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Medical



원핵세포와 진핵세포의 차이 ( Prokaryote versus eukaryote )

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Prokaryote versus eukaryote



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One believes that a single, common universal ancestor of all life was a prokaryotic cell. Prokaryotes were the only life-forms for billions of years. As a consequence of evolution in different environments the prokaryotes have evolved to become more genetically and physically diverse, adapted to different styles of life. Prokaryotes consist of two domains – Bacteria and Archaea.


Eukaryotes are more complex than prokaryotes and are (hypothetically) created when prokaryotes fused (endosymbiosis). Prokaryotes have evolved a multitude of metabolic strategies and are found in a wide range of habitats, including conditions that most other organisms (Eukaryotes) fail to survive.


In contrast to most eukaryotes prokaryotes reproduce asexually. While sexual reproduction in eukaryotes result in an offspring with a genetic material that is a mixture of the parents’ genome, a prokaryote will reproduce clones of itself. During reproduction the eukaryotes generate genetic variation by sexual recombination. Genetic variation mechanisms of prokaryotes are not tied to reproduction. One genetic variation mechanism that almost doesn’t exist among eukaryotes is horizontal gene transfer.


Prokaryotes are generally smaller than eukaryotes. The smallness has, among other things, consequences for growth rates and generation times. Diffusion limitation generally restricts the maximal size of prokaryotic cells. Because of the asexual reproduction and short generation time relative to larger organisms, prokaryotes pass the genome rapidly on to subsequent generations. Therefore genetically changed genomes are also rapidly transferred. And therefore prokaryotes swiftly adapt and colonize new niches and a wide range of habitats.


Prokaryotes are one-celled and often live in clusters or colonies. Prokaryote species live among and interact with other species in communities and consortia. The microenvironment and the interactions hold important selection pressures which affect the evolution of the prokaryotes.



































































































  Prokaryotic cell Eukaryotic cell
Domain Bacteria Archaea Eukarya
Diversity Prokaryotes are more diverse than eukaryotes
Complexity Prokaryotes are less complex than eukaryotes
Genetic variation mechanisms Asexual. Produce clones. May transfer genetic material horizontally. Sexual recombination
Organisation Uni-cellular Uni-cellular or multicellular
Diameter (micrometer) The smallest 0,1
The largest >50
Typically between 2-200
Movement Flagellum Cytoskeleton
Cell division Binary fission Mitotic spindle
Electron acceptor Oxygen or other compounds Oxygen
Major structures Nucleoid , cell wall, cytoplasmic membrane, ribosomes, inclusions Organelles, nucleus. Otherwise the same basic elements of a prokaryote
Membrane-enclosed organelles Absent Present
Peptidoglycan in cell wall Present Absent
Antibiotic sensitivity Growth inhibited by streptomycin & chloramphenicol Not inhibited by these antibiotics
Membrane lipids Unbranched hydrocarbons Some branced hybrocarbons Unbranched hybrocarbons
Species that survive above 65°C Yes No
Genetic material Often only one, circular chromosome and small amounts of extrachromosomal DNA arranged in (usually circular) plasmids Several, linear chromosomes
Introns
(noncoding parts of genes)
Absent Present in some genes Present
Typical number of gene copies Haploid → Genotype reflects phenotype. Diploid or multiploid → Recessive genes are not expressed and hence “hidden” from selection pressure.
Location of chromosomes Cytoplasma Nucleus
Location of RNA synthesis Cytoplasma Nucleus
Location of protein synthesis Cytoplasma
RNA polymerase One kind Several kinds
Initiator amino acid for start of protein synthesis Formyl-methionine Methionine


Electronegativities of the elements

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Electronegativities of the elements














































































































































































→ Atomic radius decreases → Ionization energy increases → Electronegativity increases →
Group (vertical) 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18
Period (horizontal)
1 H
2.20
He
 
2 Li
0.98
Be
1.57
B
2.04
C
2.55
N
3.04
O
3.44
F
3.98
Ne
 
3 Na
0.93
Mg
1.31
Al
1.61
Si
1.90
P
2.19
S
2.58
Cl
3.16
Ar
 
4 K
0.82
Ca
1.00
Sc
1.36
Ti
1.54
V
1.63
Cr
1.66
Mn
1.55
Fe
1.83
Co
1.88
Ni
1.91
Cu
1.90
Zn
1.65
Ga
1.81
Ge
2.01
As
2.18
Se
2.55
Br
2.96
Kr
3.00
5 Rb
0.82
Sr
0.95
Y
1.22
Zr
1.33
Nb
1.6
Mo
2.16
Tc
1.9
Ru
2.2
Rh
2.28
Pd
2.20
Ag
1.93
Cd
1.69
In
1.78
Sn
1.96
Sb
2.05
Te
2.1
I
2.66
Xe
2.67
6 Cs
0.79
Ba
0.89
*
 
Hf
1.3
Ta
1.5
W
2.36
Re
1.9
Os
2.2
Ir
2.20
Pt
2.28
Au
2.54
Hg
2.00
Tl
1.62
Pb
2.33
Bi
2.02
Po
2.0
At
2.2
Rn
 
7 Fr
0.7
Ra
0.9
**
 
Rf
 
Db
 
Sg
 
Bh
 
Hs
 
Mt
 
Ds
 
Rg
 
Uub
 
Uut
 
Uuq
 
Uup
 
Uuh
 
Uus
 
Uuo
 
Lanthanides *
 
La
1.1
Ce
1.12
Pr
1.13
Nd
1.14
Pm
1.13
Sm
1.17
Eu
1.2
Gd
1.2
Tb
1.1
Dy
1.22
Ho
1.23
Er
1.24
Tm
1.25
Yb
1.1
Lu
1.27
Actinides **
 
Ac
1.1
Th
1.3
Pa
1.5
U
1.38
Np
1.36
Pu
1.28
Am
1.13
Cm
1.28
Bk
1.3
Cf
1.3
Es
1.3
Fm
1.3
Md
1.3
No
1.3
Lr
 

Periodic table of electronegativity using the Pauling scale

See also Periodic table

Chemical polarity

No Comments Filed Under: Medical

Chemical polarity


 



Polarity refers to the dipole-dipole intermolecular forces between the slightly positively-charged end of one molecule to the negative end of another or the same molecule. Molecular polarity is dependent on the difference in electronegativity between atoms in a compound and the asymmetry of the compound’s structure. For example, water is thought to be polar because of the uneven sharing of its electrons. However, methane is considered non-polar because the carbon shares the hydrogen molecules uniformally.


 


Theory


 




Diagram showing the net effect of symmetrical polar bonds (direction of yellow arrows show the migration of electrons) within boron trifluoride cancelling out to give a net polarity of zero. δ- shows an increase in negative charge and δ+ shows an increase in positive charge.

Electrons are not always shared equally between two bonding atoms: one atom might exert more of a force on the electron cloud than the other. This “pull” is termed electronegativity and measures the attraction for electrons a particular atom has. The unequal sharing of electrons within a bond leads to the formation of an electric dipole: a separation of positive and negative electric charge.


Atoms with high electronegativities - such as fluorine, oxygen, and nitrogen - exert a greater pull on electrons than atoms with lower electronegativities. In a bonding situation this can lead to unequal sharing of electrons between atoms as electrons will spend more time closer to the atom with the higher electronegativity.


