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PHAR150GBiochemistryDayMembraneTransport-4.pptx

PHAR 150G

Biochemistry

Membrane Transport

Vicky Mody, PhD

[email protected]

1

Learning Objectives

Transport of bacteria into cell membrane.

Explain what are transporters, their classification and their functions.

Define the terms uniport, antiport, symport, active transport, and passive transport.

Compare and contrast properties of carriers and channels.

Explain similarities and differences between enzymes & transporters.

Describe specific examples of passive transporters as well as primary & secondary active transporters.

Define ligand gated and voltage gated channels, with examples.

2

Case 1

A patient comes to the ER with the episodes of vomiting and watery diarrhea. He was severely dehydrated, with a severe drop in blood pressure related to fluid losses. He was diagnosed with cholera, caused by the bacteria Vibrio cholerae.

What is the mechanism of water, Na+, and Cl- loss in cholera.

Case 2

In a movie a person X tries to kill person Y by giving him a lethal dose of potassium chloride. Increase in potassium will cause membrane depolarization and increasing the refractory period and the delaying the action potential.

a) Potassium chloride is a salt so how is it transported across the membrane.

Disorder Cause Explanation
Gas gangrene Environmental Bacterial (clostridium) infection that secretes a toxin, which is a lipase, leading to cell membrane destruction. This leads to capillary destruction, and impaired blood flow to the affected area.
Cholera Bacteria Vibro cholera Watery diarrhea leading to dehydration caused by cholera toxin ADP-ribosyl a class of G proteins, altering their function and affecting water and salt transport across the intestinal mucosa.

Diseases discussed in this Class

Must Know

5

Cell Structure

6

Membranes : Boundaries of cells & organelles

Marks Biochemistry, 4th edition

A

B

A

FIGURE 11-1 Biological membranes. Viewed in cross section, all cell membranes share a characteristic trilaminar appearance. This erythrocyte was stained with osmium tetroxide and viewed with an electron microscope. The plasma membrane appears as a three-layer structure, 5 to 8 nm (50 to 80 Å) thick. The trilaminar image consists of two electron-dense layers (the osmium, bound to the inner and outer surfaces of the membrane) separated by a less dense central region.

Membranes : Boundaries of cells & organelles

Marks Biochemistry, 4th edition

FIGURE 11-1 Biological membranes. Viewed in cross section, all cell membranes share a characteristic trilaminar appearance. This erythrocyte was stained with osmium tetroxide and viewed with an electron microscope. The plasma membrane appears as a three-layer structure, 5 to 8 nm (50 to 80 Å) thick. The trilaminar image consists of two electron-dense layers (the osmium, bound to the inner and outer surfaces of the membrane) separated by a less dense central region.

Membranes : Boundaries of cells & organelles

Composed of lipids & proteins

Exhibit selective permeability

Two layers : inner & outer

Specific composition for specific types

Variation between species, tissue/cell types & organelles

FIGURE 11-1 Biological membranes. Viewed in cross section, all cell membranes share a characteristic trilaminar appearance. This erythrocyte was stained with osmium tetroxide and viewed with an electron microscope. The plasma membrane appears as a three-layer structure, 5 to 8 nm (50 to 80 Å) thick. The trilaminar image consists of two electron-dense layers (the osmium, bound to the inner and outer surfaces of the membrane) separated by a less dense central region.

Phospholipids on Membranes

Marks Biochemistry, 4th edition

Importance of Carbohydrates on Cell Surface

11

Carbohydrates on Cell Surfaces

Marks Biochemistry, 4th edition

FIGURE 11-1 Biological membranes. Viewed in cross section, all cell membranes share a characteristic trilaminar appearance. This erythrocyte was stained with osmium tetroxide and viewed with an electron microscope. The plasma membrane appears as a three-layer structure, 5 to 8 nm (50 to 80 Å) thick. The trilaminar image consists of two electron-dense layers (the osmium, bound to the inner and outer surfaces of the membrane) separated by a less dense central region.

The A, B, and O blood groups are determined by the carbohydrate composition of the glycolipids on the cell surface.

These glycolipids may also serve as binding sites for viruses and bacterial toxins before penetrating the cell.

For example, the cholera AB toxin binds to GM1-gangliosides on the surface of the intestinal epithelial cells. The toxin is then endocytosed in caveolae (invaginations or “caves” that can form in specific regions of the membrane). Once inside the cell, the toxin will alter normal cellular metabolism.

Importance of Carbohydrates on Plasma Membrane

Must Know

Bacterial Membrane Transport

14

Bacterial Penetration into the Cell Membrane

o understand how Tamilflu and Relenza function and how the virus might become resistant to them, we need a little background on the life cycle of the flu virus. When an unsuspecting victim inhales a flu virus, a protein on the surface of the virus called hemagglutinin (the ‘H’ in H1N1, for example) binds to a receptor called sialic acid on the surface of cells in the respiratory tract (see structure of sialic acid in picture above).

The cell takes in the virus, which then replicates inside the host cell. The newly formed viruses leave the cell by budding off the surface. The hemagglutinin on the new viruses can then bind to the sialic acid on the surface of other host cells, thus infecting new cells. For this to occur, however, the viruses need to escape the host cells. Another viral surface protein, neuraminidase (the ‘N’ in H1N1, for example), breaks down the sialic acid receptors so the viruses can escape.

Tamiflu and Relenza are structurally similar to sialic acid and will bind to the neuraminidase, but they cannot be broken down. Therefore, neuraminidase cannot bind to sialic acid on the cell surface when it has Tamiflu or Relenza bound to it. Because they prevent neuraminidase from functioning, the two drugs are collectively referred to as neuraminidase inhibitors (NAIs). When NAIs are present, some of the newly produced virus will get stuck to the original host cell and will not be able to infect other cells.  Some viruses will still escape, so NAIs don’t cure the flu but rather reduce its severity.

The influenza virus life cycle can be divided into the following stages: entry into the host cell; entry of vRNPs into the nucleus; transcription and replication of the viral genome; export of the vRNPs from the nucleus; and assembly and budding at the host cell plasma membrane. In this review, each stage of the viral life cycle will briefly be described.

Phagocytosis is a compartmentalization of solid or big particles. Englufed foreign particle is called phagosome

When the particle which is to be phagocytosed then it is called autophagocytosis. Phagocytosis is the process of endocytosis. When the particles are small or liquid then then it is called endocytosis.

HA is a homotrimer that forms spikes on the viral lipid membrane. These spikes of HA bind to sialic acid found on the surface of the host cell’s membrane [7]. The HA precursor, HA0, is made up of two subunits: HA1, which contains the receptor binding domain, and HA2, which contains the fusion peptide. These subunits are linked by disulphide bonds [8]. Two major linkages are found between sialic acids and the carbohydrates they are bound to in glycoproteins: α(2,3) and α(2,6). These are extremely important for the specificity of the HA molecules in binding to cell surface sialic acid receptors found in different species. Viruses from humans recognize the α(2,6) linkage, whereas those from avians and equines recognize the α(2,3) linkages. Those from swine recognize both [7]. This explains the importance of swine being a good mixing vessel for avian and human influenza viruses, hence producing dangerous pathogenic viruses.

