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Heredity is a Division B event that rotated in for the 2019, 2020 and 2021 seasons. It was previously an event for the 2013 and 2014 seasons. The event covers topics relating to genetics, molecular biology, and hereditary inheritance.
- 1 Inheritance
- 2 DNA
- 3 RNA
- 4 Mitosis & Cell Cycle
- 5 Meiosis
- 6 Genetic Disorders
- 7 Resources
Single-Factor (Monohybrid) Crosses
The images to the right are examples of Punnett squares, named after the geneticist Reginald C. Punnett. Punnett squares show the cross between alleles and the genotype of the resulting offspring. Since both of the Punnet squares in the diagram only cross one trait (one pair of alleles), it is called a monohybrid or single-factor cross. Likewise, when two traits (two pairs of alleles) are crossed, it is called a dihybrid or two-factor cross. Dihybrid crosses are described in the next section of this page.
The Punnett square at left shows a cross between two heterozygous plants (that is, they each have one dominant allele and one recessive allele). The Punnett square at right shows a cross between a homozygous tall plant and a homozygous short plant (homozygous means that both alleles are the same). The letters inside the boxes represent the genotype of each offspring, with each individual letter representing a single allele. Note that the choice of letters is arbitrary and dictated mostly by convention - for simple dominant/recessive genes, the first letter of the dominant trait name is most common, as uppercase for the dominant trait and lowercase for the recessive trait. For example, in the first square, the genotypes of the offspring will be TT, Tt, and tt (2 of the 4 offspring will have the same genotype-Tt).
It is helpful to memorize the genotypic and phenotypic ratios of a heterozygous monohybrid cross. If two heterozygotes are crossed (like the left Punnett Square in the image to the right) then the genotypic ratio will always be:
- 1 homozygous dominant : 2 heterozygous : 1 homozygous recessive
and the phenotypic ratio will be:
- 3 dominant : 1 recessive
Note that genotypic and phenotypic ratios are often written without the particular allelic combinations or traits - for example, the above two ratios will most often be written as 1:2:1 and 3:1 respectively.
Memorizing other simple crosses (such as a single-factor homozygous dominant x homozygous recessive cross) is useful and saves time on tests. Here are some simple monohybrid crosses with their respective genotypic and phenotypic ratios.
|Cross||Geontypic ratio||Phenotypic ratio|
|Aa x Aa (Heterozygous x Heterozygous)||1 AA : 2 Aa : 1 aa||3 dominant : 1 recessive|
|AA x aa (Homozygous dominant x Homozygous recessive)||0 AA : 4 Aa : 0 aa||4 dominant : 0 recessive|
|AA x Aa (Homozygous dominant x Heterozygous)||2 AA : 2 Aa : 0 aa||4 dominant : 0 recessive|
|Aa x aa (Heterozygous x homozygous recessive)||0 AA : 2 Aa : 2 aa||2 dominant : 2 recessive|
The two remaining types of crosses, AA x AA and aa x aa, are not shown because the ratios are trivial - since only one allele is present between both parents, all offspring will be homozygous for that allele and display the associated trait.
Note that a genotype refers to a combination of alleles, while a phenotype refers to a trait displayed by an organism. Likewise, the genotypic ratio is a ratio of the various possible genotypes in a cross, while the phenotypic ratio is a ratio of the various possible phenotypes in a cross. These terms are important and often confused - pay attention to the exact terms being used on tests so that your answers match what is being asked for by the questions.
Two-Factor (Dihybrid) Crosses
Two-factor (dihybrid) crosses are similar to single-factor crosses, but involve two traits as opposed to one single trait. An example of this revolving around peas is pictured to the right. Both organisms are heterozygous for the two traits being crossed, meaning that their genotypes are RrYy. In this example, the "R" allele represents the shape of the seed and the "Y" allele represents the color. It is important to note the genotypic and phenotypic ratios for a heterozygous dihybrid cross. Regardless of the alleles, if two dihybrid heterozygotes are crossed, then the resulting phenotypic ratio will be:
- 9 D/D: 3 D/R: 3 R/D: 1 R/R (D = Dominant trait, R = Recessive trait)
and the genotypic ratio will be:
- 1 D/D: 2 D/H: 1 D/R: 4 H/H: 4 H/D: 1 R/D: 2 R/H: 1 R/R (D = Homozygous dominant, R = Homozygous recessive, H = Heterozygous)
So, the phenotypic ratio for the pictured dihybrid cross is:
- 9 round/yellow:3 round/green: 3 wrinkled/yellow: 1 wrinkled/green
Note that a dihybrid cross can be broken down into two overlaid monohybrid crosses. Each group of four squares in the image (top left, bottom left, top right, and bottom right) represent one of the possible results of a monohybrid cross Rr x Rr. Each of the squares within those four groups represents the possible results of a monohybrid cross Yy x Yy - this can occur once for each possible result of the Rr x Rr cross.