Bonds can fall between one of two extremes - being completely non-polar or completely polar. A completely non-polar bond occurs when the electronegativities are identical and therefore possess a difference of zero. A completely polar bond is more correctly termed ionic bonding and occurs when the difference between electronegativities is large enough that one atom takes an electron from the other. The terms “polar” and “non-polar” bonds usually refer to covalent bonds. To determine the polarity of a covalent bond using numerical means, the difference between the electronegativity of the atoms is taken. If the result is between 0.5 and 2 then, generally, the bond is polar


 


 




A commonly-used example of a polar compound is water (H2O). The electrons of water’s hydrogen atoms are strongly attracted to the oxygen atom, and are actually closer to oxygen’s nucleus than to the hydrogen nuclei; thus, water has a relatively strong negative charge in the middle (red shade), and a positive charge at the ends (blue shade).

 


[edit] Polarity of molecules


A compound is composed of one or more chemical bonds between different atoms. The polarity of each bond within the compound may determine the overall polarity of the compound: how polar or non-polar it is.


A polar molecule may be polar as a result of polar bonds or as a result of an asymmetric arrangement of non-polar bonds and non bonding pairs of electrons.


Example 1. A polar molecule by virtue of polar bonds (bonds which have unequal sharing of electrons between the two atoms involved in bonding), e.g hydrogen fluoride, HF, where the bonding pair of electron is displaced towards the more electronegative fluorine atom.


Example 2. In ammonia, NH3, the three N-H bonds have only a slight polarity (towards the more electronegative nitrogen atom), however the lone pair of electrons (pointing towards the fourth apex of the approximate tetrahedron, (VSEPR) is electron rich and results in a powerful dipole across the whole ammonia molecule.


A non-polar compound may be non polar because there is (almost) no polarity in the bonds or because of the symmetrical arrangement of polar bonds.


Example 3. Methane, CH4 The four C-H bonds, arranged tetrahedrally around the carbon atom, has very little polarity in the bonds and so there is no dipole in the molecule.


Example 4. BF3, boron trifluoride has a trigonal planar arrangement of three polar bonds at 120o This results in no overall dipole in the molecule.



[edit] Properties and examples


While molecules can be described as “polar,” “non-polar,” or “semi-polar,” it must be noted that this is often a relative term, with one molecule simply being more polar or more non-polar than another. As such, there are no ultimate properties which can be ascribed to polar or non-polar molecules. However, the following properties are typical of such molecules.



[edit] Polar molecules


Examples of household polar molecules include ammonia and sugar (glucose). Polar molecules are generally able to dissolve in water (hydrophilic) due to the polar nature of water. Polar molecules have slightly positive and slightly negatively charged ends.



[edit] Non-polar molecules


Examples of household non-polar compounds include fats, oil and petrol. Most non-polar molecules are water insoluble (hydrophobic) at room temperature. However many non-polar organic solvents, such as turpentine, are able to dissolve non-polar substances - like dissolves like. Also a non-polar compound occurs when there is an equal sharing of electrons between two atoms.


When comparing a polar and non-polar molecule with similar molar masses, the polar molecule generally has a higher boiling point, because of the dipole-dipole interaction between their molecules.



[edit] Predicting molecule polarity







































Formula Description Example
Polar AB Linear Molecules CO
HAx Molecules with a single H HCl
AxOH Molecules with an OH at one end C2H5OH
OxAy Molecules with an O at one end H2O
NxAy Molecules with an N at one end NH3
Nonpolar Ax All elements O2
CxAy Most carbon compounds CO2



[edit] Electronegativity difference predictions


Non-polar covalent bond: 0.0-0.4


Slightly polar bond: 0.5-0.9


Moderately polar bond: 1-1.3


Highly polar bond: 1.4-1.7


Slightly ionic bond: 1.8-2.2


Ionic Bond: 2.3+



[edit] See also



  • Solubility
  • Emulsion
  • Detergent
  • Dipole
  • Covalent bond
  • Electronegativity
  • Dielectric
  • Chemical bonding

Ionic bond

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Ionic bond



From Wikipedia, the free encyclopedia



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Sodium and chlorine bonding ionically to form sodium chloride. Sodium loses its outer electron endothermically to give it a noble gas electron configuration, and this electron enters the chlorine atom exothermically. The oppositely charged ions are then attracted to each other, and their bonding releases energy. The net transfer of energy is that energy leaves the atoms, so the reaction is able to take place.


An ionic bond (or electrovalent bond) is a type of chemical bond that can often form between metal and non-metal ions (or polyatomic ions such as ammonium) through electrostatic attraction.


The metal donates one or more electrons, forming a positively charged ion or cation with a stable electron configuration. These electrons then enter the non metal, causing it to form a negatively charged ion or anion which also has a stable electron configuration. The electrostatic attraction between the oppositely charged ions causes them to come together and form a bond.


For example, common table salt is made of sodium chloride. In the ionic bonding, the sodium (Na) loses one electron, forming a cation, and the chlorine (Cl) gains an electron to form an anion. These ions are then attracted to each other in a 1:1 ratio to form sodium chloride (NaCl).



Na+ + Cl- → NaCl




Electron configurations of lithium and fluorine. Lithium has one electron in its outer shell, held rather loosely because the ionization energy is low. Fluorine carries 7 electrons in its outer shell. When one electron moves from lithium to fluorine, each ion acquires the noble gas configuration. The bonding energy from the electrostatic attraction of the two oppositely-charged ions has a large enough negative value that the overall bonded state energy is lower than the unbonded state

The removal of electrons from the atoms is endothermic and causes the ions to have a higher energy. There may also be energy changes associated with breaking of existing bonds or the addition of more than one electron to form anions. However, the attraction of the ions to each other lowers their energy.


Ionic bonding will occur only if the overall energy change for the reaction is favourable – when the bonded atoms have a lower energy than the free ones. The larger the resulting energy change the stronger the bond. The low electronegativity of metals and high electronegativity of non-metals means that the energy change of the reaction is most favorable when metals lose electrons and non-metals gain electrons.


Pure ionic bonding is not known to exist. All ionic bonds have a degree of covalent bonding or metallic bonding. The larger the difference in electronegativity between two atoms, the more ionic the bond. Ionic compounds conduct electricity when molten or in solution. They generally have a high melting point and tend to be soluble in water.







Contents

[hide]


  • 1 Polarization effects
  • 2 Ionic structure
  • 3 Ionic versus covalent bonds
  • 4 Electrical conductivity
  • 5 Substances in ionic form
  • 6 See also
  • 7 External links


[edit] Polarization effects


Ions in crystal lattices of purely ionic compounds are spherical; however, if the positive ion is small and/or highly charged, it will distort the electron cloud of the negative ion. This polarization of the negative ion leads to a build-up of extra charge density between the two nuclei, i.e., to partial covalency. Larger negative ions are more easily polarized, but the effect is usually only important when positive ions with charges of 3+ (e.g., Al3+) are involved (e.g., pure AlCl3 is a covalent molecule). However, 2+ ions (Be2+) or even 1+ (Li+) show some polarizing power because their sizes are so small (e.g., LiI is ionic but has some covalent bonding present).



[edit] Ionic structure


Ionic compounds in the solid state form a continuous ionic lattice structure in an ionic crystal. The simplest form of ionic crystal is a simple cubic. This is as if all the atoms were placed at the corners of a cube. This unit cell has a weight that is the same as 1 of the atoms involved. When all the ions are approximately the same size, they can form a different structure called a face-centered cubic (where the weight is 4 * atomic weight), but, when the ions are different sizes, the structure is often body-centered cubic (2 times the weight). In ionic lattices the coordination number refers to the number of connected ions.