Upon binding to the host cell’s sialic acid residues, receptor-mediated endocytosis occurs and the virus enters the host cell in an endosome. The endosome has a low pH of around 5 to 6, which triggers the fusion of the viral and endosomal membranes. The low pH induces a conformational change in HA0, leading to maintenance of the HA1 receptor-binding domain but exposing the HA2 fusion peptide. This fusion peptide inserts itself into the endosomal membrane, bringing both the viral and endosomal membranes into contact with each other. Several crystal structures of HA in its various conformations, i.e., at neutral and acid pH, have been solved and are reviewed in [7] and [8].

The acidic environment of the endosome is not only important for inducing the conformation in HA0 and, thus, fusion of the viral and endosomal membranes but also opens up the M2 ion channel. M2 is a type III transmembrane protein that forms tetramers, whose transmembrane domains form a channel that acts as a proton-selective ion channel [9,10]. Opening the M2 ion channels acidifies the viral core. This acidic environment in the virion releases the vRNA from M1 such that vRNA is free to enter the host cell’s cytoplasm [11].

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Entry of vRNAs into the nucleus

Influenza viral transcription and replication occurs in the nucleus; therefore, after being released into the cytoplasm, the vRNP must enter the nucleus. The viral proteins that make up the vRNP are NP, PA, PB1, and PB2. All of these proteins have known nuclear localization signals (NLSs) that can bind to the cellular nuclear import machinery and, thus, enter the nucleus. To date, it is unclear which NLS is the most important for vRNP nuclear entry. The different NLSs present in each of these viral proteins are reviewed in [12]. It is known that import occurs via the Crm1 dependent pathway by binding to the various karyopherins involved in nuclear import, for example, importin α and β.

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Transcription and replication of the viral genome

The influenza viral genome is made up of negative sense strands of RNA. In order for the genome to be transcribed, it first must be converted into a positive sense RNA to serve as a template for the production of viral RNAs.

Replication of the genome does not require a primer; instead, the viral RNA dependent RNA polymerase (RdRp) initiates RNA synthesis internally on viral RNA. This is possible, as the extreme 5’ and 3’ ends of the genome exhibit partial inverse complementarity and, hence, are able to base pair with one another to form various corkscrew configurations. It appears that a great number of di-nucleotide base pairs form, although the full mechanism of viral genome replication is still yet to be understood [13-16].

Given that the influenza A virus only encodes for 11 proteins, it has generated many sophisticated methods of utilizing the host cell’s machinery for its own purposes. Through understanding viral transcription, we have learned of a unique mechanism whereby the virus hijacks the host’s transcription machinery for its own benefits.

Mature cellular messenger RNAs (mRNAs) have a 5’ methylated cap and a poly(A) tail. It is known that the vRNPs have poly(A) tails but no 5’ caps. It was confusing when the influenza community discovered that the viral mRNAs did have a 5’ methylated cap and a poly(A) tail, but the 5’ cap was not found in the viral genome [17,18]. Much study went into this problem, and soon it was determined that the 5’ methylated caps of the viral mRNAs actually belonged to the cellular mRNAs. That discovery lead to the formulation of the “cap-snatching” mechanism [19-26]. The viral RdRp is made up of three viral proteins: PB1, PB2, and PA. PB2 has endonuclease activity. It binds to the 5’ methylated caps of cellular mRNAs and cleaves the cellular mRNAs’ 10 to 15 nucleotides 3’ to the cap structure. This cellular capped RNA fragment is used by the viral RdRp to prime viral transcription [27].

Cellular RNA Polymerase II (Pol II) binds to DNA and starts transcription. During transcription initiation, serine 5 on the C-terminal repeat domain (CTD) of Pol II is phosphorylated, leading to the activation of cellular cap synthesis complex. The influenza RdRp has been shown to bind preferentially to this form of Pol II, indicating that this could be the point at which “cap snatching” could occur [28].

Six but two of the viral segments encode for one protein. Segments 7 and 8 encode for two proteins each due to splicing. Segment 7 encodes for M1 and M2; whereas, segment 8 encodes for NS1 and NEP. M2 and NEP are the spliced products and generally are found in much lower abundance than NS1 and M1 [29]. The virus uses the host cell’s splicing machinery to express both of these proteins [30]. Despite influenza’s need for the cellular splicing machinery, it prevents the host cell from using its own splicing machinery for processing the host cell mRNAs. NS1 binds to U6 small nuclear RNAs (snRNAs) [31,32] and other splicing components, causing them to re-localize to the nucleus of infected cells [33]. In this way, influenza is able to inhibit splicing of cellular mRNAs. It also has been shown to bind to a novel protein called NS1 binding protein (NS1-BP), causing it to re-localize to the nucleus in infected cells. The function of NS1-BP is unknown, although it is predicted to be involved in splicing given its co-localization with SC35, a spliceosome assembly factor [34]. NP also has been shown to interact with UAP56, a splicing factor involved in spliceosomal formation and mRNA nuclear export, although the importance of NP’s binding to UAP56 is yet to be established [35].

The mechanism of polyadenylation of viral mRNAs is very unusual. Cellular mRNAs are polyadenylated through cleavage at the polyadenylation signal (AAUAAA) by cleavage and polyadenylation specificity factor (CPSF) and subsequent addition of a poly(A) tail at the 3’ end of the mRNA. Viral mRNAs do not contain this sequence; instead, the viral RdRp remains bound to the 5’ end of the template viral RNA, leading to steric blockage at the end of viral RNA synthesis [36,37]. Each viral segment has a stretch of five to seven U residues approximately 17 nucleotides from the 5’ end, and this forms the basis of the viral polyadenylation signal [38]. Therefore, polyadenylation of the viral mRNAs occurs due to a stuttering mechanism, whereby the RdRp moves back and forth over this stretch of U residues, leading to the formation of a poly(A) tail [39,40]. Interestingly, NS1 inhibits the nuclear export of cellular mRNAs by preventing cellular mRNAs from being cleaved at the polyadenylation cleavage site [41]. It does this by binding to the CPSF [42] and poly(A) binding protein II (PABPII), which is involved in stimulating poly(A) polymerase to add the poly(A) tail onto newly cleaved mRNAs [43].

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Export of vRNPs from the nucleus

It is known that only negative sense vRNPs are exported from the nucleus [44]. vRNPs appear to be exported out of the nucleus via the CRM1 dependent pathway through the nuclear pores. NP has been shown to interact with CRM1 directly, although no GTP hydrolysis activity could be detected. This indicates an unusual method of export if the binding of NP to CRM1 is critical for export of the vRNPs. M1 is known to interact directly with the vRNPs through the C-terminal end of the protein. Interestingly, the N-terminal portion of the protein is known to have an NLS potentially involved in the import of the vRNPs. It has been shown that the N-terminal portion of M1 can bind to NEP, thus masking the NLS. NEP also has been shown to bind to CRM1 with the accompanying GTP hydrolysis that normally occurs in a CRM1-dependent export pathway. Therefore, it is hypothesised that M1 binds to the negative sense vRNPs, as well as binding to NEP. In turn, NEP binds to CRM1, and through this “daisy-chain” complex, the vRNPs are exported out of the nucleus [12,45,46].

Recently, live imaging has been employed to visualize the movement of vRNPs during the influenza life cycle. It has been shown that NP preferentially localizes to the apical side of infected nuclei, indicating polarized exit of the viral genome [47,48].

