About 5 billion years. However, long before that - somewhere around 500 million to 1 billion years from now - the Sun is expected to become so hot that no life can survive on Earth - unless we do something about it, of course.
Basically, the stars on the "Main Sequence" are the ones that fuse hydrogen-1 into helium-4. Once a star burns up its hydrogen-1 fuel, or doesn't have much left, it will start burning helium-4 into heavier elements. It is then that the star leaves the "Main Sequence".
The main factor is its mass.
It depends on the mass of the star. The lower the mass, the longer it will stay on the main sequence. A red dwarf may stay on the main sequence for trillions of years, while a blue star only lasts a few million years.
mRNA becomes associated with ribosomes in the cytoplasm. Ribosomes are the cellular structures where mRNA is used as a template for protein synthesis. This association allows for translation, the process of converting the mRNA sequence into a protein.
Yes, it is quite common for snowball bushes to bloom flowers before their leaves appear. The flower buds usually form before the leaves, and once the flowers have bloomed, the leaves will start to grow. It's a natural cycle for many plants, especially those that are deciduous.
A red main sequence star would be a red dwarf or a branch red giant. To be on the main sequence, you have to have hydrogen nuclear fusion.
Hydrogen fusion to make helium. When a star runs out of hydrogen in its core to fuse, it begins collapsing, leaves the main sequence, then ignites helium fusion to make carbon, becoming a red giant.
Basically, the stars on the "Main Sequence" are the ones that fuse hydrogen-1 into helium-4. Once a star burns up its hydrogen-1 fuel, or doesn't have much left, it will start burning helium-4 into heavier elements. It is then that the star leaves the "Main Sequence".
The Sun is currently on the main sequence, and will stay on it for about another 4.5 billion years. Our sun is currently 4.5 billion years old, which is considered middle age for a star/the sun. The sun has used up half of the available hydrogen, which leaves our sun with about 5 billion years left, before the sun's hydrogen is burnt out, and the sun is no longer our primary source of energy for the earth or any other planet that has life on it.
Leaves falll
The fight sequence with the crazy 88 and o-ren at the house of blue leaves is what film cinematorgraphy highlight?
Astronomers use spectroscopy to analyze the light emitted by stars. By studying the absorption lines in a star's spectrum, astronomers can identify the elements present in its composition. Since hydrogen leaves a distinct signature in these absorption lines, scientists have found that hydrogen is the most abundant element in stars, including our Sun.
the Stomach leaves a print on the water, which can't be removed, and scientists can tell how many from that - i don't know how many though . . . . .
what type of scientists is interested in the rate of photosynthesis in leaves
Scientists group leaves on the basis of their leaflets and axillary buds into simple and compound leaves; they are then further categorized according to shape and leaf venation
Varies from plant to plant depending on what compounds are in their leaves. Most likely Oxygen, Carbon, Nitrogen, and Hydrogen.
http://www.youtube.com/watch?v=9acI8EWNqzg