| Literature DB >> 31622354 |
Juliana Cordeiro1, Tuane Letícia Carvalho2, Vera Lúcia da Silva Valente3, Lizandra Jaqueline Robe2,4.
Abstract
Transposable elements (TEs) have the main role in shaping the evolution of genomes and host species, contributing to the creation of new genes and promoting rearrangements frequently associated with new regulatory networks. Support for these hypotheses frequently results from studies with model species, and Drosophila provides a great model organism to the study of TEs. Micropia belongs to the Ty3/Gypsy group of long terminal repeats (LTR) retroelements and comprises one of the least studied Drosophila transposable elements. In this study, we assessed the evolutionary history of Micropia within Drosophilidae, while trying to assist in the classification of this TE. At first, we performed searches of Micropia presence in the genome of natural populations from several species. Then, based on searches within online genomic databases, we retrieved Micropia-like sequences from the genomes of distinct Drosophilidae species. We expanded the knowledge of Micropia distribution within Drosophila species. The Micropia retroelements we detected consist of an array of divergent sequences, which we subdivided into 20 subfamilies. Even so, a patchy distribution of Micropia sequences within the Drosophilidae phylogeny could be identified, with incongruences between the species phylogeny and the Micropia phylogeny. Comparing the pairwise synonymous distance (dS) values between Micropia and three host nuclear sequences, we found several cases of unexpectedly high levels of similarity between Micropia sequences in divergent species. All these findings provide a hypothesis to the evolution of Micropia within Drosophilidae, which include several events of vertical and horizontal transposon transmission, associated with ancestral polymorphisms and recurrent Micropia sequences diversification.Entities:
Year: 2019 PMID: 31622354 PMCID: PMC6797199 DOI: 10.1371/journal.pone.0220539
Source DB: PubMed Journal: PLoS One ISSN: 1932-6203 Impact factor: 3.240
Presence/absence of Micropia sequences in the genomes of Drosophilidae species.
Methodology employed and GeneBank accession numbers are also shown.
| Genus | Subgenus | Group species | Species | Presence/absence | Methodology | GenBank acc. nos. |
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*Sequences used as initial BLASTn queries. Capital letters refer to the fly collector/supplier:
ATucson Drosophila Stock Center (currently The National Drosophila Species Stock Center at Cornell University)
BDr. Luciano Basso da Silva
CDr. Marco Silva Gottschalk
DMSc. Jonas da Silva Doge
EDra. Daniela Cristina De Toni. Species vouchers are available at the Laboratório de Drosophilidae at Universidade Federal do Rio Grande do Sul.
Fig 1Phylogenetic reconstruction of species analyzed in this study.
Phylogenetic reconstruction was based on data compiled from previous studies [50, 51, 52, 53, 54, 55 and 56] which have a limited overlap on sampled species. Species name in black represents the presence of Micropia sequences and species name in grey represents the absence of such sequences. Distinct branch colors represent distinct subgenera within the Drosophila genus, and the classification follows [43]. Drosophila genus group species are also indicated to the right. Scaptodrosophila and Phortica are represented as outgroups of the Drosophila genus. The dashed line represents the potential phylogenetic position of D. zottii, since there is no molecular phylogeny neither any nuclear or mitochondrial gene available for this species.
Fig 2Bayesian phylogenetic tree of the Drosophilidae Micropia sequences analyzed in this study after the second filtering step.
The phylogenetic tree was based on amino acid sequences following a mixed evolution model with gamma correction. Bargues and Lerat´s sequences [15] were included in the analysis. Numbers from 1 to 20 on the left represent the Micropia subfamilies recovered in our data. Filled circles after Micropia sequence names indicate sequences involved in possible HTT events based on one-tailed Fisher’s exact test involving pairwise comparisons of dS values between Micropia and nuclear genes (Adh in orange, Amd in pink, Ddc in purple; see S6 Table). Stars represent the four best-characterized Micropia elements (D. hydei dhMiF2 and dhMiF8; and D. melanogaster Dm11 and Dm2). The posterior probability of each clade is indicated beside its respective internal branch.