As with monohybrid crosses, dihybrid crosses can involve parents with various combinations of genotypes. While it may not be practical to memorize all of the different types of dihybrid crosses, it is useful to have them on a notesheet for reference, since they frequently come up on tests.
Crosses and Punnett squares may be used with any number of genes. As of the 2019 rules, trihybrid crosses are a Nationals-only topic, rarely seen on tests, and higher crosses are not allowed on tests. Like single- and double-factor crosses, three-factor (trihybrid) crosses show three different traits that are crossed. The image at right shows a trihybrid cross between two parents that are heterozygous for all three traits (that is, a genotype of AaBbCc). Trihybrid crosses are rarely seen on tests, so don't spend too much time practicing them until the later stages of competition.
Special Forms of Inheritance
Strict dominant/recessive genes are useful for illustrating the basic concepts of Mendelian inheritance but are relatively rare in real life. Various other forms of allele interactions are also part of this event.
Incomplete dominance and Codominance
In some cases neither of the two alleles establishes dominance, and the heterozygous phenotype is different from either of the homozygous phenotypes. This can result in either incomplete dominance or codominance, depending on the specifics of the phenotypic expression.
In incomplete dominance, the heterozygous phenotype is an intermediate variety between the two homozygous phenotypes. For example, 4 o'clock flowers have a homozygous red phenotype and a homozygous white phenotype, while the heterozygous condition displays a pink color (see the image at left). Often, incomplete dominance is shown in the allele symbols with an "I" and the first letter of the particular phenotype in superscript.
Codominance is very similar to incomplete dominance, but the specifics of the phenotypic interaction are different. In codominance, the heterozygous phenotype displays both homozygous phenotypes in some way. For example, roan cows express both the red and white alleles in patches (see the image at right). Another example of a gene that includes codominance is ABO blood type, described in a later section.
Note that the convention of capital letters vs. "I" and superscript for codominance vs. incomplete dominance is loose - the use of a particular convention doesn't necessarily help distinguish the two on tests.
Sex-linked traits are features that are associated with the genes on the sex chromosomes. Most sex-linked genes, such as the recessive alleles for red-green color blindness and hemophilia, are carried on the X chromosome; however, there are a few Y-linked genes (e.g. some forms of baldness).
The most notable feature of X-linked recessive traits is the fact that they tend to occur more often in males since only a single X chromosome with the allele is needed for the trait to be displayed (as males have one X and one Y chromosome). In contrast, females must have the allele on both X chromosomes to display the trait. The Punnett square at left is an example of hemophilia, a common example of an X-linked recessive trait. X-linked traits may be dominant as well, though that is much less common. It is also worth noting that due to X chromosome inactivation in females, the dominant/recessive model is not as accurate for X-linked traits.
Y-linked traits are less common than X-linked traits due to the smaller size of the Y chromosome. They also follow a much simpler inheritance pattern since they can only pass through the male line. If a father has the trait, all of his sons will also have the trait, and vice-versa (since they can only receive the one affected Y chromosome).
Most phenotypic features are controlled by more than one set of non-allelic genes acting on them, such as height, skin color, intelligence, and hair and eye color. Usually this type of problem is seen as a typical two or three, etc factor cross with the more dominants, the more expression of the trait in question.
There may be more than the usual two alleles for any given gene. A particular individual may have two of those alleles in some combination. Especially, this appears in fur or pelt conditions of domestic animals. The types of interactions between these alleles may vary - for example, the most common example (the ABO blood type system) includes 3 alleles - the IA and B alleles, which are codominant with each other (despite the frequent use of "I" and superscript, this is not an example of incomplete dominance), and the i allele (representing blood type O) which is recessive to IA and IB.
While lethal alleles do not affect the way you set up your Punnett square, they can appear to alter Mendelian ratios. A lethal genotype is one that causes death before the individual can reproduce and pass their genes on to the next generation. As such, they remove an expected progeny class after a specific cross. For example, in Mexican hairless dogs, the genotype hh means that the dog is hairy, Hh means that the dog is hairless, but HH means that they die as embryos - thus the term "lethal".
Epistasis is where one set of genes stops or inhibits the action of other genes. The most common example of epistasis is albinism. Consider a simple dominant/recessive gene for eye coloration, where B = brown and b = blue (simplified for illustrative purposes). Say there is another simple dominant/recessive gene where P = normal pigmentation and p = not pigmented (i.e. albino). If the albinism gene is homozygous dominant or heterozygous in an individual they will have normal pigmentation and their eye color will be according to their eye color genotype. If, however, they are homozygous recessive for albinism they will have reddish eyes (which is the typical phenotype for albino eyes), regardless of whether their eye color genotype is BB, Bb, or bb - the epistatic albinism gene overrides the eye color gene. Epistasis genes do not necessarily have to be recessive - for example, some flowers have epistatic genes where the dominant allele suppresses the production of certain pigments.