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Assembly and budding at the host cell’s plasma membrane

After the vRNPs have left the nucleus, all that is left for the virus to do is form viral particles and leave the cell. Since influenza is an enveloped virus, it uses the host cell’s plasma membrane to form the viral particles that leave the cell and go on to infect neighbouring cells. It is possible to create virus particles that do not contain any or only a few vRNPs, but all the viral proteins normally found within the viral lipid bilayer, i.e., HA, NA, and M2, must be present to form a viral particle [4].

Virus particles bud from the apical side of polarized cells [4]. Because of this, HA, NA, and M2 are transported to the apical plasma membrane. It has been shown through deletion and mutational analysis that the tail of M2 is extremely important in the formation of viral particles. Viruses that had the M2 tail deleted or partially mutated produced elongated particles [49]. M1, which is present underneath the lipid bilayer, is important in the final step of closing and budding off of the viral particle [6,50]. Several host factors are involved in the budding off of viruses from plasma membranes, and these are reviewed in [4,51].

There are two models that have been hypothesized to explain the packaging of viral genomic segments into virions: the random packaging model [52,53] and the specific packaging model [54]. The former predicts that viral genomic segments are randomly packaged into virions; whereas, the latter predicts that there are signals present in the viral segments dictating which segments are to be packaged into the virions. Packaging signals have been identified in the 5’ and 3’ non-coding and coding regions of some of the viral segments [55-59], thus leaning toward the specific packaging model.

One of the most important steps that must occur before the newly made viral particle can leave the plasma membrane is the cleavage of sialic acid residue from glycoproteins and glycolipids. NA removes these sialic acids. Without this process, the viral particle would not be released from the plasma membrane [60].

15

One of the bacterial toxins secreted by Clostridium perfringens, the bacteria that cause gas gangrene, is a lipase that hydrolyzes phosphocholine from phosphatidylcholine and from sphingomyelin.

The resulting lysis (breakage) of the cell membrane releases intracellular contents that provide the bacteria with nutrients for rapid growth.

These bacteria are strict anaerobes and grow only in the absence of oxygen. As their toxins lyse membranes in the endothelial cells of blood vessels, the capillaries are destroyed, and the bacteria are protected from oxygen transported by the red blood cells, antibiotics and components of the immune system carried in the blood.

Gangrene is necrosis caused by loss of blood supply.

Clostridium Perfringens

Must Know

How are nutrient or ions transported in and out of the cell

17

Importance of Membrane Transport Proteins

18

Membrane Transport Proteins

Many molecules must move back and forth from inside and outside of the cell

Most cannot pass through without the assistance of proteins in the membrane bilayer

Private passageways for select substances

Each cell has membrane has a specific set of proteins depending on the cell

Must Know

Movement of Small Molecules

Ion Concentrations

Must Know

Click to edit Master text styles

Second level

Third level

Fourth level

Fifth level

Ion Concentrations

The maintenance of solutes on both sides of the membrane is critical to the cell

Helps to keep the cell from rupturing

Concentration of ions on either side varies widely

Na+ and Cl- are higher outside the cell

K+ is higher inside the cell

Must balance the number of positive and negative charges, both inside and outside cell

Must Know

Impermeable Membranes

Ions and hydrophilic molecules cannot easily pass thru the hydrophobic membrane

Small and hydrophobic molecules can

Must know the list to the left

Must Know

Membrane Transporters

24

Classification of transporters

Ligand Gated

Must Know

Transporters

Carriers

Primary Active Transporters

Secondary active transporters

Voltage Gated

Leaky

Stress activated

Uniport

(facilitative)

Symport

Antiport

Channels

Carrier vs Channel Proteins

26

Carrier vs Channel Proteins

Must Know

Carrier vs Channel Proteins

Carrier proteins – move the solute across the membrane by binding it on one side and transporting it to the other side

Requires a conformation change.

Can be active or passive diffusion

Channel protein – small hydrophilic pores that allow for solutes to pass through

Always use PASSIVE diffusion to move across

Also called ion channels when only ions moving

Must Know

Carrier vs Channel

Channels, if open, will let solutes pass if they have the right size and charge

Trapdoor-like

Carriers require that the solute fit in the binding site

Hence carriers are specific like an enzyme and its substrate

Carriers

30

Primary Active Transport

(Understand the concept and where they are present)

31

Primary Active Transport

Primary transport use energy from ATP to actively transport a molecule across.

Na+/K+-ATPase

Ca+2 -ATPase

Gastric H+/K+-ATPase

Osteoclast H+-ATPase

P-glycoprotein (also an ATPase)

Must Know

Na/K ATPases

Primary Active transport

33

INSIDE

OUTSIDE

Na/K ATPases

Na+ ions

K+ ions

Na/K ATPase enzyme

Primary Active Transport

In Na+,K+-ATPase, the three sodium ions from one side of the cells will bind to the inside of the ATPase.

This would trigger phosphorylation of the enzyme which will change its confirmation.

This change in confirmation favors binding of 2 K ions from the other side.

This leads to rapid release of Na ions and binding of K ions to ATPases.

The binding of K ions triggers dephosphorylation lead to native state of enzyme.

Must Know

Primary Active Transport

The basic mechanism of how ATPases works in same in all.

In those when only one ion is involved such as in Ca ATPase, or Osteoclast H+-ATPase the process is triggered by high Calcium or H+ concentration, respectively, on one side of the cell.

Dephosphorylation takes place due to highly unstable form of phorphorylated enzymes.

Must Know

The Gastric H+/K+- ATPase

This enzyme is similar to Na,K-ATPase and Ca-ATPase

Must Know

37

Osteoclast H+-ATPase pump

TRANSPORT OF PROTONS out of osteoclast lowers pH of extracellular space near the bone to ~ 4

Solubilizes hydroxyapatite, bone mineral matrix

Calcium released is utilized by soft tissues such as nerves and muscles

Must Know

Bone factory- Proton Pump

Bone material undergoes ongoing remodeling

Osteoclasts tear down bone tissue

Osteoblasts build it back up

Osteoclasts function by:

Secreting acid into the space between the osteoclast membrane and the bone surface

Acid dissolves the Ca-phosphate matrix of the bone

ATP-driven proton pump in the membrane does this!

Must Know

39

P-glycoprotein

Pumps out of the cell a wide variety of drugs

Also called Multi-Drug Resistance ATPase or MDR ATPase

Found to be related to acquisition of drug resistance

MDR ATPase defeats efforts of chemotherapy

Must Know

Secondary Active Transport

41

Secondary Active Transport

In contrast to primary active transport, secondary active transport processes relies on the electrochemical gradient created by difference in concentration of ions on two sides.

Many amino acids and sugars are accumulated inside the cells driven by ion gradients

PHA3102 Biochemistry II - Dr. Santos -Q2 2014

Must Know

42

Secondary Active Transport

Must Know

FIGURE 11-33 Three general classes of transport systems. Transporters differ in the number of solutes (substrates) transported and the direction in which each solute moves. Examples of all three types of transporters are discussed in the text. Note that this classification tells us nothing about whether these are energy-requiring (active transport) or energy-independent (passive transport) processes.

Secondary Active Transport

Uniport (facilitative transporters) – movement of only one type of ions in a particular direction

Symport – two ions move in the same direction. For e.g. ions and amino acids or sugars are transported in the same direction across the membrane

Antiport - ions and transported species move in opposite directions.