[edit] Ionic versus covalent bonds


In an ionic bond, the atoms are bound by attraction of opposite ions, whereas, in a covalent bond, atoms are bound by sharing electrons. In covalent bonding, the molecular geometry around each atom is determined by VSEPR rules, whereas, in ionic materials, the geometry follows maximum packing rules.



[edit] Electrical conductivity




Main article: Electrolyte

Ionic substances in solution conduct electricity because the ions are free to move and carry the electrical charge from the anode to the cathode. Ionic substances conduct electricity when molten because atoms (and thus the electrons) are mobilised. Electrons can flow directly through the ionic substance in a molten state.



[edit] Substances in ionic form

























































































































































































Common Cations
Stock System Name Formula Historic Name
Simple Cations
Aluminium Al3+
Barium Ba2+
Beryllium Be2+
Caesium Cs+
Calcium Ca2+
Chromium(II) Cr2+ Chromous
Chromium(III) Cr3+ Chromic
Chromium(VI) Cr6+ Chromyl
Cobalt(II) Co2+ Cobaltous
Cobalt(III) Co3+ Cobaltic
Copper(I) Cu+ Cuprous
Copper(II) Cu2+ Cupric
Copper(III) Cu3+
Gallium Ga3+
Gold(I) Au+
Gold(III) Au3+
Helium He2+ (Alpha particle)
Hydrogen H+ (Proton)
Iron(II) Fe2+ Ferrous
Iron(III) Fe3+ Ferric
Lead(II) Pb2+ Plumbous
Lead(IV) Pb4+ Plumbic
Lithium Li+
Magnesium Mg2+
Manganese(II) Mn2+ Manganous
Manganese(III) Mn3+ Manganic
Manganese(IV) Mn4+ Manganyl
Manganese(VII) Mn7+
Mercury(II) Hg2+ Mercuric
Nickel(II) Ni2+ Nickelous
Nickel(III) Ni3+ Nickelic
Potassium K+
Silver Ag+
Sodium Na+
Strontium Sr2+
Tin(II) Sn2+ Stannous
Tin(IV) Sn4+ Stannic
Zinc Zn2+
Polyatomic Cations
Ammonium NH4+
Hydronium H3O+
Nitronium NO2+
Mercury(I) Hg22+ Mercurous















































































































































































































Common Anions
Formal Name Formula Alt. Name
Simple Anions
Arsenide As3−
Azide N3−
Bromide Br−
Chloride Cl−
Fluoride F−
Hydride H−
Iodide I−
Nitride N3−
Oxide O2−
Phosphide P3−
Sulphide S2−
Peroxide O22−
Oxoanions
Arsenate AsO43−
Arsenite AsO33−
Borate BO33−
Bromate BrO3−
Hypobromite BrO−
Carbonate CO32−
Hydrogen Carbonate HCO3− Bicarbonate
Chlorate ClO3−
Perchlorate ClO4−
Chlorite ClO2−
Hypochlorite ClO−
Chromate CrO42−
Dichromate Cr2O72−
Iodate IO3−
Nitrate NO3−
Nitrite NO2−
Phosphate PO43−
Hydrogen Phosphate HPO42−
Dihydrogen Phosphate H2PO4−
Permanganate MnO4−
Phosphite PO33−
Sulphate SO42−
Thiosulphate S2O32−
Hydrogen Sulphate HSO4− Bisulphate
Sulphite SO32−
Hydrogen Sulphite HSO3− Bisulphite
Anions from Organic Acids
Acetate C2H3O2−
Formate HCO2−
Oxalate C2O42−
Hydrogen Oxalate HC2O4− Bioxalate
Other Anions
Hydrogen Sulphide HS− Bisulphide
Telluride Te2−
Amide NH2−
Cyanate OCN−
Thiocyanate SCN−
Cyanide CN−


[edit] See also



  • Chemical bond
  • Covalent bond
  • Linear combination of atomic orbitals
  • Metallic bonding
  • Hybridisation
  • Hydrogen bond
  • Noncovalent bonding
  • Disulfide bond
  • Chemical polarity
  • Polyatomic ion

Cyclooxygenase (COX)

No Comments Filed Under: Medical


 


Cyclooxygenase (COX) is an enzyme (EC 1.14.99.1) that is responsible for formation of important biological mediators called prostanoids (including prostaglandins, prostacyclin and thromboxane). Pharmacological inhibition of COX can provide relief from the symptoms of inflammation and pain; this is the method of action of well-known drugs such as aspirin and ibuprofen.







Contents

[hide]


  • 1 Physiology
  • 2 Pharmacology

    • 2.1 Classical NSAIDs
    • 2.2 Newer NSAIDs
    • 2.3 Non-NSAID COX inhibition
    • 2.4 Cardiovascular side effects of COX inhibitors

  • 3 References
  • 4 Further reading
  • 5 See also
  • 6 External links


[edit] Physiology


See also prostaglandin and eicosanoid for more details


COX converts arachidonic acid (AA, an ω-6 PUFA) to prostaglandin H2 (PGH2), the precursor of the series-2 prostanoids. The enzyme contains two active sites: a heme with peroxidase activity, responsible for the reduction of PGG2 to PGH2, and a cyclooxygenase site, where arachidonic acid is converted into the hydroperoxy endoperoxide prostaglandin G2 (PGG2). The reaction proceeds through H atom abstraction from arachidonic acid by a tyrosine radical generated by the peroxidase active site. Two O2 molecules then react with the arachidonic acid radical, yielding PGG2.


Currently three COX isoenzymes are known—COX-1, COX-2 and COX-3. COX-3 is a splice variant of COX-1 which retains intron one and has a frameshift mutation, thus some prefer the name COX-1b or COX-1 variant (COX-1v).[1]


Different tissues express varying levels of COX-1 and COX-2. Although both enzymes act basically in the same fashion, selective inhibition can make a difference in terms of side-effects. COX-1 is considered a constitutive enzyme, being found in most mammalian cells. More recently it has been shown to be upregulated in various carcinomas and to have a central role in tumorigenesis. COX-2, on the other hand, is undetectable in most normal tissues. It is an inducible enzyme, becoming abundant in activated macrophages and other cells at sites of inflammation.


Both COX-1 and -2 also oxygenate two other essential fatty acids – DGLA (ω-6) and EPA (ω-3) – to give the series-1 and series-3 prostanoids, which are less inflammatory than those of series-2. DGLA and EPA are competitive inhibitors with AA for the COX pathways. This inhibition is a major mode of action in the way that dietary sources of DGLA and EPA (e.g. borage, fish oil) reduce inflammation.





Enzyme cyclooxygenase (box: first step in creating prostaglandins from fatty acids) (more details…)




Cyclooxygenase reaction mechanism


[edit] Pharmacology


In terms of their molecular biology, COX-1 and COX-2 are of similar molecular weight (approximately 70 and 72 kDa respectively), and having 65% amino acid sequence homology and near-identical catalytic sites. The most significant difference between the isoenzymes, which allows for selective inhibition, is the substitution of isoleucine at position 523 in COX-1 with valine in COX-2. The relatively smaller Val523 residue in COX-2 allows access to a hydrophobic side-pocket in the enzyme (which Ile523 sterically hinders). Drug molecules, such as DuP-697 and the coxibs derived from it, bind to this alternative site and are considered to be selective inhibitors of COX-2.



[edit] Classical NSAIDs


The main COX inhibitors are the non-steroidal anti-inflammatory drugs (NSAIDs).