A pedigree is a graphical depiction of the inheritance pattern of a single trait through a family tree. The image at right shows an example of a pedigree, with some common symbols in the key. The conventions of squares for males and circles for females, as well as that of shading to show individuals with the trait in question, are among the few that are common to all pedigrees - there is a lot of variation. For example, some pedigrees indicate carriers of a trait with partially shaded squares/circles, while others do not.
Often, questions involving pedigrees may ask competitors to determine the genotypes of several individuals or identify the inheritance pattern of the trait in question. For example, consider the pedigree at right. Based on the fact that neither individual in the first generation has the trait but some of their direct offspring do, we know that carriers are not marked in this pedigree (and we also know that the trait cannot be dominant). The fact that all six affected individuals are male strongly implies that the trait is sex-linked. Y-linkage can be ruled out because some affected sons have unaffected fathers, and vice-versa. Therefore, the most likely inheritance pattern for this trait is X-linked recessive. Note that we have not ruled out an autosomal recessive inheritance pattern since there is not enough information in this pedigree to do so.
DNA is made up of three components: a phosphate group, a deoxyribose sugar, and heterocyclic (the ring contains both nitrogen and carbon atoms) ring(s) for the nitrogenous base. Purines have two such rings; pyrimidines, one. The bases found in DNA are adenine and guanine (purines), and thymine and cytosine (pyrimidines), and are usually referenced by their first letter A, T, C, or G, especially when writing sequences. Mnemonics for remembering purines vs. pyrimidines are "CUT pie" and "Pure As Gold;" C, U (uracil in RNA), and T are pyrimidines, while A, G are purines; purine is the shorter word and has more rings.
Note that nucleotides and nucleosides are different. Nucleosides consist of just the deoxyribose sugar and the base (heterocyclic rings). Nucleotides are nucleosides with phosphate groups; as such, sometimes nucleotides are referred to as nucleoside phosphates, with a prefix on phosphates describing the number of phosphate groups attached (e.g. triphosphate if there are three).
The carbons on the sugar are number with primes (e.g. 3', read as "three prime"). The phosphate group is attached to the 5' carbon, and the nitrogenous base is attached to the 1' carbon. The sugar and phosphate groups form the backbone or the sides of the double helix "ladder" and the nitrogenous bases stick out from the chain like "rungs" of the ladder.
Watson, Crick, and Maurice Wilkins are often credited with finding the structure of DNA. Rosalind Franklin, however, was the first to use X-ray diffraction to see the DNA helix. Watson and Crick used her work to discover the helical structure in 1953. See The Double Helix by James D. Watson for more information.
DNA is stored in the nucleus of a cell in a form known as chromatin. This chromatin consists of loose DNA, proteins called histones, and RNA. Chromatin has a variety of functions including:
- Packaging loose DNA into a more dense shape
- Reinforcing DNA so mitosis can occur
- Preventing DNA damage that could result in mutation or cell death
- Controlling gene expression and replication
There are two varieties of chromatin known as euchromatin and heterochromatin. Euchromatin is the most actively transcribed form of DNA, and 92% of the human genome is euchromatic. Heterochromatin is more tightly packed, and typically is responsible for structural functions such as the centromeres and telomeres on a chromosome.
Chromatin condenses into chromosomes at the beginning of mitosis. During mitosis, the chromosome has a copy of itself attached to it at the centromere known as a chromatid. This copy was created during DNA replication. These chromatids are later separated and becomes their own individual chromosomes. During mitosis all chromatids are sister chromatids, meaning that they are identical. Non-sister chromatids appear in meiosis when a paternal and maternal chromosome are paired together.
Adenine only hydrogen bonds with thymine and guanine bonds only with cytosine. This is called base pairing. According to Chargaff's rule, an organism should have equal percentages of adenine and thymine and cytosine and guanine. One way to remember which base pairs with which is to remember the "curvy" letters go together. If Chargaff's rules do not hold, the organism's DNA may be single-stranded rather than double-stranded.
In RNA, uracil replaces thymine and thus, uracil bonds with adenine. DNA bases are Adenine-Thymine, Cytosine-Guanine. RNA bases are Adenine-Uracil, Cytosine-Guanine. Any other base pairing combinations are considered errors.
When a cell divides, it makes a duplicate of its DNA in the S-phase of the cell cycle so the daughter cells will have a complete set of chromosomes (see below, Mitosis). This process is DNA replication, also called DNA synthesis.