Mean pairwise amino acid genetic distances between Micropia subfamilies.
| 01 | 02 | 03 | 04 | 05 | 06 | 07 | 08 | 09 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 | 19 | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Subf. 02 | 0.357 | ||||||||||||||||||
| Subf. 03 | 0.313 | 0.345 | |||||||||||||||||
| Subf. 04 | 0.327 | 0.343 | 0.297 | ||||||||||||||||
| Subf. 05 | 0.385 | 0.407 | 0.338 | 0.335 | |||||||||||||||
| Subf. 06 | 0.436 | 0.397 | 0.412 | 0.423 | 0.315 | ||||||||||||||
| Subf. 07 | 0.410 | 0.442 | 0.324 | 0.341 | 0.376 | 0.376 | |||||||||||||
| Subf. 08 | 0.690 | 0.739 | 0.533 | 0.620 | 0.625 | 0.496 | 0.302 | ||||||||||||
| Subf. 09 | 0.407 | 0.521 | 0.328 | 0.360 | 0.368 | 0.351 | 0.181 | 0.433 | |||||||||||
| Subf. 10 | 0.421 | 0.407 | 0.341 | 0.345 | 0.381 | 0.400 | 0.217 | 0.451 | 0.237 | ||||||||||
| Subf. 11 | 0.468 | 0.461 | 0.431 | 0.405 | 0.454 | 0.422 | 0.274 | 0.512 | 0.284 | 0.271 | |||||||||
| Subf. 12 | 0.435 | 0.425 | 0.360 | 0.368 | 0.480 | 0.441 | 0.366 | 0.635 | 0.384 | 0.361 | 0.426 | ||||||||
| Subf. 13 | 0.664 | 0.401 | 0.580 | 0.574 | 0.549 | 0.751 | 0.518 | 0.586 | 0.584 | 0.535 | 0.573 | 0.437 | |||||||
| Subf. 14 | 0.413 | 0.441 | 0.358 | 0.382 | 0.393 | 0.374 | 0.332 | 0.577 | 0.334 | 0.317 | 0.385 | 0.354 | 0.539 | ||||||
| Subf. 15 | 0.381 | 0.512 | 0.346 | 0.363 | 0.398 | 0.406 | 0.323 | 0.586 | 0.318 | 0.324 | 0.385 | 0.302 | 0.440 | 0.304 | |||||
| Subf. 16 | 1.499 | 0.857 | 1.345 | 1.425 | 1.338 | 1.460 | 1.437 | 1.368 | 1.401 | 1.359 | 1.302 | 1.484 | 1.408 | 1.391 | 1.507 | ||||
| Subf. 17 | 0.406 | 0.511 | 0.349 | 0.375 | 0.418 | 0.426 | 0.297 | 0.586 | 0.313 | 0.327 | 0.398 | 0.292 | 0.431 | 0.336 | 0.140 | 1.365 | |||
| Subf. 18 | 0.401 | 0.449 | 0.330 | 0.375 | 0.418 | 0.390 | 0.339 | 0.611 | 0.312 | 0.318 | 0.391 | 0.288 | 0.430 | 0.310 | 0.149 | 1.533 | 0.137 | ||
| Subf. 19 | 0.376 | 0.505 | 0.334 | 0.351 | 0.371 | 0.390 | 0.266 | 0.598 | 0.285 | 0.287 | 0.337 | 0.301 | 0.465 | 0.309 | 0.119 | 1.375 | 0.157 | 0.160 | |
| Subf. 20 | 0.366 | 0.460 | 0.330 | 0.356 | 0.309 | 0.432 | 0.233 | 0.496 | 0.238 | 0.285 | 0.367 | 0.247 | 0.651 | 0.280 | 0.145 | 1.509 | 0.138 | 0.123 | 0.113 |