The classical COX inhibitors are not selective (i.e. they inhibit all types of COX), and the main adverse effects of their use are peptic ulceration and dyspepsia. It is believed that this may be due to the “dual-insult” of NSAIDs - direct irritation of the gastric mucosa (many NSAIDs are acids), and inhibition of prostaglandin synthesis by COX-1. Prostaglandins have a protective role in the gastrointestinal tract, preventing acid-insult to the mucosa.



[edit] Newer NSAIDs


Selectivity for COX-2 is the main feature of celecoxib, rofecoxib and other members of this drug class, but these drugs carry the risk of peptic ulceration. COX-2-selectivity does not seem to affect other side-effects of NSAIDs (most notably an increased risk of renal failure), and some results have aroused the suspicion that there might be an increase in the risk for heart attack, thrombosis and stroke by a relative increase in thromboxane. Rofecoxib (brand name Vioxx) was taken off the market in 2004 because of these concerns. Some other COX-2 selective NSAIDs, such as celecoxib and etoricoxib, are still on the market.



[edit] Non-NSAID COX inhibition


Acetaminophen, also known as paracetamol, reversibly inhibits COX-3. COX-3 produces prostanoids in the brain, but does not participate in eicosanoid signalling in inflammation. Acetaminophen thereby interferes with the perception of pain. Since it has no effect on inflammation, it is not classed as an NSAID.[2][3]



[edit] Cardiovascular side effects of COX inhibitors


COX-2 inhibitors have been found to increase the risk of atherothrombosis even with short term use. A 2006 analysis of 138 randomised trials and almost 150 000 participants [4] showed that selective COX-2 inhibitors are associated with a moderately increased risk of vascular events, mainly due to a twofold increased risk of myocardial infarction, and also that high dose regimens of some traditional NSAIDs such as diclofenac and ibuprofen are associated with a similar increase in risk of vascular events.


COX-2 inhibitor

No Comments Filed Under: Medical

COX-2 selective inhibitor is a form of Non-steroidal anti-inflammatory drug (NSAID) that directly targets COX-2, an enzyme responsible for inflammation and pain. Selectivity for COX-2 reduces the risk of peptic ulceration, and is the main feature of celecoxib, rofecoxib and other members of this drug class. Cox-2-selectivity does not seem to affect other adverse-effects of NSAIDs (most notably an increased risk of renal failure), and some results have aroused the suspicion that there might be an increase in the risk for heart attack, thrombosis and stroke by a relative increase in thromboxane. Rofecoxib was taken off the market in 2004 because of these concerns.







Contents

[hide]


  • 1 Research history
  • 2 Adverse-effects and withdrawal of Vioxx
  • 3 Early COX-2 inhibiting drugs
  • 4 Comparative studies
  • 5 Combinations of drugs
  • 6 Risks and adverse effects
  • 7 Considerations for prescription
  • 8 Future of Cox 2 Inhibitors a treatment for neuroblastomas
  • 9 References
  • 10 External links


[edit] Research history


The COX2 enzyme was discovered in 1988 by Daniel Simmons, a Brigham Young University researcher formerly of Harvard University. Dr. Simmons immediately understood the importance of his discovery. The same day the enzyme was sequenced, he had his notebook notarized as proof of his discovery. Subsequently, Monsanto, the research firm with whom Dr. Simmons had contracted, fraudulently broke contract and refused to give Dr. Simmons any royalties and profits from his discovery. A lawsuit is currently in progress by Dr. Simmons against the drug developers. [1]


In the course of the search for a specific inhibitor of the negative effects of prostaglandins which spared the positive effects, it was discovered that prostaglandins could indeed be separated into two general classes which could loosely be regarded as “good prostaglandins” and “bad prostaglandins”, according to the structure of a particular enzyme involved in their synthesis, cyclooxygenase.


Prostaglandins whose synthesis involves the cyclooxygenase-I enzyme, or COX-1, are responsible for maintenance and protection of the gastrointestinal tract, while prostaglandins whose synthesis involves the cyclooxygenase-II enzyme, or COX-2, are responsible for inflammation and pain.


The existing nonsteroidal antiinflammatory drugs (NSAIDs) differ in their relative specificities for COX-2 and COX-1; while aspirin is equipotent at inhibiting COX-2 and COX-1 enzymes in vitro and ibuprofen demonstrates a sevenfold greater inhibition of COX-1, other NSAIDs appear to have partial COX-2 specificity, particularly meloxicam (Mobic). Studies of meloxicam 7.5 mg per day for 23 days find a level of gastric injury similar to that of a placebo, and for meloxicam 15 mg per day a level of injury lower than that of other NSAIDs; however, in clinical practice meloxicam can still cause some ulcer complications.


A search for COX-2-specific inhibitors resulted in promising candidates such as valdecoxib, celecoxib, and rofecoxib (marketed under the brand names Bextra, Celebrex, and Vioxx respectively). Valdecoxib and rofecoxib are about 300 times more potent at inhibiting COX-2, than COX-1, suggesting the possibility of relief from pain and inflammation, without gastrointestinal irritation, and promising to be a boon for those who had experienced such adverse effects previously or had comorbidities that could lead to such complications. Celecoxib is approximately 30 times more potent at inhibiting COX-2 than COX-1.


Although individual reactions to particular NSAIDs vary, in general the efficacy of COX-2 inhibitors has proved similar to that of other NSAIDs, as expected since both classes of drug inhibit the desired target, the action of COX-2 prostaglandins. The drugs’s effectiveness is similar to that of traditional NSAIDs such as ibuprofen, diclofenac, or naproxen.



[edit] Adverse-effects and withdrawal of Vioxx


On September 27, 2004 Vioxx (Rofecoxib) was withdrawn voluntarily from the market, due to an increased risk of myocardial infarction and stroke. At present it is unclear whether this adverse effect pertains also to other drugs of this group or is specific for Vioxx.


Beasley Allen Law Firm is spearheading the review of over 31,000 claims against the manufacturers of Bextra, Celebrex and Vioxx.



[edit] Early COX-2 inhibiting drugs


Celebrex and Vioxx were introduced in 1999 and rapidly became the most frequently prescribed new drugs in the United States. By October 2000, their US sales exceeded 100 million prescriptions per year for $3 billion, and were still rising, sales of Celebrex alone reaching $3.1 billion in 2001. A Spanish study found that between January 2000 and June 2001, 7% of NSAID prescriptions and 29% of NSAID expenditures were for COX-2 inhibitors. Over the period of the study, COX-2 inhibitors rose from 10.03% of total NSAIDs prescribed by specialty physicians to 29.79%, and from 1.52% to 10.78% of NSAIDs prescribed by primary care physicians (98.23% of NSAIDs and 94.61% of COX-2 inhibitors were prescribed by primary care physicians). For specialty physicians, rofecoxib and celecoxib were third and fifth most frequently prescribed NSAIDs but first and second in cost, respectively; for primary care physicians they were ninth and twelfth most frequently prescribed NSAIDs and first and fourth in cost.


The cause of the rapid widespread acceptance of Celebrex and Vioxx by physicians was the publication of two large trials in JAMA, the Celecoxib Long-term Arthritis Safety Study (CLASS) study, and the Vioxx Gastrointestinal Outcomes Research (VIGOR) study. Both publications concluded that COX-2 specific NSAIDs were associated with significantly fewer adverse gastrointestinal effects. In the CLASS trial comparing Celebrex 800 mg/day to ibuprofen 2400 mg/day and diclofenac 150 mg/day for osteoarthritis or rheumatoid arthritis for six months, Celebrex was significantly associated with fewer upper gastrointestinal complications (0.44% vs. 1.27%, P=0.04), with no significant difference in incidence of cardiovascular events in patients not taking aspirin for cardiovascular prophylaxis. In the VIGOR trial testing Vioxx 50 mg/day versus naproxen for rheumatoid arthritis, Vioxx reduced the risk of symptomatic ulcers and clinical upper gastrointestinal events (perforations, obstructions and bleeding) by 54%, to 1.4% from 3%, the risk of complicated upper gastrointestinal events (complicated perforations, obstructions and bleeding in the upper gastrointestinal tract) by 57%, and the risk of bleeding from anywhere in the gastrointestinal tract by 62%. An enormous marketing effort capitalized on these publications; Vioxx was the most heavily advertised prescription drug in 2000, and Celebrex the seventh, according to IMS Health.