First, helicase separates the strands by breaking the hydrogen bonds between nitrogenous bases while topisomerase relieves supercoiling in the DNA caused by helicase. This area of separation is called a replication fork. Single-stranded DNA-binding protein keeps the separated DNA strands from rejoining (re-annealing).
Before DNA polymerase can enter the replication fork to make copies of the DNA strands, primase must put down an RNA "primer" that forms hydrogen bonds with existing DNA bases; this is the starting point for DNA polymerase. The next step is elongation by DNA polymerase, which creates some difficulties because of how enzymes "read." DNA polymerases can only copy from 5' to 3' which works for one strand, called the leading strand. However, the complementary DNA strand is 3' to 5'; this strand is called the lagging strand. While DNA polymerases can copy the leading strand in one piece without a problem, it can only replicate the lagging strand in spurts by replicating small sections in the 5' to 3' direction. The replicated portions of the lagging strand done in spurts are called Okazaki fragments. Each Okazaki fragment requires a new primer before DNA polymerase can copy that fragment. (In eukaryotic replication, only the DNA polymerases involved in elongation have proofreading capability. Therefore, primers are a possible site for errors which are more frequent along the lagging strand.)
Once elongation is complete, an exonuclease (an enzyme that cleaves nitrogenous bonds) replaces the RNA primers with DNA bases. Finally, ligase connects the backbones of adjacent sections by catalyzing the formation of phosphodiester bonds between the 3' hydroxyl group and the 5' phosphate. This connects backbones of replicated sections with each other and the rest of the DNA strand.
Prokaryotes, which have circular genomes, usually only have one active origin of replication. This means replication starts at one point along the loop, continues around the entire loop (in opposite directions on complementary strands) until the entire genome is copied. Eukaryotes can have multiple origins of replication. This means multiple sets of enzymes replicating DNA can simultaneously copy different sections of DNA. Ligase connects these many sections that are replicated, forming one continuous genome.
DNA replication is considered semi-conservative. This means that after copying a strand of double-stranded DNA, each copy will have one strand from the original parent strand. This contrasts with conservative replication where one strand would be entirely original and a second would be entirely new.
RNA (ribonucleic acid) is usually a single-stranded nucleotide chain, not a double helix like DNA. While it does not share the same structure as DNA, it has many similar properties. RNA consists of a ribose sugar and hydroxyl group (on the 2' carbon of ribose), as opposed to deoxyribose (which only has hydrogen on the 2' carbon). RNA also consists of adenine, guanine and cytosine, but thymine is replaced with uracil.
There are three major types of RNA. While there are many other minor types, these three are heavily involved in translation.
- Messenger RNA (mRNA): Encodes the sequence of amino acids that becomes a protein.
- Transfer RNA (tRNA): Transports amino acids to ribosomes during translation. It contains about 80 RNA nucleotides, with an amino acid attached to the 3' end and an a complimentary anticodon attached to the 5' end.
- Ribosomal RNA (rRNA): Along with ribosomal proteins, rRNA makes up the ribosome which is molecular machine the that translates mRNA into proteins.
Some of the other classifications of RNA are useful to recognize and are listed below.
- Non-coding RNAs (ncRNA): This refers to any RNAs that do not result in a protein product. This includes tRNA and rRNA mentioned above.
- microRNA (miRNA): Short sections of RNA that can anneal to matching complementary strands of RNA, silencing expression by preventing their translation.
- Small nuclear RNA (snRNA): snRNA is involved in splicing of pre-mRNA. Splicing only occurs in eukaryotes, and produces different transcripts by removing introns.
- Pre-messenger RNA (pre-mRNA): This refers to newly transcribed RNA that has not be processed by post-transcriptional processing.
- Heterogenous nuclear RNA (hnRNA): RNAs located in the nucleus, which includes pre-mRNA.
Transcription (DNA to mRNA)
Transcription is the process of transcribing DNA into pre-mRNA so that it can be later translated into proteins. This is the first major step of gene expression and occurs within the nucleus in eukaryotes. Transcription produces a complementary sequence to the DNA; A pairs with T in DNA, U pairs with A, G pairs with C and C pairs with G. For example:
DNA: 3' GCACGTGTAGCATAGTACTAG 5' mRNA: 5' CGUGCACAUCGUAUCAUGAUC 3'
Transcription occurs in the nucleus during the G0 phase (non-dividing) as well as the G1 and G2 phases of the cell cycle. In eukaryotes, it occurs in three distinct stages: initiation, elongation, and termination.
- Activator proteins bind to distal control elements that are located before the DNA sequence known as a promoter. Promoters are located near but before the start sites of genes, and allow various proteins and enzymes (such as RNA polymerase II) to form an initiation complex via binding that begins transcription. Note that promoters are part of initiation and their specific sequences are not transcribed.
- Proteins called transcription factors bind to a specific DNA sequence known as a promoter. At this point in the process, the DNA is still double stranded. RNA polymerase binds to the promoter region shortly after the transcription factors.