PHA3102 Biochemistry II - Dr. Santos -Q2 2014

Must Know

Uniporters (facilitative transporters),

Symporters,

Antiporters,

Carrier Transporters

Must Know

Uniport

Also called as facilitative transport

Must Know

46

Glucose

Glucose Transporters

Functioning of GLUT : A model

Must Know

Functioning of GLUT : A model

FIGURE 11-31 Model of glucose transport into erythrocytes by GLUT1. The transporter exists in two conformations: T1, with the glucose-binding site exposed on the outer surface of the plasma membrane, and T2, with the binding site exposed on the inner surface. Glucose transport occurs in four steps. 1 Glucose in blood plasma binds to a stereospecific site on T1; this lowers the activation energy for 2 a conformational change from glucoseout • T1 to glucosein • T2, effecting the transmembrane passage of the glucose. 3 Glucose is released from T2 into the cytoplasm, and 4 the transporter returns to the T1 conformation, ready to transport another glucose molecule.

Functioning of GLUT : A model

The transporter exists in two conformations:

T1, -The glucose-binding site exposed on the outer surface of the plasma membrane, and

T2, - The binding site exposed on the inner surface.

Must Know

FIGURE 11-31 Model of glucose transport into erythrocytes by GLUT1. The transporter exists in two conformations: T1, with the glucose-binding site exposed on the outer surface of the plasma membrane, and T2, with the binding site exposed on the inner surface. Glucose transport occurs in four steps. 1 Glucose in blood plasma binds to a stereospecific site on T1; this lowers the activation energy for 2 a conformational change from glucoseout • T1 to glucosein • T2, effecting the transmembrane passage of the glucose. 3 Glucose is released from T2 into the cytoplasm, and 4 the transporter returns to the T1 conformation, ready to transport another glucose molecule.

Functioning of GLUT : A model

Glucose transport occurs in four steps.

Glucose in blood plasma binds to a stereospecific site on T1.

This lowers the activation energy for a conformational change from glucoseout • T1 to glucosein • T2, effecting the transmembrane passage of the glucose.

Glucose is released from T2 into the cytoplasm, and

The transporter returns to the T1 conformation, ready to transport another glucose molecule.

Must Know

FIGURE 11-31 Model of glucose transport into erythrocytes by GLUT1. The transporter exists in two conformations: T1, with the glucose-binding site exposed on the outer surface of the plasma membrane, and T2, with the binding site exposed on the inner surface. Glucose transport occurs in four steps. 1 Glucose in blood plasma binds to a stereospecific site on T1; this lowers the activation energy for 2 a conformational change from glucoseout • T1 to glucosein • T2, effecting the transmembrane passage of the glucose. 3 Glucose is released from T2 into the cytoplasm, and 4 the transporter returns to the T1 conformation, ready to transport another glucose molecule.

When glucose is high outside the cell, the insulin triggers the GLUT in open conformation to take in glucose and move it to the cytosol where the concentration is low.

When glucose levels are low in the blood, glucagon (hormone) triggers the breakdown of glycogen (e.g., from the liver), glucose levels are high in the cell and then the conformation moves the glucose out of the cell to the blood stream

Glucose moves according to the concentration gradient across the membrane.

Functioning of GLUT : A model

Must Know

Antiport

Must Know

52

HCO3-/Cl- antiport in HB/HCO3- buffer system

Must Know

53

Bicarbonate-Hemoglobin Buffer System

The bicarbonate buffer system and hemoglobin in red blood cells cooperate in buffering the blood and transporting CO2 to the lungs.

Bicarbonate-Hemoglobin Buffer System

Most of the CO2 produced from tissue metabolism in the TCA cycle diffuses into the interstitial fluid and the blood plasma and then into red blood cells.

Bicarbonate-Hemoglobin Buffer System

Most of the CO2 produced from tissue metabolism in the TCA cycle diffuses into the interstitial fluid and the blood plasma and then into red blood cells.

Bicarbonate-Hemoglobin Buffer System

Although no carbonic anhydrase can be found in blood plasma or interstitial fluid, the RBC contain high amounts of this enzyme, and CO2 is rapidly converted to H2CO3 within these cells.

Bicarbonate-Hemoglobin Buffer System

The carbonic acid dissociates to yield HCO3- and H+

Bicarbonate-Hemoglobin Buffer System

The bicarbonate anion is transported out of the red blood cells into the blood in exchange for chloride anions, and thus bicarbonate is relatively high in the plasma.

HCO3-

Cl-

HCO3-

HCO3-

Cl-

Cl-

Cl-

Cl-

HCO3-

HCO3-

Bicarbonate-Hemoglobin Buffer System

The H+ released is also buffered by combination with hemoglobin (Hb). The side chain of the amino acid histidine in hemoglobin has a pKa of 6.7 and is thus able to accept a proton.

Bicarbonate-Hemoglobin Buffer System

As the red blood cells approach the lungs, the direction of the equilibrium reverses.

Bicarbonate-Hemoglobin Buffer System

CO2 is released from the red blood cells, causing more carbonic acid to dissociate into CO2 and water and more hydrogen ions to combine with bicarbonate.

Bicarbonate-Hemoglobin Buffer System

Hemoglobin loses some of its hydrogen ions, a feature that allows it to bind oxygen more readily

Bicarbonate-Hemoglobin Buffer System

Hydrogen ions obtained from deprotonation of Hb combines with HCO3- to form H2CO3 which will further release CO2.

Must Know

Erythrocyte chloride-bicarbonate exchanger

Integral RBC membrane protein also called anion exchanger (AE) simultaneously moves HCO3- and Cl-, hence called a antiport.

Solute transport is in the direction of concentration gradient

Increases CO2 carrying capacity of blood

Increases HCO3- transport rate across RBC membrane a million fold

Must Know

FIGURE 11-32 Chloride-bicarbonate exchanger of the erythrocyte membrane. This cotransport system allows the entry and exit of HCO3– without changing the membrane potential. Its role is to increase the CO2-carrying capacity of the blood.

Na+/H+ Antiport in Hb/HCO3- buffer system

Must Know

66

H

Na

Na

Na

Na

Na

Na

Na

Na

HCO3-

Lumen

Basolateral Membrane

K+

Na/K pump

Na/H+ pump

K+ Channel

Carbonic Anhydrase

HCO3-

HCO3-

HCO3-

HCO3-

Must Know

67

H

Na

Na

Na

Na

Na

Na

Na

Na

HCO3-

Lumen

Basolateral Membrane

K+

Na/K pump

Na/H+ pump

K+ Channel

Carbonic Anhydrase

HCO3-

HCO3-

HCO3-

HCO3-

Must Know

Symport

69

Synport absorption of Amino Acids

K+

Na

Na

K+

Na

Na

Na

ÀA

ÀA

K+

Na

Na/K ATPase

Na/AA Carriers

Na ion

K Ion

Amino Acid

Facilitated

Transporter

Portal Vein

Serosal

Side

Intestinal

Lumen

Na

Must Know

Absorption of Amino Acids

Amino acids absorption from the lumen of the small intestine to the inside of the cell is driven by the low intracellular Na+ concentration.

Low intracellular Na+ results from pumping sodium out of the cell by Na+K+- ATPase on the serosal membrane

Amino acids are then transported into the cell with Na ions due to the presence of Na dependent co-transporters on the luminal side of the intestinal cells.