[edit] Comparative studies


In a metaanalysis of eight osteoarthritis studies, the incidence of withdrawal because of adverse gastrointestinal events was 3.5% for Vioxx, compared to 4.8% for ibuprofen, diclofenac, or nabumetone (Relafen). Endoscopic studies of patients receiving Celebrex 50-400 mg twice daily for 12-24 weeks found rates of upper gastrointestinal complications similar to placebo and significantly lower than naproxen 500 mg twice daily and ibuprofen 800 mg three times daily, but not statistically significantly different from patients receiving diclofenac 75 mg twice daily.11 The analysis found that Vioxx provided significant gastrointestinal benefits in patients both at high risk and at low risk of developing gastrointestinal problems; patients at low risk still had 88% fewer gastrointestinal problems with Vioxx.


The results of the CLASS study were confirmed by the Successive Celecoxib Efficacy and Safety Studies (SUCCESS) study, which examined the effectiveness and safety of celecoxib 200 mg and 400 mg daily and how well it was tolerated by patients in terms of adverse effects, compared with the most common NSAID regimens in the countries studied (diclofenac 100 mg daily and naproxen 1000 mg daily). SUCCESS showed that celecoxib was as effective as the conventional NSAIDs in controlling the pain of arthritis, and caused fewer gastrointestinal ulcers or ulcer complications (such as perforations or bleeding) and fewer upper gastrointestinal adverse effects, e.g. 29% less chance of having nausea and 22% less chance of abdominal pain. In addition, hospitalization rates for upper gastrointestinal problems were 2 to 4 times lower with celecoxib, and because there were fewer adverse effects, there was 23% less chance of a celecoxib patient stopping treatment. The study also found that there was no real advantage to taking a bigger dose of celecoxib: the 200 mg dose was found to be just as effective as the 400 mg dose.


The VIGOR study was followed by the Assessment of Difference between Vioxx and Naproxen to Ascertain Gastrointestinal Tolerability and Effectiveness (ADVANTAGE) study, which showed that 9.1% of people taking Vioxx received a gastro-protective medicine compared with 11.2% of people taking naproxen, a reduction of 19%. In addition, after 3 months, 5.9% of people stopped taking Vioxx compared with 8.1% who stopped taking naproxen, a reduction of 27%. ADVANTAGE was the first study comparing the gastrointestinal tolerability of Vioxx and naproxen in a group that included patients taking low-dose aspirin for cardiovascular reasons. This was followed by the Experience with Vioxx in Arthritis (EVA) survey of 5,986 Belgian physicians and 74,192 people with osteoarthritis, which found that, after 12.5 or 25 mg of Vioxx once daily for 30 days, 80% of the patients wished to continue treatment with Vioxx and more than 80% of doctors said they would continue prescribing Vioxx. The preference to continue taking Vioxx was especially strong in people who previously treated with older NSAIDs.


In a six week long study comparing Vioxx 25 mg once daily, Vioxx 12.5 mg once daily, Celebrex 200 mg once daily, and paracetamol 1,000 mg four times daily for osteoarthritis of the knee, higher dose Vioxx was found to be superior to the other three treatments for reduction of nocturnal pain, and superior to Celebrex and acetaminophen for reduction of resting pain. At six weeks, 60% of high dose Vioxx patients reported a good or excellent response, compared to 46% of Celebrex patients and 39% of paracetamol patients. Low dose Vioxx was not found to be statistically significant from Celebrex at this dose. Similar results were found for early response to therapy.


However, when the Food and Drug Administration (FDA) later presented more complete data from the CLASS and VIGOR trials on its web site, the results were less certain. The CLASS trial was revealed to also have twelve and fifteen month time points which had not been discussed in the JAMA publication; in this segment of the trial, the number of ulcer-related complications for Celebrex caught up to the control NSAID group. Similarly, the complete VIGOR study data revealed that in fact, when all adverse events, not just gastrointestinal, were tabulated, the patients receiving VIOXX had suffered (barely) significantly higher incidence of adverse events overall than the control NSAID group. In particular, the risk of serious cardiovascular thrombotic events, e.g. myocardial infarction, was 1.7% in the VIOXX patients versus 0.7% in the control group, and there were significantly more withdrawals in the Vioxx group for causes including hypertension, edema, hepatotoxicity, heart failure, or pathological laboratory findings. The mean increases in systolic and diastolic blood pressure in the Vioxx group were 4.6 mmHg and 1.7 mmHg respectively, compared to 1.0 and 0.1 mmHg in the control NSAID group. An estimated 43,000,000 Americans, nearly one out of six, suffers from arthritis. However, 42% (18 million) of these also suffer from hypertension. Therefore, the promise of better patient outcomes and lowered medical costs from use of COX-2 inhibitors may not be as great as previously hoped. Questions remain regarding the relative safety and cost effectiveness of this new class. While endoscopic evidence of gastrointestinal damage is frequently seen in studies of nonspecific NSAIDs, the actual incidence of clinically evident symptoms and patient discomfort is much lower; furthermore, in cases of short-term therapy, any such damage generally reverses itself quickly after termination of the drug.



[edit] Combinations of drugs


A model comparing the theoretical relative frequency of gastrointestinal adverse effects and cost effectiveness of celecoxib, nonspecific NSAIDs alone, NSAIDs plus a proton pump inhibitor, NSAIDs plus an H2 receptor antagonist, NSAIDs plus misoprostol, and diclofenac/misoprostol, found the lowest probability of adverse gastrointestinal events for celecoxib, followed by NSAIDs plus a proton pump inhibitor, NSAIDs plus an H2 receptor antagonist, NSAID plus misoprostol, diclofenac/misoprostol, and NSAID alone. In total cost, including drug plus treatment of any gastrointestinal effects, the lowest cost treatment was celecoxib, followed by NSAIDs alone and diclofenac/misoprostol, with the other NSAID plus gastrointestinal protection regimens being much more costly. Similarly, a model of cost effectiveness of rofecoxib and celecoxib compared to high-dose acetaminophen or ibuprofen, with and without misoprostol, in patients with osteoarthritis of the knee found that acetaminophen had the lowest cost for average patients. For those not responding to paracetamol, ibuprofen was the most cost effective treatment by a large margin, but for those who did not respond to acetaminophen and had a high risk of gastrointestinal damage, rofecoxib was the most cost effective treatment.