- RNA polymerase unwinds approximately 14 base pairs to form an "open complex" that becomes the transcription bubble. As the RNA polymerase begins creating RNA, the produced RNA enters the RNA exit channel and leaves behind the initial transcription factors.
- RNA polymerase begins unwinding the double helix and exposes 10-20 nucleotides at at time for transcription. RNA polymerase builds the new RNA using free-floating RNA nucleotides in the nucleoplasm.
- RNA polymerase travels from the 3' → 5' direction on the template strand of DNA, producing a mRNA strand in the 5' → 3' direction. This process produces an RNA copy of the 5' → 3' DNA strand (e.g. if the DNA strand being transcribed is 3'-ATCG-5', the RNA product will be 5'-UAGC-3', which matches the DNA sequence's complementary strand, 5'-TAGC-3' but with U instead of T.)
- RNA transcription occurs very quickly, and can involve multiple RNA polymerases simultaneously working on a single gene. The typical rate of elongation is 10-100 nucleotides/sec.
- Elongation also involves a proofreading mechanism that can replace incorrect nucleotides. Transcription pauses, allowing RNA editing factors to bind to the new strand of mRNA and edit base order.
- The RNA codes for the polyadenylation sequence (AAUAAA), and the proteins associated with the RNA polymerase stop moving.
- RNA polymerase continues moving, adding hundreds of adenine nucleotides to the end of the mRNA strand. Spare RNA created like this may be used by enzymes.
- A termination factor releases the newly created mRNA, called pre-mRNA, which after post-transcriptional processing leaves the nucleus and travels to the ribosome where it is translated into a protein.
Pre-mRNA Processing (Post-Transcriptional Processing)
Pre-mRNA processing is a process that only occurs in eukaryotes. When mRNA is first transcribed, it is known as a pre-mRNA. This processing turns it into a full-fledged mRNA, allowing it to be translated into proteins. First, a 5' cap is added to the beginning, 5' end, of the pre-mRNA, and a 3' poly-A tail is added to the end. The 5' cap is a modified guanine molecule, 7-methylguanylate, that protects the 5' end of the transcript from degradation by ribonucleases (RNases). The 5' cap also allows the ribosome to attach to the mRNA in the first step of translation. The 3' poly-A tail is made of 100-200 adenine (A) bases, stabilizing the mRNA. The poly-A tail is gradually degraded by RNases, so the length of the sequence helps delay degradation from reaching the protein-coding sequence of the RNA. The addition of the cap is simply known as mRNA capping, while the addition of the tail is known as polyadenylation.
In splicing, snRNP (small nuclear ribonucleoproteins) and snRNA (small nuclear RNAs) remove sections of the transcript called as introns, leaving behind the remaining sections, exons. This post-translational processing step allows for one pre-mRNA to code for many different protein produces by merely varying which introns are removed. For more information on splicing, see Designer Genes#Alternative splicing.
Translation (mRNA to Protein)
Translation is the process of translating the mRNA created during transcription into a protein. These proteins are responsible for different genetic traits such as hair/eye color, blood type, or hereditary conditions such as color blindness. These proteins may also have important cellular functions, such as DNA replication.
Translation takes place in the cytosol on ribosomes, enzymes with three chambers and two subunits that consists of rRNA and other proteins. Ribosomes are often referred to by their small subunit and large subunit. The small subunit initially binds to the mRNA, while the large subunit contains the chambers responsible for protein synthesis. The three chambers are the A site (aminoacyl-tRNA binding site), the P site (peptidyl-tRNA binding site) and the E site (exit site). Like transcription, translation occurs in three steps: initiation, elongation, and termination. An mRNA transcript is translated into a protein by reading three mRNA bases at a time; these three-letter "words" are called codons and correspond to a complementary anticodon.
- The small subunit attaches to the mRNA and locates the start codon, AUG. The charged methionine tRNA binds to the start codon.
- The large subunit arrives and and attaches to the small subunit, completing the translation initiation complex.
- Amino acids are brought to the ribosome by charged aminoacyl-tRNA molecules and are added to the polypeptide chain one by one.
- As the charged tRNA molecules enter the complex through the A site, they move to the P site to the E site.
- The anticodon on a tRNA molecule binds to the mRNA codon at the A site.
- At the P site, an rRNA molecule in the large subunit catalyzes the formation of a peptide bond between the amino acid on the tRNA and the polypeptide chain.
- The tRNA exits the ribosomal complex through the E site. The tRNA, having lost its amino acid to the growing polypeptide, is now considered uncharged.
- The stop codon (UAA, UAG, or UGA) on the mRNA reaches the A site.
- Release factors bind to the stop codon at the A site.