Must Know

Amino acids that enter the blood are transported across cell membranes of the various

tissues principally by Na-dependent cotransporters and, to a lesser extent, by

facilitated transporters (Table 37.1). In this respect, amino acid transport differs

from glucose transport, which is Na-dependent transport in the intestinal and renal

epithelium but facilitated transport in other cell types. The Na dependence of

amino acid transport in liver, muscle, and other tissues allows these cells to concentrate

amino acids from the blood. These transport proteins have a different

genetic basis, amino acid composition, and somewhat different specificity than

those in the luminal membrane of intestinal epithelia. They also differ somewhat

between tissues. For instance, the N system for glutamine uptake is present in the

liver but either not present in other tissues or present as an isoform with different

properties. There is also some overlap in specificity of the transport proteins, with

most amino acids being transported by more than one carrier.

71

Absorption of Amino Acids

Amino acids are then transported out of the cells by facilitated transporters.

At least six different facilitated transporters present with overlapping specificities.

Once in the blood, amino acids are transported to cells in various tissues via Na-dependent cotransporters.

Must Know

Amino acids that enter the blood are transported across cell membranes of the various

tissues principally by Na-dependent cotransporters and, to a lesser extent, by

facilitated transporters (Table 37.1). In this respect, amino acid transport differs

from glucose transport, which is Na-dependent transport in the intestinal and renal

epithelium but facilitated transport in other cell types. The Na dependence of

amino acid transport in liver, muscle, and other tissues allows these cells to concentrate

amino acids from the blood. These transport proteins have a different

genetic basis, amino acid composition, and somewhat different specificity than

those in the luminal membrane of intestinal epithelia. They also differ somewhat

between tissues. For instance, the N system for glutamine uptake is present in the

liver but either not present in other tissues or present as an isoform with different

properties. There is also some overlap in specificity of the transport proteins, with

most amino acids being transported by more than one carrier.

72

Carrier Proteins

Required for almost all small organic molecules

Exception – fat-soluble molecules (steroids, and thyroids) and small uncharged molecules that can pass by simple diffusion

Usually only carry one type of molecule

Carriers can also be in other membranes of the cell such as the mitochondria

Must Know

Channel Proteins

Must Know

74

Channel Proteins

Channel proteins create a hydrophilic opening in which small water-soluble molecules can pass into or out of the cell

Gap junctions and pores (as in nuclear envelope) make very large openings

Ion channels are very specific with regards to pore size and the charge on the molecule to be moved

Move mainly Na, K, Cl and Ca

Must Know

Ion Channels

Must Know

Channels Are Either Open or Closed

Must Know

Ion Channels

Have ion selectivity – allows some ions to pass and restricts others

Based on pore size and the charges on the inner ‘wall’ of the channel

Ion channels are not always open

Have the ability to regulate the movement of ions so that control can maintain the ion concentrations within the cell

Channels are gated – open or closed

Specific stimuli triggers the change in shape and opening or closing of channel

Must Know

Variety of Channels

Ion channels vary with respect to

Ion selectivity – which ions can go thru

Gating – conditions that influence opening and closing

Must Know

Membrane Ion Channels

Passive, or leakage, channels – always open under resting conditions

Chemical (or ligand)-gated channels – open with binding of a specific ligand.

Voltage-gated channels – open and close in response to changes in the membrane potential

Mechanically-gated channels – open and close in response to physical deformation of receptors

Types of plasma membrane ion channels

Must Know

80

Leakage Channels

Must Know

81

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Cardiac Cells in Resting State

K+

K+

K+

K+

K+

K+

K+

K+

K+ Channel

Cardiac Cells

Must Know

Ligand Gated Channel Proteins

Ca2+ secretion

Must Know

83

Insulin Secretion

Glucose is uptaken by GLUT2 receptors and metabolized to G-6-P, converts ADP to ATP

Depending on ATP/ADP ratio  closure of potassium channels  opening of calcium channels  release of preformed insulin granules from islet cells

84

Biosynthesis of Insulin

Insulin has a place in the biochemistry “ hall of fame” in that it was the first protein for which the chemical structure and

molecular weight were determined and was the first genetically engineered drug approved by the U.S. Food and Drug

Administration (7). The active insulin hormone is composed of a 21-amino-acid A chain and a 30-amino-acid B chain that

are linked by two disulfide bonds. Separately, each chain is biologically inactive. Insulin is initial ly synthesized as a

110-amino-acid preprohormone in the pancreatic β cells. The preprohormone then undergoes translocation through the

membrane of the rough endoplasmic reticulum. During this process, the cleavage of 24-amino-acids from the N-terminus of

the B chain occurs to produce proinsulin. Inside the rough endoplasmic reticulum, the protein folds, and the three critical

disulfide bonds form. In the Golgi complex, proinsulin undergoes additional modification that is catalyzed by calciumdependent

endopeptidases (PC2 and PC3). In this process, four basic amino acids as well as the connecting C-peptide are

removed via proteolysis (Fig. 32.1). The resulting insulin protein represents the active form of the hormone found in the

plasma. In solution, insulin can exist as a monomer, dimer, or hexamer. In the pancreas, insulin is stored in its hexameric

form. In this form, two zinc ions are coordinated per insulin hexamer. The half-life of insulin is 5 to 6 minutes, whereas the

half life of proinsulin is approximately 17 minutes (5).

Secretion of Insulin

Secretion of insulin from the pancreas is very tightly regulated. When glucose enters the β cell (GLUT-2–facilitated

transport), it is phosphorylated by glucokinase to G6P. The G6P is used to generate ATP, thereby changing the ratio of

ATP to adenosine diphosphate (ADP) and prevents an ATP-sensitive potassium channel from functioning, which in turn

leads to depolar ization of the β cells. This prompts activation of a voltage-gated calcium channel and calcium flows into the

β cells. The elevated intracellular calcium concentrations causes activation of phospholipases A2 and C, and levels of

inositol triphosphate rise (5). Inositol tr iphosphate, an intracellular second messenger , facilitates additional release of

calcium into the cytosol. The intracellular concentrations of calcium are now sufficiently high to promote insulin secretion

from the β cells. Several classes of pharmacological agents alter the regulation of insulin release. A list of these agents

and their respective effect on insulin secretion can be found in Table 32.5.

Insulin interacts with its cell surface receptor via key amino acid residues located along the N- and C- termini of the A chain

of insulin and along the carboxy terminus of the B chain of insulin (Table 32.6) . The binding of insul in occurs to amino acid

residues located within the N- and C-terminal regions of the α subunit of the receptor , which includes a cysteine-rich region

(5). Binding and activation of the insulin receptor results in a cascade of biochemical events previously descr ibed.

Insulin Secretion

Glucose is uptaken by GLUT2 receptors and metabolized to G-6-P, converts ADP to ATP

Depending on ATP/ADP ratio  closure of potassium channels  opening of calcium channels  release of preformed insulin granules from islet cells

G-6-P

85

Biosynthesis of Insulin

Insulin has a place in the biochemistry “ hall of fame” in that it was the first protein for which the chemical structure and

molecular weight were determined and was the first genetically engineered drug approved by the U.S. Food and Drug

Administration (7). The active insulin hormone is composed of a 21-amino-acid A chain and a 30-amino-acid B chain that

are linked by two disulfide bonds. Separately, each chain is biologically inactive. Insulin is initial ly synthesized as a

110-amino-acid preprohormone in the pancreatic β cells. The preprohormone then undergoes translocation through the

membrane of the rough endoplasmic reticulum. During this process, the cleavage of 24-amino-acids from the N-terminus of

the B chain occurs to produce proinsulin. Inside the rough endoplasmic reticulum, the protein folds, and the three critical

disulfide bonds form. In the Golgi complex, proinsulin undergoes additional modification that is catalyzed by calciumdependent

endopeptidases (PC2 and PC3). In this process, four basic amino acids as well as the connecting C-peptide are

removed via proteolysis (Fig. 32.1). The resulting insulin protein represents the active form of the hormone found in the

plasma. In solution, insulin can exist as a monomer, dimer, or hexamer. In the pancreas, insulin is stored in its hexameric

form. In this form, two zinc ions are coordinated per insulin hexamer. The half-life of insulin is 5 to 6 minutes, whereas the

half life of proinsulin is approximately 17 minutes (5).

