|
PAM Value |
Distance(%) |
|
|
80 |
50 |
|
|
100 |
60 |
|
|
200 |
75 |
|
|
250 |
85 |
<- Twilight zone |
|
300 |
92 |
|
(From Doolittle, 1987, Of URFs and ORFs, University Science Books)
When the PAM distance value between two distantly related proteins nears the value 250 it becomes difficult to tell whether the two proteins are homologous, or that they are two at randomly taken proteins that can be aligned by chance. In that case we speak of the 'twilight zone'.

The relation between the observed percentage in distance of two sequences versus PAM value. Two randomly diverging sequences change in a negatively exponential fashion. After the insertion of gaps to two random sequences, it can be expected that they will be 80 - 90 % dissimilar (from Doolittle, 1987 ).
"
|
|
Rate of Change |
Theoretical |
|
Pseudogenes |
400 |
45 |
|
Fibrinopeptides |
90 |
200 |
|
Lactalbumins |
27 |
670 |
|
Lysozymes |
24 |
850 |
|
Ribonucleases |
21 |
850 |
|
Haemoglobins |
12 |
1500 |
|
Acid proteases |
8 |
2300 |
|
Cytochrome c |
4 |
5000 |
|
Glyceraldehyde-P dehydrogenase |
2 |
9000 |
|
Glutamate dehydrogenase |
1 |
18000 |
|
Origin of the Universe |
15 billion yrs |
|
Formation of the Solar System |
4.6 " |
|
First Self-replicating System |
3.5 " |
|
Prokaryotic-Eukaryotic Divergence |
2.0 " |
|
Plant-Animal Divergence |
1.0 " |
|
Invertebrate-Vertebrate Divergence |
0.5 " |
|
Mammalian Radiation Beginning |
0.1 " |