- A water molecule is added to the end of the polypeptide instead of an amino acid, and hydrolysis releases the chain so it can be later folded into its final structure.
In eukaryotes, protein folding occurs in the rough endoplasmic reticulum (rough ER) and can be facilitated by chaperone proteins that help proteins fold correctly. In prokaryotes, which lack compartmentalized organelles, transcription and translation can occur simultaneously, meaning a protein can be made while the mRNA that codes it is still being made!
Interpreting Genetic Code
In translation, each of the three-letter codons corresponds with a complementary anticodon on a particular tRNA; different tRNA molecules are attached to different amino acids (the building blocks of proteins), meaning that each codon corresponds with one amino acid. Since there are only four different RNA nucleotides (A, U, C, and G), there are 64 possible three-letter codons. However, there are only 20 standard amino acids. This means that multiple codons can code for the same amino acid; this redundancy is called degeneracy. Usually, but not always, codons that code for the same amino acid have the same first two letters with a differing third letter; this property where a different third letter allows coding for the same amino acid is called wobble.
A sequence or chain of amino acids is called a polypeptide. Polypeptides are translated from the N-terminus to the C-terminus; the N-terminus has an amino group, and the C-terminus has a carboxylate group. A protein can consist of a single polypeptide or multiple polypeptides. Proteins are responsible for most biological functions in the body such as DNA replication, transcription, transporting molecules, and regulation of gene expression. Proteins are very complex macromolecules and have four different levels of structure. The amino acid sequence created in translation is known as the primary structure. The other levels of structure involve interactions between these amino acids or between entire polypeptides.
It is possible to interpret a DNA sequence into an amino acid sequence by using a chart like the one shown to the right. First, find the RNA nucleotides that would pair with the DNA nucleotides. This is the transcription step.
DNA: 3' TAC AGG TAG CTA GTT ATT 5' RNA: 5' AUG UCC AUC GAU CAA UAA 3'
Then, convert each three-letter codon to amino acids, following the sequence of nucleotides on the chart from the inside out. For example, the RNA sequence AUG corresponding to methionine (Met) starts translation, so methionine is found at the beginning of every newly-translated protein. (Although this does not mean that every protein begins with methionine; in many cases, the protein is processed after translation and the methionine may be removed. Methionine also isn't restricted to only being a start codon; it can also be elsewhere in the protein.)
In the center of the circle, start with the A quadrant, then follow the U quadrant and then the G quadrant. Note that the stop codon does not code for an amino acid.
RNA: 5' AUG UCC AUC GAU CAA UAA 3' Amino Acids: N- Methionine Serine Isoleucine Aspartic Acid Glutamine Stop -C
While remembering the codon to amino acid conversions is not necessary, it may be helpful to remember the start and stop codons. The start codon is AUG; stop codons are UAA, UAG, and UGA. A mnemonic for remembering the stop codons is "U Are Amazing, U Are Genius, U Got A's."
The 20 amino acids also can be referred to by their full names, but are more commonly referred to by their three-letter or single-letter abbreviations, which are listed in the table below. The example peptide above could be called Met-Ser-Ile-Asp-Glu or MSIDE. Peptide sequences are always written from N- to C-terminus.
List of Amino Acids
|Name||Abbreviation||One Letter Code|
Mitosis & Cell Cycle
The body grows by cell division, and mitosis is the process of cell division in somatic cells (that is, all cells other than the germ cells which produce eggs and sperm). In mitosis, a single diploid (two copies of each chromosome, one from each parent) cell divides to produce two diploid cells (the daughter cells). It is a part of the cell cycle, which describes the general life cycle of a cell.
Specifically, mitosis refers to the separation of replicated DNA chromosomes (and as a result the creation of two nuclei), while cytokinesis is the actual division of the cell into two distinct cells with each their own membrane. Mitosis can be divided into four phases: prophase, metaphase, anaphase, and telophase. Before mitosis is a step called interphase.
Interphase is the part of the cell cycle that does not constitute mitosis; it is the phase in between two cell divisions, when the cell is growing. Most cells spend about 90% of their time in interphase. It consists of three separate stages:
- G1 phase (Gap 1) - This is the primary growth phase of a cell, and typically the longest phase. The cell grows and absorbs nutrients during this time. During this phase, organelles such as mitochondria and chloroplasts (for plant cells) are duplicated.
- S phase (Synthesis) - Since the daughter cells must each have a full set of chromosomes (i.e. diploid), the DNA in the parent cell must replicate, which it does during this relatively short phase.
- G2 phase (Gap 2) - A second, typically shorter gap phase in which the cell grows and prepares for mitosis.