Secretion of Insulin

Secretion of insulin from the pancreas is very tightly regulated. When glucose enters the β cell (GLUT-2–facilitated

transport), it is phosphorylated by glucokinase to G6P. The G6P is used to generate ATP, thereby changing the ratio of

ATP to adenosine diphosphate (ADP) and prevents an ATP-sensitive potassium channel from functioning, which in turn

leads to depolar ization of the β cells. This prompts activation of a voltage-gated calcium channel and calcium flows into the

β cells. The elevated intracellular calcium concentrations causes activation of phospholipases A2 and C, and levels of

inositol triphosphate rise (5). Inositol tr iphosphate, an intracellular second messenger , facilitates additional release of

calcium into the cytosol. The intracellular concentrations of calcium are now sufficiently high to promote insulin secretion

from the β cells. Several classes of pharmacological agents alter the regulation of insulin release. A list of these agents

and their respective effect on insulin secretion can be found in Table 32.5.

Insulin interacts with its cell surface receptor via key amino acid residues located along the N- and C- termini of the A chain

of insulin and along the carboxy terminus of the B chain of insulin (Table 32.6) . The binding of insul in occurs to amino acid

residues located within the N- and C-terminal regions of the α subunit of the receptor , which includes a cysteine-rich region

(5). Binding and activation of the insulin receptor results in a cascade of biochemical events previously descr ibed.

Insulin Secretion

Glucose is uptaken by GLUT2 receptors and metabolized to G-6-P, converts ADP to ATP

Depending on ATP/ADP ratio  closure of potassium channels  opening of calcium channels  release of preformed insulin granules from islet cells

G-6-P

86

Biosynthesis of Insulin

Insulin has a place in the biochemistry “ hall of fame” in that it was the first protein for which the chemical structure and

molecular weight were determined and was the first genetically engineered drug approved by the U.S. Food and Drug

Administration (7). The active insulin hormone is composed of a 21-amino-acid A chain and a 30-amino-acid B chain that

are linked by two disulfide bonds. Separately, each chain is biologically inactive. Insulin is initial ly synthesized as a

110-amino-acid preprohormone in the pancreatic β cells. The preprohormone then undergoes translocation through the

membrane of the rough endoplasmic reticulum. During this process, the cleavage of 24-amino-acids from the N-terminus of

the B chain occurs to produce proinsulin. Inside the rough endoplasmic reticulum, the protein folds, and the three critical

disulfide bonds form. In the Golgi complex, proinsulin undergoes additional modification that is catalyzed by calciumdependent

endopeptidases (PC2 and PC3). In this process, four basic amino acids as well as the connecting C-peptide are

removed via proteolysis (Fig. 32.1). The resulting insulin protein represents the active form of the hormone found in the

plasma. In solution, insulin can exist as a monomer, dimer, or hexamer. In the pancreas, insulin is stored in its hexameric

form. In this form, two zinc ions are coordinated per insulin hexamer. The half-life of insulin is 5 to 6 minutes, whereas the

half life of proinsulin is approximately 17 minutes (5).

Secretion of Insulin

Secretion of insulin from the pancreas is very tightly regulated. When glucose enters the β cell (GLUT-2–facilitated

transport), it is phosphorylated by glucokinase to G6P. The G6P is used to generate ATP, thereby changing the ratio of

ATP to adenosine diphosphate (ADP) and prevents an ATP-sensitive potassium channel from functioning, which in turn

leads to depolar ization of the β cells. This prompts activation of a voltage-gated calcium channel and calcium flows into the

β cells. The elevated intracellular calcium concentrations causes activation of phospholipases A2 and C, and levels of

inositol triphosphate rise (5). Inositol tr iphosphate, an intracellular second messenger , facilitates additional release of

calcium into the cytosol. The intracellular concentrations of calcium are now sufficiently high to promote insulin secretion

from the β cells. Several classes of pharmacological agents alter the regulation of insulin release. A list of these agents

and their respective effect on insulin secretion can be found in Table 32.5.

Insulin interacts with its cell surface receptor via key amino acid residues located along the N- and C- termini of the A chain

of insulin and along the carboxy terminus of the B chain of insulin (Table 32.6) . The binding of insul in occurs to amino acid

residues located within the N- and C-terminal regions of the α subunit of the receptor , which includes a cysteine-rich region

(5). Binding and activation of the insulin receptor results in a cascade of biochemical events previously descr ibed.

Insulin Secretion

Glucose is uptaken by GLUT2 receptors and metabolized to G-6-P, converts ADP to ATP

Depending on ATP/ADP ratio  closure of potassium channels  opening of calcium channels  release of preformed insulin granules from islet cells

G-6-P

87

Biosynthesis of Insulin

Insulin has a place in the biochemistry “ hall of fame” in that it was the first protein for which the chemical structure and

molecular weight were determined and was the first genetically engineered drug approved by the U.S. Food and Drug

Administration (7). The active insulin hormone is composed of a 21-amino-acid A chain and a 30-amino-acid B chain that

are linked by two disulfide bonds. Separately, each chain is biologically inactive. Insulin is initial ly synthesized as a

110-amino-acid preprohormone in the pancreatic β cells. The preprohormone then undergoes translocation through the

membrane of the rough endoplasmic reticulum. During this process, the cleavage of 24-amino-acids from the N-terminus of

the B chain occurs to produce proinsulin. Inside the rough endoplasmic reticulum, the protein folds, and the three critical

disulfide bonds form. In the Golgi complex, proinsulin undergoes additional modification that is catalyzed by calciumdependent

endopeptidases (PC2 and PC3). In this process, four basic amino acids as well as the connecting C-peptide are

removed via proteolysis (Fig. 32.1). The resulting insulin protein represents the active form of the hormone found in the

plasma. In solution, insulin can exist as a monomer, dimer, or hexamer. In the pancreas, insulin is stored in its hexameric

form. In this form, two zinc ions are coordinated per insulin hexamer. The half-life of insulin is 5 to 6 minutes, whereas the

half life of proinsulin is approximately 17 minutes (5).

Secretion of Insulin

Secretion of insulin from the pancreas is very tightly regulated. When glucose enters the β cell (GLUT-2–facilitated

transport), it is phosphorylated by glucokinase to G6P. The G6P is used to generate ATP, thereby changing the ratio of

ATP to adenosine diphosphate (ADP) and prevents an ATP-sensitive potassium channel from functioning, which in turn

leads to depolar ization of the β cells. This prompts activation of a voltage-gated calcium channel and calcium flows into the

β cells. The elevated intracellular calcium concentrations causes activation of phospholipases A2 and C, and levels of

inositol triphosphate rise (5). Inositol tr iphosphate, an intracellular second messenger , facilitates additional release of

calcium into the cytosol. The intracellular concentrations of calcium are now sufficiently high to promote insulin secretion

from the β cells. Several classes of pharmacological agents alter the regulation of insulin release. A list of these agents

and their respective effect on insulin secretion can be found in Table 32.5.

