will observe that the raisins closest to them seem to recede, and the farther the raisins are from them the faster they seem to recede, yet in reality the bread and raisins recede or move away from them at a constant rate but to the observer it seems that they move at different rates of speed. Which means that where ever you are in the solar system all of the bodies in the universe are moving away from you at a constant rate of speed.
Its very slow, despite orbiting the sun in a very quick time. it rotates once every 58.6 days relative to background stars.
There is no difference between them they are same rate constant is another name of specific rate constant
The rate constant is the reaction rate divided by the concentration terms.
The rate constant is the reaction rate divided by the concentration terms.
The rate constant is the reaction rate divided by the concentration terms.
No. Only a linear function has a constant rate of change.No. Only a linear function has a constant rate of change.No. Only a linear function has a constant rate of change.No. Only a linear function has a constant rate of change.
A relative rate constant the rate at which a reaction will take place. Ex. V = k [A][B] the constant ,k, is a constant value for the rate of the reaction in said equation.
The rate constant decreases.
It means the same rate. Its going/moving at a constant rate.
The rate constant decreases.
No. An object in free-fall accelerates at a constant rate of acceleration.Its speed grows at a constant rate.
constant rate means that rate which is fixed and can not be changed. varying rate is that rate which is not fixed and can be change easily.
You can determine if a rate of change is constant, by taking the instantaneous rate of change at multiple points - if they are all equal to each other, it can be assumed that the rate of change is constant. Alternatively, you can differentiate the function (if there is an associated function) - if this comes to a constant i.e. a number, then the rate of change is constant.