Two critical checkpoints occur around these phases: the G1 checkpoint after the G1 phase, and the G2 checkpoint at the end of the G2 phase. The G1 checkpoint checks for existing DNA damage and proper nutrients for growth. The G2 checkpoint checks for proper DNA replication from the S phase and if necessary makes repairs. A cell that passes both checkpoints may proceed from interphase to mitosis. These checkpoints are important for ensuring proper division of cells, and malfunctioning checkpoints can allow unregulated cell division that can proceed to cancer.
The first step of mitosis is prophase. Prophase can be divided into two separate part: early prophase, and late prophase (prometaphase). Some argue that prometaphase is its own distinct step, while others consider both to be part of prophase.
At the beginning of early prophase, chromatin condenses to form chromosomes which protects the DNA; (a condensed chromosome is more likely to be transferred in one pieces without breaking apart). The mitotic spindle (also called the spindle apparatus) also begin to form; this is a skeleton consisting of strong microtubules (proteins) which organize chromosomes and move them during mitosis. The mitotic spindle originates from the centrioles in centrosomes of the cell. The nuclear envelope breaks down and the nucleolus (within the nucleus) disappears, which is a sign that the cell is undergoing mitosis.
In prometaphase, the mitotic spindle begin to organize the chromosomes by moving them. The chromosomes have finished condensing and are very compact. The microtubules of the spindle apparatus bind to the chromosomes at the kinetochore, which is a patch of protein found on the centromere of each sister chromatid. The centromere is the section of DNA where the sister chromatids (each copy of a chromosome) are the most tightly attached. Not all microtubules bind to chromosomes, and some just help stabilize the spindle.
In metaphase, all of the chromosomes have been arranged by the spindle apparatus, and they are lined up at the middle of the cell along an invisible plane called the metaphase plate. The two kinetochores on each chromosome are attached to microtubules originating from opposite ends of the cell. Before anaphase, the cell ensures that every chromosome is properly aligned and attached to the microtubules. This is called the spindle checkpoint, and it ensures that sister chromatids split properly during anaphase. If something is wrong, the cell pauses its division until the problem is fixed.
During anaphase, the sister chromatids are separated and pulled towards opposite ends (poles) of the cell. The proteins holding them together are broken down, and each is now its own chromosome. Microtubules that aren't attached to chromosomes push apart, elongating the cell and separating the poles. All of these processes are carried out by motor proteins.
Improper separation of sister chromatids or nondisjunction may occur at this step, causing a single cell to receive both chromatids.
Once the cell reaches telophase, it is nearly finished dividing. The mitotic spindle is broken back down, and two new nuclear envelopes begin to form, one for each set of chromosomes. The nucleoli reappear in each cell, and the chromosomes begin to decondense into chromatin. Telophase is essentially the reverse of prophase.
Cytokinesis overlaps with the final stages of mitosis, and can begin in either anaphase or telophase. It is different in animal and plant cells, since animal cells do not have a cell wall. In animal cells, the cell is drawn shut across a cleavage furrow by microfilaments and the two cells split. In plant cells, a cell plate forms down the middle and divides the two daughter cells with a new wall.
Meiosis is the process of cell division that is unique to germ cells. It produces haploid eggs and sperm from diploid progenitors. It occurs in two stages, Meiosis I and Meiosis II, each of which goes through the four main stages of mitosis, although in a different way that allows for genetically variable daughter cells.
During prophase I, the chromosomes condense as the nuclear envelope breaks down. By this point all of the cell's genetic material has replicated, so each chromosome is an X-shape consisting of two identical chromatids. Also during this phase, homologous pairs of chromosomes line up and undergo crossing over - homologous sections of the chromosomes swap. This process increases the genetic diversity of the haploid cells that are produced at the end of meiosis. As with mitosis, the centrosomes and spindle fiber structures form during prophase I.
Unlike mitosis, where the chromatids are separated, in meiosis I each chromosome is separated from its homologous chromosome. In metaphase I each chromosome will "join" with its homologous chromosome (forming a tetrad) and align across the centerline of the cell. Each chromosome is separated from its homologue during anaphase I, and during telophase I and cytokinesis the cell divides completely, forming two diploid daughter cells with differing DNA.
Some cells go into a rest stage, sometimes known as interphase II, after meiosis I is complete. Often, the nuclear envelope reforms and chromosomes uncondense prior to meiosis II.
Meiosis II is more similar to mitosis, except that the parent cells are diploid instead of tetraploidal (which is how the mitosis parent is after replication during interphase). Each cell divides the same way as in mitosis, with the chromosomes splitting at their centromeres. Note that because crossing over during prophase I occurs independently on each chromatid, the four daughter cells produced as a result of meiosis II are typically all genetically different.
In spermatogenesis, typically all of the daughter cells can become viable sperm. In contrast, during oogenesis only one of the four daughter cells will become a viable egg cell. The egg cell will receive most of the cytoplasm and organelles, while the remaining three daughter cells become shrunken polar bodies. Most of the organelles brought by the sperm cell are destroyed after fertilization. Incidentally, this is what allows matrilineal heredity to be traced via mitochondrial DNA.