[edit] Risks and adverse effects


This cardiovascular risk of COX-2 specific inhibitors is not surprising since prostaglandins are involved in regulation of blood pressure by the kidneys. Therefore, cardiovascular effects of NSAIDs prescribed for arthritis pain and inflammation need to be considered when choosing the appropriate medication for each patient. A French study of osteoarthritis patients over 65 years of age determined that, compared to Celebrex (200 mg once daily), patients taking Vioxx (25 mg once daily) suffered a two-fold increase in clinically significant edema and 60% more frequent increases in systolic blood pressure greater than 20 mmHg, as early as the second week of treatment. This has significant implications, since it has been estimated that every 2 mmHg increase in blood pressure raises the risk of stroke by two thirds and the risk of myocardial infarction by one third, suggesting that Celebrex may be a better choice for hypertensive patients or those at risk for edema. In addition, COX-2 inhibitors lack some of the platelet inhibiting properties of aspirin and other nonspecific NSAIDs and may, directly or indirectly, lead to increased risk of thrombosis, particularly in high risk patients where low dose aspirin therapy is warranted. On the other hand, this property makes them a better choice for perisurgical pain management, where inhibition of blood clotting would be problematic.


There are other differences between Celebrex and Vioxx that influence prescribing practices. Patients with known sensitivity to sulfa drugs are likely to be sensitive to Celebrex as well, due to similarity in structure. Vioxx has a more rapid onset and is approved for acute pain as well as osteoarthritis, while Celebrex is approved for rheumatoid arthritis as well as osteoarthritis.3



[edit] Considerations for prescription


A key assumption made in early COX-2 cost-effectiveness studies was lower cost due to a reduction in coprescription of agents used to protect the gastrointestinal tract from traditional NSAIDs. However, if gastroprotective agents continue to be coprescribed along with COX-2 inhibitors, there would seem to be no advantage to the use of these higher cost NSAIDs. Similarly, in patients who take aspirin for cardiovascular benefit, with its attendant gastrointestinal irritation, prescription of COX-2 inhibitors to avoid gastrointestinal irritation would seem to offer no advantage. This was confirmed by the CLASS study, which found significantly lower incidence of upper gastrointestinal complications alone and combined with symptomatic ulcers in patients taking Celebrex 400 mg twice daily, compared to ibuprofen 800 mg three times daily or diclofenac 75 mg twice daily; but this freedom from gastrointestinal complications was lost in patients taking concurrent low dose aspirin.



[edit] Future of Cox 2 Inhibitors a treatment for neuroblastomas


Recent studies have shown that small tumors of the sympathetic nervous system (neuroblastoma) have abnormal levels of COX-2 expressed (Johnsen et al). These studies report that and overexpression of the COX-2 enzyme has an adverse effect on the tumor suppressor, p53. p53 is an apoptosis transcription factor normally found in the cytosol, when cellular DNA is damaged beyond repair, p53 is transported to the nucleus where is promotes p53 mediated cell suicide (apoptosis) (Lau et al, 2006). Two of the metabolites of COX-2, prostaglandin A2 (PGA2) and A1 (PGA1), when present in high quantities binds to p53 in the cytosol and inhibits its ability to cross into the nucleus. This essentially sequesters p53 in the cytosol and prevents apoptosis (Lau et al, 2006). coxibs such as CELEBREX? (celecoxib), by selectively inhibiting the overexpressed COX-2, allow p53 to work properly. Functional p53 allows DNA damaged neuroblastoma cells to commit suicide through apoptosis, halting tumor growth. COX-2 up-regulation has also been linked to the phosphorylation and activation of the E3 ubiquitin ligase HDM2, a protein that mediates p53 ligation and tagged destruction, through ubiquitination (Lau et al, 2006). The mechanism for this neuroblastoma HDM2 hyperactivity is unknown. Studies have shown that COX-2 inhibitors block the phosphorilation of HDM2 preventing its activation (Figure 6B). In vitro, the use of COX-2 inhibitors such as CELEBREX? (celecoxib) lowers the level of active HDM2 found in neuroblastoma cells. The exact process of how COX-2 inhibitors block HDM2 phosphorilation is unknown, but this mediated reduction in active HDM2 concentration level restores the cellular p53 levels. After treatment with CELEBREX? (celecoxib), the restored p53 function allows DNA damaged neuroblastoma cells to commit suicide through apoptosis reducing the size of growth of the tumor (Lau et al, 2006).


Monoamine oxidase

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Monoamine oxidase



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“MAO” redirects here. For other uses, see Mao (disambiguation).




































Ribbon diagram of a monomer of human MAO-A, with FAD and clorgiline bound, oriented as if attached to the outer membrane of a mitochondrion. From PDB 2BXS.

monoamine oxidase A
Identifiers
Symbol MAOA
Entrez 4128
HUGO 6833
OMIM 309850
RefSeq NM_000240
UniProt P21397
Other data
EC number 1.4.3.4
Locus Chr. X p11.4-p11.3




































Cartoon diagram of human MAO-B. From PDB 1GOS.

monoamine oxidase B
Identifiers
Symbol MAOB
Entrez 4129
HUGO 6834
OMIM 309860
RefSeq NM_000898
UniProt P27338
Other data
EC number 1.4.3.4
Locus Chr. X p11.4-p11.3

Monoamine oxidases (singular abbreviation MAO) (EC 1.4.3.4) are enzymes that catalyze the oxidation of monoamines. They are found bound to the outer membrane of mitochondria in most cell types in the body. The enzyme was discovered by Mary Hare in the liver, and received the name of tyramine oxidase.[1]







Contents

[hide]


  • 1 Locations of MAO-A and MAO-B
  • 2 Function
  • 3 Subtype Specificities
  • 4 Disorders resulting from MAO dysfunction
  • 5 Genetics
  • 6 See also
  • 7 References
  • 8 External links


[edit] Locations of MAO-A and MAO-B


In humans there are two types of MAO: MAO-A and MAO-B.



  • Both are found in neurons and astroglia.
  • Outside the central nervous system:

    • MAO-A is also found in the liver, gastrointestinal tract and placenta.
    • MAO-B is mostly found in blood platelets.


[edit] Function


Monoamine oxidases catalyze the oxidative deamination of monoamines. Oxygen is used to remove an amine group from a molecule, resulting in the corresponding aldehyde and ammonia. The general form of the catalyzed reaction (with R denoting an arbitrary group) is

     H                      H
R-C-NH2 + O2 + H2O → R-C=O + NH3 + H2O2
H

Monoamine oxidase contains the covalently-bound cofactor FAD.



[edit] Subtype Specificities


MAO-A is particularly important in the catabolism of monoamines ingested in food. Both MAOs are also vital to the inactivation of monoaminergic neurotransmitters, for which they display different specificities.



  • Serotonin, norepinephrine (noradrenaline), and epinephrine (adrenaline) are mainly broken down by MAO-A.
  • Phenethylamine is broken down by MAO-B.
  • Both forms break down dopamine.


[edit] Disorders resulting from MAO dysfunction


Because of the vital role that MAOs play in the inactivation of neurotransmitters, MAO dysfunction (too much/too little MAO activity) is thought to be responsible for a number of neurological disorders. For example, unusually high or low levels of MAOs in the body have been associated with depression, substance abuse, attention deficit disorder, and irregular sexual maturation. Monoamine oxidase inhibitors are one of the major classes of drug prescribed for the treatment of depression, although they are last line treatment due to risk of the drug’s interaction with diet or other drugs. Excessive levels of catecholamines (epinephrine, norepinephrine, and dopamine) may lead to a hypertensive crisis, and excessive levels of serotonin may lead to serotonin syndrome.


PET research has shown that MAO is also heavily depleted by use of tobacco cigarettes.[2]



[edit] Genetics


The genes encoding MAO-A and MAO-B are located side-by-side on the short arm of the X chromosome, and have about 70% sequence similarity. Rare mutations in the gene are associated with Brunner syndrome.


