Stellar evolution is the process by which a star undergoes a sequence of radical changes during its lifetime. Depending on the mass of the star, this lifetime ranges from only a few million years (for the most massive) to trillions of years (for the less massive), considerably more than the age of the universe. ^
Small, relatively cold, low mass red dwarfs burn hydrogen slowly and will burn for hundreds of billions of years
Massive hot supergiants will live for just a few million years.
A mid-sized star like the Sun will remain on the main sequence for about 10 billion years. Hope tis helps!!
The answer for your question is 1. Easy to grow crops
Answer:
A. The rest is still out of frame
Explanation:
The mRNA codon translated to amino acids is placed below.
While serine, which is one of the amino acids in the original protein, is still there as a part of the new sequence, there are a host of other frame shift mutations. While it is possible to phosphorylate a serine in any of these amino acid sequences, the secondary and tertiary structure of these are different to each other.
Original:
5' - UG | GUC | GGC | GAG | AAC | GAA | AGC | GC - 3'
Val Gly Glu Asn Glu Ser
Mutation:
5' - UG | GUC | GGG | AGC | ACG | AAA | GCG | C - 3'
Val Gly Ser Thr Lys Ala