Genetic disorders are inherited medical conditions caused by abnormalities in the DNA. There are a variety of types of genetic disorders, and some are rarer than others. They are typically caused by mutations in specific genes, deletion of genes, or a person having an additional chromosome. While these genes can be known as disease-causing genes, the abnormality of a gene is the cause of the disorder.
One of the most common genetic disorders is known as trisomy 21, or Down Syndrome. An individual with this disorder has a third copy of chromosome 21. Cystic fibrosis is also a genetic disorder, caused by mutation in a protein known as CFTR. Even color blindness is a genetic disorder, caused by a mutation on the X chromosome.
Polysomy and Monosomy
Polysomy is when an individual having more than two copies of a particular chromosome. Most often this is a trisomy, such as trisomy 21 (Down Syndrome) - affected individuals have three copies of chromosome 21. Monosomy is when an individual has one copy of a chromosome rather than the normal two copies. The only known monosomy in which individuals survive to birth is Turner's Syndrome, a monosomy of the sex chromosomes in which affected individuals are females that have a single X chromosome.
Addition, Deletion, Translocation
Addition, deletion and translocation are all different forms of mutations. Addition (also known as insertion or an insertion mutation) is the addition of nucleotides into a DNA sequence. Additions can range in size from one base pair to entire sections of chromosomes being added in the wrong place. Deletion is a similar concept, but with the removal of nucleotides. In deletion, a part of a chromosome or DNA sequence is lost during replication. Any number of nucleotides can be deleted, though small deletions are typically less dangerous. Large deletions can be fatal, and some can result in various genetic disorders such as Williams syndrome.
Translocation is when the parts of a chromosome are rearranged, occasionally resulting in a genetic disorder. Translocation can be balanced or unbalanced, with unbalanced translocation resulting in missing or extra genes. There are multiple forms of translocation, but the most common is reciprocal translocation. This occurs when two parts of two chromosomes swap places, resulting in genes changing locations and occasionally gene fusion. Balanced translocation occurring during meiosis typically doesn't result in any visible symptoms, though in about 6% of cases it can result in autism or congenital abnormalities. However, translocation occurring in somatic cells during mitosis can result in various forms of cancer. Translocation can also result in infertility, or in specific cases a form of Down syndrome.
A karyotype is a chart that shows each chromosome. Each karyotype displays 23 pairs of chromosomes, including the X/Y chromosomes. Every pair is assigned a number (except for the sex chromosomes; they are always referred to as the X and Y chromosomes). Some genetic disorders can be detected by analyzing the number of chromosomes and/or the sex chromosomes. The gender of the individual can also be deduced from looking at the sex chromosomes. If there is an X and a Y, the individual is a male. A female has two X chromosomes and no Y chromosome.
A karyotype is created by stopping cells in cell division and staining the chromosomes, then observing them under a light microscope.
Karyotypes can be used to diagnose genetic diseases - most often polysomy or monosomy, but also some types of deletion and addition in certain chromosomes. For example, a karyotype can reveal a third chromosome 21, resulting in Down syndrome. It can also reveal Turner syndrome (45, X), a disorder that results in females with one X chromosome, and Klinefelter's syndrome (47, XXY), in which a man has two X chromosomes and one Y chromosome.
In humans, the male and female share 22 of the 23 pairs of chromosomes in each body cell. The 23rd pair is known as the sex chromosomes because it determines the sex of the individual. In the male, the sex chromosome consists of an X and a Y chromosome(XY) while the pair in females consists of two X chromosomes(XX). The male is the one who determines the sex of the child and the female gives an X to all eggs while the male randomly produces about 50% X sperm and 50% Y sperm.
In rare cases, through nondisjunction, a person will have three sex chromosomes. If they have three X (XXX) chromosomes, they are female. If they have even one Y chromosome (XXY), they are male. Although they will show more feminine qualities, any person who has a Y chromosome is considered a male. Other types of sex chromosome polysomy, as well as one monosomy (X), have been known to occur, though more rarely.
Common Genetic Disorders
Several genetic disorders appear frequently on tests as examples. While this event typically does not deal with the specifics of each disorder, it may be useful to know the inheritance patterns of some common disorders:
- Cystic Fibrosis - Autosomal recessive
- Down Syndrome - Trisomy of chromosome 21
- Hemophilia - Sex-linked (X-chromosome) recessive
- Polydactyly - Autosomal dominant
- Red-green color blindness - Sex-linked (X chromosome) recessive
- Sickle-cell anemia - Autosomal recessive
- Tay-Sach's Disease - Autosomal recessive degenerative disorder in Ashkenazi Jews