A study reported in Science in August 2002 concluded that maltreated children with a low-activity polymorphism in the promoter region of the MAO-A gene were more likely to develop antisocial conduct disorders than maltreated children with the high-activity variant.[3] The suggested mechanism for this effect is the decreased ability of those with low MAO-A activity to quickly degrade norepinephrine, the synaptic neurotransmitter involved in sympathetic arousal and rage. This is alleged to provide direct support for the idea that genetic susceptibility to disease is not determined at birth, but varies with exposure to environmental influences.


Research also uncovered a possible link between predisposition to novelty seeking and a genotype of the MAO-A gene.[4]


In 2006, a New Zealand researcher, Dr Rod Lea said that a particular variant (or genotype) was over-represented in Māori, a Warrior gene. This supported earlier studies finding different proportions of variants in different ethnic groups. This is the case for many genetic variants, with 33% White/Non-Hispanic, 61% Asian/Pacific Islanders having the low-activity MAO-A promoter variant.[5]


Catecholamine

No Comments Filed Under: Medical

Catecholamines are chemical compounds derived from the amino acid tyrosine containing catechol and amine groups. Some of them are biogenic amines. Catecholamines are water soluble and are 50% bound to plasma proteins, so they circulate in the bloodstream. The most abundant catecholamines are epinephrine (adrenaline), norepinephrine (noradrenaline) and dopamine, all of which are produced by phenylalanine and tyrosine. Tyrosine is created from phenylalanine by hydroxylation thanks to the enzyme, phenylalanine hydroxylase (tyrosine is also ingested directly from dietary protein). Tyrosine is then sent to catecholamine secreting neurons. Here many kinds of reactions convert it to dopamine, to norepinephrine and epinephrine eventually.[1] Catecholamines as hormones are released by the adrenal glands in situations of stress such as psychological stress or low blood sugar levels[2].







Contents

[hide]


  • 1 Production
  • 2 Function

    • 2.1 Modality
    • 2.2 Effects

  • 3 Structure
  • 4 Degradation
  • 5 See also
  • 6 References
  • 7 External links


[edit] Production


Catecholamines are produced mainly by the chromaffin cells of the adrenal medulla and the postganglionic fibers of the sympathetic nervous system. Dopamine, which acts as a neurotransmitter in the central nervous system, is largely produced in neuronal cell bodies in two areas of the brainstem: the substantia nigra and the ventral tegmental area.



[edit] Function



[edit] Modality


Two catecholamines, norepinephrine and dopamine, act as neurotransmitters in the central nervous system and as hormones in the blood circulation. The catecholamine norepinephrine is a neurotransmitter of the peripheral sympathetic nervous system but is also present in the blood (mostly through “spillover” from the synapses of the sympathetic system).


High catecholamine levels in blood are associated with stress, which can be induced from psychological reactions or environmental stressors such as elevated sound levels, intense light, or low blood sugar levels.


Extremely high levels of catecholamine (also known as catecholamine toxicity) can occur in CNS trauma due to stimulation and/or damage of nuclei in the brainstem, particularly those nuclei affecting the sympathetic nervous system. In emergency medicine, this occurrence is widely known as catecholamine dump.



[edit] Effects


Catecholamines cause general physiological changes that prepare the body for physical activity (fight-or-flight response). Some typical effects are increases in heart rate, blood pressure, blood glucose levels, and a general reaction of the sympathetic nervous system. Some drugs, like tolcapone (a central COMT-inhibitor), raise the levels of all the catecholamines.



[edit] Structure


Catecholamines have the distinct structure of a benzene ring with two hydroxyl groups, an intermediate ethyl chain and a terminal amine group.



[edit] Degradation


They have a half-life of approximately a few minutes when circulating in the blood.


Monoamine oxidase (MAO) is the main enzyme responsible for degradation of catecholamines.


Methamphetamine and MAOIs bind to MAOs to inhibit their action of breaking down catecholamines. This is primarily the reason why the effects of amphetamines last longer than cocaine and other substances. Amphetamines not only causes a release of dopamine, epinephrine, and norepinephrine into the blood stream, but also keeps it working there for a long time.


 




tyrosine is the precursor of catecholamines

 



epinephrine

 



norepinephrine

 



dopamine

 

 


No higher resolution available.
Biosynthese_Adrenalin.png (652 × 246 pixels, file size: 6 KB, MIME type: image/png)

Vanillyl mandelic acid

No Comments Filed Under: Medical


Vanillyl mandelic acid (VMA) is a metabolite of the catecholamine: norepinephrine.


VMA is found in the urine, along with other catecholamine metabolites, including homovanillic acid (HVA). In timed urine tests the quantity (concentration μg /24 h) is assessed, along with creatinine clearance, and the concentration of cortisols, catecholamines, and metanephrines.


These urinalysis tests are used to diagnose an adrenal gland tumor called pheochromocytoma, a tumor of catecholamine-secreting chromaffin cells. These tests may also be used to diagnose neuroblastomas, and to monitor treatment of these conditions.


Norepinephrine breaks down into normetanephrine and VMA. Norepinephrine is one of the hormones produced by the adrenal glands, which are found on top of the kidneys. They are released into the blood during times of physical or emotional stress, which are factors that may skew the results of the test.


 


Homovanillic acid (HOC6H3(OCH3)CH2COOH; synonyms: 3-Methoxy-4-hydroxyphenyl acetic acid; HVA; 4-Hydroxy-3-methoxy-benzeneacetic acid; 4-Hydroxy-3-methoxyphenylacetic acid) is a major catecholamine metabolite. It is used as a reagent to detect oxidative enzymes.


In psychiatry and neuroscience, brain and cerebrospinal fluid levels of HVA are measured as a marker of metabolic stress caused by 2-deoxy-D-glucose.1


 


2-Deoxy-D-glucose


 


2-Deoxy-D-glucose is a glucose molecule which has the 2-hydroxyl group replaced by hydrogen, so that it cannot undergo further glycolysis. Glucose hexokinase traps this substance in most cells (with exception of liver and kidney) so that it makes a good marker for tissue glucose use and hexokinase activity. Many cancers have elevated glucose uptake and hexokinase levels. 2-Deoxyglucose labeled with tritium or carbon-14 has been a popular ligand for laboratory research in animal models, where distribution is assessed by tissue-slicing followed by autoradiography, sometimes in tandem with either conventional or electron microscopy.


Recent work on the ketogenic diet as a treatment for epilepsy have investigated the role of glycolysis in the disease. 2-Deoxyglucose has been proposed by Garriga-Canut et al. as a mimic for the ketogenic diet, and shows great promise as a new anti-epileptic drug.[2] Garriga-Canut et al suggest that 2-DG works, in part, by decreasing the expression of Brain-derived neurotrophic factor (BDNF). Such uses are complicated by the fact that 2-deoxyglucose does have some toxicity.


In living systems, such as in medical imaging (PET scanning), fluorodeoxyglucose is used, where one of the 2-hydrogens of 2-deoxy-D-glucose is replaced with the positron-emitting isotope fluorine-18, which emits paired gamma rays, allowing distribution of the tracer to be imaged by external gamma camera(s). This is increasingly done in tandem with a CT function which is part of the same PET/CT machine, to allow better localization of small-volume tissue glucose-uptake differences.


Retrieved from “http://en.w확인ikipedia.org/wiki/Vanillyl_mandelic_acid“


Phenethylamine

No Comments Filed Under: Medical


Phenethylamine, or β-Phenylethylamine, is an alkaloid and monoamine. In the human brain, it is believed to function as a neuromodulator or neurotransmitter (trace amine). Phenethylamine is a natural compound biosynthesized from the amino acid phenylalanine by enzymatic decarboxylation. It is also found in many foods such as chocolate, especially after microbial fermentation. It has been suggested that phenethylamine from food may have psychoactive effects in sufficient quantities. However, it is quickly metabolized by the enzyme MAO-B, preventing significant concentrations from reaching the brain.


