| Literature DB >> 25985773 |
Camile Moray1, Xia Hua2, Lindell Bromham3.
Abstract
BACKGROUND: Salt tolerance in plants is rare, yet it is found across a diverse set of taxonomic groups. This suggests that, although salt tolerance often involves a set of complex traits, it has evolved many times independently in different angiosperm lineages. However, the pattern of evolution of salt tolerance can vary dramatically between families. A recent phylogenetic study of the Chenopodiaceae (goosefoot family) concluded that salt tolerance has a conserved evolutionary pattern, being gained early in the evolution of the lineage then retained by most species in the family. Conversely, a phylogenetic study of the Poaceae (grass family) suggested over 70 independent gains of salt tolerance, most giving rise to only one or a few salt tolerant species. Here, we use a phylogenetic approach to explore the macroevolutionary patterns of salt tolerance in a sample of angiosperm families, in order to ask whether either of these two patterns - deep and conserved or shallow and labile - represents a common mode of salt tolerance evolution. We analyze the distribution of halophyte species across the angiosperms and identify families with more or less halophytes than expected under a random model. Then, we explore the phylogenetic distribution of halophytes in 22 families using phylogenetic comparative methods.Entities:
Mesh:
Year: 2015 PMID: 25985773 PMCID: PMC4436861 DOI: 10.1186/s12862-015-0379-0
Source DB: PubMed Journal: BMC Evol Biol ISSN: 1471-2148 Impact factor: 3.260
Fig. 1Family subtrees for a sample of six of the families analyzed with significant NoTO and/or SSCD values. Inferred gains of salt tolerance (see Methods) are marked on each family with black circles. Tips in the subtrees identified as halophytes are marked in black in the ring around the subtree. The subtrees represent a) Amaranthaceae, b) Apiaceae, c) Brassicaceae, d) Cucurbitaceae, e) Cyperaceae, and f) Euphorbiaceae. All 22 subtrees included in the analysis are presented in Additional file 1: Figure S1. Subtree plots were created using the “Diversitree” package [58]
Results of taxonomic and phylogenetic analyses for a sample of 22 angiosperm families
| Order | Family | Family size | Known Halophytes | Halophytes in family (%) | Taxonomic pattern | Family subtree size | Species in subtree (%) | Halophytes in subtree | Halophytes in subtree (%) | Halophytes sampled in subtree (%) | Inferred origins | NoTO | NoTO ( | SSCD ( |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Apiales | Apiaceae | 3780 | 33 | 0.9 | 1082 | 28.6 | 26 | 2.4 | 78.8 | 22 | 1.2 |
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| Arecales | Arecaceae | 2361 | 35 | 1.5 | more | 415 | 17.6 | 19 | 4.6 | 54.3 | 15 | 1.3 | 0.06 |
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| Asterales | Asteraceae | 23600 | 267 | 1.1 | 4618 | 19.6 | 97 | 2.1 | 36.3 | 87 | 1.1 |
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| - | Goodeniaceae | 430 | 6 | 1.4 | 69 | 16.0 | 6 | 8.7 | 100 | 6 | 1.0 | 0.09 |
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| Brassicales | Brassicaceae | 3710 | 38 | 1.0 | 1355 | 36.5 | 21 | 1.5 | 55.3 | 19 | 1.1 |
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| Caryophyllales | Amaranthaceae | 2275 | 507 | 22.3 | more | 613 | 26.9 | 262 | 42.7 | 51.7 | 54 | 4.9 | 0.16 |
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| - | Tamaricaceae | 90 | 55 | 61.1 | more | 42 | 46.7 | 29 | 69.0 | 52.7 | 1 | 29.0 |
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| Cucurbitales | Cucurbitaceae | 960 | 14 | 1.5 | 247 | 25.7 | 9 | 3.6 | 64.3 | 8 | 1.1 | 0.14 |
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| Ericales | Primulaceae | 2590 | 14 | 0.5 | fewer | 546 | 21.1 | 8 | 1.5 | 57.1 | 5 | 1.6 | 0.65 | 0.55 |
| Fagales | Casuarinaceae | 95 | 12 | 12.6 | more | 88 | 92.6 | 12 | 13.6 | 100 | 7 | 1.7 | 0.46 | 0.08 |
| Gentianales | Rubiaceae | 13150 | 13 | 0.1 | fewer | 1393 | 10.6 | 7 | 0.5 | 53.8 | 7 | 1.0 | 0.09 |
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| Lamiales | Acanthaceae | 4000 | 18 | 0.5 | fewer | 498 | 12.5 | 9 | 1.8 | 50.0 | 5 | 1.8 | 0.75 | 0.54 |
| - | Lamiaceae | 7173 | 27 | 0.4 | fewer | 941 | 13.1 | 14 | 1.5 | 51.9 | 11 | 1.3 | 0.14 | 0.05 |
| Malpighiales | Euphorbiaceae | 5735 | 42 | 0.7 | fewer | 1047 | 18.3 | 16 | 1.5 | 38.1 | 14 | 1.1 |
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| - | Rhizophoraceae | 149 | 19 | 12.8 | more | 40 | 26.8 | 18 | 45.0 | 94.7 | 6 | 3.0 | 0.52 | 0.71 |
| Myrtales | Combretaceae | 500 | 12 | 2.4 | more | 25 | 5.0 | 8 | 32.0 | 66.7 | 6 | 1.3 | 0.23 | 0.25 |
| - | Lythraceae | 620 | 21 | 3.4 | more | 119 | 19.2 | 14 | 11.8 | 66.7 | 8 | 1.8 | 0.53 | 0.46 |
| - | Myrtaceae | 4620 | 47 | 1.0 | 612 | 13.2 | 20 | 3.3 | 42.6 | 19 | 1.1 |
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| Poales | Cyperaceae | 5430 | 121 | 2.2 | more | 1087 | 20.0 | 57 | 5.2 | 47.1 | 52 | 1.1 |
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| - | Juncaceae | 430 | 22 | 5.1 | more | 124 | 28.8 | 12 | 9.7 | 54.5 | 8 | 1.5 | 0.31 | 0.45 |
| - | Poaceae | 11160 | 335 | 3.0 | more | 2291 | 20.5 | 173 | 7.6 | 51.6 | 127 | 1.4 |
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| Rosales | Rosaceae | 2520 | 9 | 0.4 | fewer | 1010 | 40.1 | 8 | 0.8 | 88.9 | 8 | 1.0 | 0.05 | 0.05 |
Family and order names are based on APG III [48]. Family size is the mean estimated number of species in the family reported on the APG III website [49]. The halophytes column lists the number of known halophytes species in each family. Family subtree size represents the number of taxa in the phylogenetic tree used for analysis, and halophytes in subtree is the number of known halophytes included in each family subtree. The halophytes sampled in subtree represents the percent of known halophytes that are present in each family subtree. The taxonomic pattern column identifies families with more or fewer halophytes than expected by chance based on the taxonomic analysis (see Methods). The results of the metrics used to distinguish evolutionary patterns of salt tolerance are presented. For the number of tips per origin (NoTO), p-values represent whether the average number of halophytes arising from each inferred gain of salt tolerance is smaller expected under Brownian motion (p < 0.05). For the sum of sister clade differences (SSCD), p-values represent whether halophytes are less clustered than expected under Brownian motion (p < 0.05). Test statistics that are significantly different to the null model are presented in bold. Significant results for Tamaricaceae are italicized to highlight that this is the only significantly conserved pattern of salt tolerance, where significantly more tips per gain and a significantly smaller SSCD