Insulin interacts with its cell surface receptor via key amino acid residues located along the N- and C- termini of the A chain

of insulin and along the carboxy terminus of the B chain of insulin (Table 32.6) . The binding of insul in occurs to amino acid

residues located within the N- and C-terminal regions of the α subunit of the receptor , which includes a cysteine-rich region

(5). Binding and activation of the insulin receptor results in a cascade of biochemical events previously descr ibed.

Insulin Secretion

Glucose is uptaken by GLUT2 receptors and metabolized to G-6-P, converts ADP to ATP

Depending on ATP/ADP ratio  closure of potassium channels  opening of calcium channels  release of preformed insulin granules from islet cells

G-6-P

88

Biosynthesis of Insulin

Insulin has a place in the biochemistry “ hall of fame” in that it was the first protein for which the chemical structure and

molecular weight were determined and was the first genetically engineered drug approved by the U.S. Food and Drug

Administration (7). The active insulin hormone is composed of a 21-amino-acid A chain and a 30-amino-acid B chain that

are linked by two disulfide bonds. Separately, each chain is biologically inactive. Insulin is initial ly synthesized as a

110-amino-acid preprohormone in the pancreatic β cells. The preprohormone then undergoes translocation through the

membrane of the rough endoplasmic reticulum. During this process, the cleavage of 24-amino-acids from the N-terminus of

the B chain occurs to produce proinsulin. Inside the rough endoplasmic reticulum, the protein folds, and the three critical

disulfide bonds form. In the Golgi complex, proinsulin undergoes additional modification that is catalyzed by calciumdependent

endopeptidases (PC2 and PC3). In this process, four basic amino acids as well as the connecting C-peptide are

removed via proteolysis (Fig. 32.1). The resulting insulin protein represents the active form of the hormone found in the

plasma. In solution, insulin can exist as a monomer, dimer, or hexamer. In the pancreas, insulin is stored in its hexameric

form. In this form, two zinc ions are coordinated per insulin hexamer. The half-life of insulin is 5 to 6 minutes, whereas the

half life of proinsulin is approximately 17 minutes (5).

Secretion of Insulin

Secretion of insulin from the pancreas is very tightly regulated. When glucose enters the β cell (GLUT-2–facilitated

transport), it is phosphorylated by glucokinase to G6P. The G6P is used to generate ATP, thereby changing the ratio of

ATP to adenosine diphosphate (ADP) and prevents an ATP-sensitive potassium channel from functioning, which in turn

leads to depolar ization of the β cells. This prompts activation of a voltage-gated calcium channel and calcium flows into the

β cells. The elevated intracellular calcium concentrations causes activation of phospholipases A2 and C, and levels of

inositol triphosphate rise (5). Inositol tr iphosphate, an intracellular second messenger , facilitates additional release of

calcium into the cytosol. The intracellular concentrations of calcium are now sufficiently high to promote insulin secretion

from the β cells. Several classes of pharmacological agents alter the regulation of insulin release. A list of these agents

and their respective effect on insulin secretion can be found in Table 32.5.

Insulin interacts with its cell surface receptor via key amino acid residues located along the N- and C- termini of the A chain

of insulin and along the carboxy terminus of the B chain of insulin (Table 32.6) . The binding of insul in occurs to amino acid

residues located within the N- and C-terminal regions of the α subunit of the receptor , which includes a cysteine-rich region

(5). Binding and activation of the insulin receptor results in a cascade of biochemical events previously descr ibed.

Insulin Secretion

Glucose is uptaken by GLUT2 receptors and metabolized to G-6-P, converts ADP to ATP

Depending on ATP/ADP ratio  closure of potassium channels  opening of calcium channels  release of preformed insulin granules from islet cells

G-6-P

89

Biosynthesis of Insulin

Insulin has a place in the biochemistry “ hall of fame” in that it was the first protein for which the chemical structure and

molecular weight were determined and was the first genetically engineered drug approved by the U.S. Food and Drug

Administration (7). The active insulin hormone is composed of a 21-amino-acid A chain and a 30-amino-acid B chain that

are linked by two disulfide bonds. Separately, each chain is biologically inactive. Insulin is initial ly synthesized as a

110-amino-acid preprohormone in the pancreatic β cells. The preprohormone then undergoes translocation through the

membrane of the rough endoplasmic reticulum. During this process, the cleavage of 24-amino-acids from the N-terminus of

the B chain occurs to produce proinsulin. Inside the rough endoplasmic reticulum, the protein folds, and the three critical

disulfide bonds form. In the Golgi complex, proinsulin undergoes additional modification that is catalyzed by calciumdependent

endopeptidases (PC2 and PC3). In this process, four basic amino acids as well as the connecting C-peptide are

removed via proteolysis (Fig. 32.1). The resulting insulin protein represents the active form of the hormone found in the

plasma. In solution, insulin can exist as a monomer, dimer, or hexamer. In the pancreas, insulin is stored in its hexameric

form. In this form, two zinc ions are coordinated per insulin hexamer. The half-life of insulin is 5 to 6 minutes, whereas the

half life of proinsulin is approximately 17 minutes (5).

Secretion of Insulin

Secretion of insulin from the pancreas is very tightly regulated. When glucose enters the β cell (GLUT-2–facilitated

transport), it is phosphorylated by glucokinase to G6P. The G6P is used to generate ATP, thereby changing the ratio of

ATP to adenosine diphosphate (ADP) and prevents an ATP-sensitive potassium channel from functioning, which in turn

leads to depolar ization of the β cells. This prompts activation of a voltage-gated calcium channel and calcium flows into the

β cells. The elevated intracellular calcium concentrations causes activation of phospholipases A2 and C, and levels of

inositol triphosphate rise (5). Inositol tr iphosphate, an intracellular second messenger , facilitates additional release of

calcium into the cytosol. The intracellular concentrations of calcium are now sufficiently high to promote insulin secretion

from the β cells. Several classes of pharmacological agents alter the regulation of insulin release. A list of these agents

and their respective effect on insulin secretion can be found in Table 32.5.

Insulin interacts with its cell surface receptor via key amino acid residues located along the N- and C- termini of the A chain

of insulin and along the carboxy terminus of the B chain of insulin (Table 32.6) . The binding of insul in occurs to amino acid

residues located within the N- and C-terminal regions of the α subunit of the receptor , which includes a cysteine-rich region

(5). Binding and activation of the insulin receptor results in a cascade of biochemical events previously descr ibed.