Substituted phenethylamines are a broad and diverse class of compounds that include neurotransmitters, hormones, stimulants, hallucinogens, entactogens, anorectics, bronchodilators, and antidepressants.







Contents

[hide]


  • 1 Chemistry
  • 2 Chocolate theory of love
  • 3 Substituted phenethylamines
  • 4 Pharmacology
  • 5 Substitution table
  • 6 Graphical overview
  • 7 See also
  • 8 References
  • 9 External links


[edit] Chemistry


Phenethylamine is an aromatic amine, which is a colorless liquid at room temperature. It is soluble in water, ethanol, and ether.[1] Similar to other low-molecular-weight amines, it has a fishy odor. Upon exposure to air, it forms a solid carbonate salt with carbon dioxide. Phenethylamine is strongly basic and forms a stable crystalline hydrochloride salt with a melting point of 217 °C. Phenethylamine is also a skin irritant and possible sensitizer.



[edit] Chocolate theory of love


In the early 1980s, chemistry of love researcher Michael Libowitz, author of the popular 1983 book The Chemistry of Love, remarked to reporters that “chocolate is loaded with PEA.” This became the focus for an article in The New York Times, which was then taken up by the wire services, then by magazine free-lancers, and evolved into the now-eponymous “chocolate theory of love.”[2] However, as noted earlier, phenethylamine is rapidly metabolized by the enzyme MAO-B, preventing significant concentrations from reaching the brain, thus contributing no perceptible psychoactive effect.



[edit] Substituted phenethylamines




General structure of phenethylamines and amphetamines (see the table below).

Substituted phenethylamines carry additional chemical modifications at the phenyl ring, the sidechain, or the amino group:



  • Substituted Amphetamines are homologues of phenethylamines carrying an alpha-methyl (α-CH3) group at the sidechain carbon atom next to the amino group.
  • Catecholamines are phenethylamines carrying two hydroxy groups in positions 3 and 4 of the phenyl ring. Examples are the hormones and neurotransmitters dopamine, epinephrine (adrenaline), and norepinephrine (noradrenaline).
  • The aromatic amino acids phenylalanine and tyrosine are phenethylamines carrying a carboxyl group (COOH) in alpha position.
  • 2Cs are phenethylamines with methoxy groups attached to the 2 and 5 carbons and no alpha-methyl group.


[edit] Pharmacology


Many substituted phenethylamines are pharmacologically-active drugs due to their similarity to the monoamine neurotransmitters:



  • Stimulants like the plant alkaloids ephedrine and cathinone and the synthetic drug dextroamphetamine and methylphenidate
  • Hallucinogens like the plant alkaloid mescaline and the synthetic drug 2C-B
  • Empathogen-entactogens like MDMA (ecstasy) and MDA
  • Anorectics like phentermine, fenfluramine, and amphetamine
  • Bronchodilators like salbutamol and ephedrine
  • Antidepressants like venlafaxine, bupropion and the monoamine oxidase inhibitors phenelzine and tranylcypromine.


[edit] Substitution table


Some of the more important phenethylamines are tabulated below. For simplicity, the stereochemistry of the sidechain is not covered in the table. Hundreds of other simple synthetic phenethylamines are known. This is due in part to the pioneering work of Alexander Shulgin, much of which is described in the book PiHKAL.







































































































































































































































































































































































































Substituted phenethylamines, tabulated by structure
Short Name Rα Rβ R2 R3 R4 R5 RN Full Name
Tyramine OH 4-hydroxy-phenethylamine
Dopamine OH OH 3,4-dihydroxy-phenethylamine
Epinephrine (Adrenaline) OH OH OH CH3 β,3,4-trihydroxy-N-methylphenethylamine
Norepinephrine (Noradrenaline) OH OH OH β,3,4-trihydroxyphenethylamine
Salbutamol OH OH CH2OH C(CH3)3 β,4-dihydroxy-3-hydroxymethyl-N-tert-butyl-phenethylamine
Beta-methyl-phenethylamine CH3 β-methylphenethylamine
Amphetamine CH3 α-methylphenethylamine
Methamphetamine CH3 CH3 N-methylamphetamine
Methylphenidate N,α-butylene-β-methoxycarbonylphenethylamine
Ephedrine,
pseudoephedrine
CH3 OH CH3 N-methyl-β-hydroxyamphetamine
Acetylamphetamine CH3 COCH3 α-methyl-3-acetylphenethylamine
Cathine CH3 OH β-hydroxy-amphetamine
Cathinone CH3 =O β-ketoamphetamine
Methcathinone CH3 =O CH3 N-methyl-β-ketoamphetamine
Bupropion CH3 =O Cl C(CH3)3 3-chloro-N-tert-butyl-β-ketoamphetamine
Fenfluramine CH3 CF3 CH2CH3 3-trifluoromethyl-N-ethyl-amphetamine
Phentermine 2CH3 α,α-dimethylphenethylamine
Mescaline OCH3 OCH3 OCH3 3,4,5-trimethoxyphenethylamine
MDA CH3 -O-CH2-O- 3,4-methylenedioxyamphetamine
MDMA CH3 -O-CH2-O- CH3 3,4-methylenedioxy-N-methylamphetamine
MDMC CH3 =O -O-CH2-O- CH3 3,4-methylenedioxy-N-methyl-β-ketoamphetamine
DOM CH3 OCH3 CH3 OCH3 2,5-dimethoxy-4-methylamphetamine
DOB CH3 OCH3 Br OCH3 2,5-dimethoxy-4-bromoamphetamine
DON CH3 OCH3 NO2 OCH3 2,5-dimethoxy-4-nitroamphetamine
2C-B OCH3 Br OCH3 2,5-dimethoxy-4-bromophenethylamine
2C-C OCH3 Cl OCH3 2,5-dimethoxy-4-chlorophenethylamine
DOI CH3 OCH3 I OCH3 2,5-dimethoxy-4-iodoamphetamine
2C-I OCH3 I OCH3 2,5-dimethoxy-4-iodophenethylamine
2C-D OCH3 CH3 OCH3 2,5-dimethoxy-4-methylphenethylamine
2C-E OCH3 CH2-CH3 OCH3 2,5-dimethoxy-4-ethylphenethylamine
2C-F OCH3 F OCH3 2,5-dimethoxy-4-fluorophenethylamine
2C-N OCH3 NO2 OCH3 2,5-dimethoxy-4-nitrophenethylamine
2C-T-2 OCH3 S-CH2CH3 OCH3 2,5-dimethoxy-4-ethylthio-phenethylamine
2C-T-4 OCH3 S-CH(CH3)2 OCH3 2,5-dimethoxy-4-isopropylthio-phenethylamine
2C-T-7 OCH3 S-CH2CH2CH3 OCH3 2,5-dimethoxy-4-propylthio-phenethylamine
2C-T-8 OCH3 S-CH2-C3H5 OCH3 2,5-dimethoxy-4-cyclopropylmethylthio-phenethylamine
2C-T-9 OCH3 S-C(CH3)3 OCH3 2,5-dimethoxy-4-tert-butylthio-phenethylamine
2C-T-21 OCH3 S-CH2-CH2-F OCH3 2,5-dimethoxy-4-(2-fluoroethylthio)-phenethylamine

 




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