Insulin Secretion

G-6-P

Glucose is uptaken by GLUT2 receptors and metabolized to G-6-P, converts ADP to ATP

Depending on ATP/ADP ratio  closure of potassium channels  opening of calcium channels  release of preformed insulin granules from islet cells

90

Biosynthesis of Insulin

Insulin has a place in the biochemistry “ hall of fame” in that it was the first protein for which the chemical structure and

molecular weight were determined and was the first genetically engineered drug approved by the U.S. Food and Drug

Administration (7). The active insulin hormone is composed of a 21-amino-acid A chain and a 30-amino-acid B chain that

are linked by two disulfide bonds. Separately, each chain is biologically inactive. Insulin is initial ly synthesized as a

110-amino-acid preprohormone in the pancreatic β cells. The preprohormone then undergoes translocation through the

membrane of the rough endoplasmic reticulum. During this process, the cleavage of 24-amino-acids from the N-terminus of

the B chain occurs to produce proinsulin. Inside the rough endoplasmic reticulum, the protein folds, and the three critical

disulfide bonds form. In the Golgi complex, proinsulin undergoes additional modification that is catalyzed by calciumdependent

endopeptidases (PC2 and PC3). In this process, four basic amino acids as well as the connecting C-peptide are

removed via proteolysis (Fig. 32.1). The resulting insulin protein represents the active form of the hormone found in the

plasma. In solution, insulin can exist as a monomer, dimer, or hexamer. In the pancreas, insulin is stored in its hexameric

form. In this form, two zinc ions are coordinated per insulin hexamer. The half-life of insulin is 5 to 6 minutes, whereas the

half life of proinsulin is approximately 17 minutes (5).

Secretion of Insulin

Secretion of insulin from the pancreas is very tightly regulated. When glucose enters the β cell (GLUT-2–facilitated

transport), it is phosphorylated by glucokinase to G6P. The G6P is used to generate ATP, thereby changing the ratio of

ATP to adenosine diphosphate (ADP) and prevents an ATP-sensitive potassium channel from functioning, which in turn

leads to depolar ization of the β cells. This prompts activation of a voltage-gated calcium channel and calcium flows into the

β cells. The elevated intracellular calcium concentrations causes activation of phospholipases A2 and C, and levels of

inositol triphosphate rise (5). Inositol tr iphosphate, an intracellular second messenger , facilitates additional release of

calcium into the cytosol. The intracellular concentrations of calcium are now sufficiently high to promote insulin secretion

from the β cells. Several classes of pharmacological agents alter the regulation of insulin release. A list of these agents

and their respective effect on insulin secretion can be found in Table 32.5.

Insulin interacts with its cell surface receptor via key amino acid residues located along the N- and C- termini of the A chain

of insulin and along the carboxy terminus of the B chain of insulin (Table 32.6) . The binding of insul in occurs to amino acid

residues located within the N- and C-terminal regions of the α subunit of the receptor , which includes a cysteine-rich region

(5). Binding and activation of the insulin receptor results in a cascade of biochemical events previously descr ibed.

Insulin Secretion

Glucose is uptaken by GLUT2 receptors and metabolized to G-6-P, converts ADP to ATP

Depending on ATP/ADP ratio  closure of potassium channels  opening of calcium channels  release of preformed insulin granules from islet cells

G-6-P

Must Know

91

Biosynthesis of Insulin

Insulin has a place in the biochemistry “ hall of fame” in that it was the first protein for which the chemical structure and

molecular weight were determined and was the first genetically engineered drug approved by the U.S. Food and Drug

Administration (7). The active insulin hormone is composed of a 21-amino-acid A chain and a 30-amino-acid B chain that

are linked by two disulfide bonds. Separately, each chain is biologically inactive. Insulin is initial ly synthesized as a

110-amino-acid preprohormone in the pancreatic β cells. The preprohormone then undergoes translocation through the

membrane of the rough endoplasmic reticulum. During this process, the cleavage of 24-amino-acids from the N-terminus of

the B chain occurs to produce proinsulin. Inside the rough endoplasmic reticulum, the protein folds, and the three critical

disulfide bonds form. In the Golgi complex, proinsulin undergoes additional modification that is catalyzed by calciumdependent

endopeptidases (PC2 and PC3). In this process, four basic amino acids as well as the connecting C-peptide are

removed via proteolysis (Fig. 32.1). The resulting insulin protein represents the active form of the hormone found in the

plasma. In solution, insulin can exist as a monomer, dimer, or hexamer. In the pancreas, insulin is stored in its hexameric

form. In this form, two zinc ions are coordinated per insulin hexamer. The half-life of insulin is 5 to 6 minutes, whereas the

half life of proinsulin is approximately 17 minutes (5).

Secretion of Insulin

Secretion of insulin from the pancreas is very tightly regulated. When glucose enters the β cell (GLUT-2–facilitated

transport), it is phosphorylated by glucokinase to G6P. The G6P is used to generate ATP, thereby changing the ratio of

ATP to adenosine diphosphate (ADP) and prevents an ATP-sensitive potassium channel from functioning, which in turn

leads to depolar ization of the β cells. This prompts activation of a voltage-gated calcium channel and calcium flows into the

β cells. The elevated intracellular calcium concentrations causes activation of phospholipases A2 and C, and levels of

inositol triphosphate rise (5). Inositol tr iphosphate, an intracellular second messenger , facilitates additional release of

calcium into the cytosol. The intracellular concentrations of calcium are now sufficiently high to promote insulin secretion

from the β cells. Several classes of pharmacological agents alter the regulation of insulin release. A list of these agents

and their respective effect on insulin secretion can be found in Table 32.5.

Insulin interacts with its cell surface receptor via key amino acid residues located along the N- and C- termini of the A chain

of insulin and along the carboxy terminus of the B chain of insulin (Table 32.6) . The binding of insul in occurs to amino acid

residues located within the N- and C-terminal regions of the α subunit of the receptor , which includes a cysteine-rich region

(5). Binding and activation of the insulin receptor results in a cascade of biochemical events previously descr ibed.

Ligand Gated Channel Proteins

Cl- secretetion

Must Know

92

Mechanism of Chloride Transport

H2O

H2O

Must Know

Mechanism of Chloride Transport

Activation of cAMP will lead to phosphorylation of CFTR.

CFTR phosphorylation will trigger the opening of chloride channels

To maintain the electrical neutrality Na and water follows through paracellular route.

Must Know

Case 1

A patient comes to the ER with the episodes of vomiting and watery diarrhea. He was severely dehydrated, with a severe drop in blood pressure related to fluid losses. He was diagnosed with cholera, caused by the bacteria Vibrio cholerae.

What is the mechanism of water, Na+, and Cl- loss in cholera.

Mechanism of Chloride Transport

Voltage Gated Channel Proteins

97

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

K+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Ca++

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Action Potential in Non Pacemaker Cells

K+

K+

K+

K+

K+

K+

K+

K+

K+ Channel

Cardiac Cells

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+

Na+ surge due to action potential in neighboring cells

K+

K+

K+

K+

K+

K+

ms

mV

-100

-50

0

Must Know

Case 2

In a movie a person X tries to kill person Y by giving him a lethal dose of potassium chloride. Increase in potassium will cause membrane depolarization and increasing the refractory period and the delaying the action potential.

Potassium chloride is a salt so how is it transported across the membrane.

Ans:

Increase in potassium ions outside the cells will decrease the tendency of potassium to leak out of the cells causing membrane depolarization.

This will eventually delay the action potential

Voltage-Gated Channels

Move impulses along the nerve

Have voltage sensors that are sensitive to changes in membrane potential

Allows for changes in the charge across the membrane

Distribution of ions gives rise to membrane potential

Must Know

Stress Activated Channel Proteins

Must Know

101

Auditory Hair Cells

Stress activated

The sound waves cause the stereocilia to TILT and this causes the channels to open and transport signal to the brain

Hair cells to auditory nerve to brain

Must Know

3 Types of Channels

Voltage-gated channels – controlled by membrane potential

Ligand-gated channels – controlled by binding of a ligand to a membrane protein (either on the outside or the inside)

Stress activated channel – controlled by mechanical force on the cell

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