ORIGINAL PAPERFirst Molecular Characterization of the Elusive Marine Protist Meteora sporadica
Introduction
Meteora sporadica is an extremely unusual protist that was first reported 20 years ago in deep sea sediment samples from the Sporades Basin in the Eastern Mediterranean Sea (Hausmann et al. 2002). It exhibited small colorless non-flagellated cells with an oval shape that measured 3.0–4.4 μm long and 2.0–4.0 μm wide. What made this protist truly unique were its unusual appendages and movement. Meteora glides on substrates using two types of appendages: two lateral arm-like appendages (one on each side of the equatorial plan of the cell), which present a continuous rowing movement, and two longer appendages, one on each pole of the cell, aligned in the direction of the cell movement. No other eukaryotic organism has ever been described to move in this peculiar way. It was hypothesized that the rowing movement of the two short arms enhances the chance to encounter bacterial prey, which is then immobilized by putative extrusome granules (up to 2 on each arm) (Hausmann et al. 2002).
Due to the striking morphological dissimilarity with members of all other known eukaryotic taxa, Meteora was classified as Protista incertae sedis. Unfortunately, the authors of the original description did not succeed to stablish a culture and no molecular data has been obtained for this species to date. In this study, we determined the 18S rRNA gene sequence of protist cells collected from sediment of a shallow marine lagoon in the Mediterranean island of Mljet (Croatia), which were morphologically indistinguishable from the previously described Meteora sporadica. The morphological similarity and geographical proximity between our sampling point and the type locality support the notion that the protist cells studied in this work correspond to the type species Meteora sporadica. The analysis of its 18S rRNA gene sequence allowed us to study its phylogeny, which showed its lack of close affinity with any other eukaryotic group, and its absence in environmental 18S rRNA gene sequence databases.
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Habitat
We observed Meteora cells after culture enrichment of sediment samples from the shallow marine lagoon Malo Jezero (Mljet Island, Croatia, Mediterranean Sea), collected in July 2014 and kept frozen at −20 °C for several years (until September 2019). After 48 h of incubation of thawed sediment at room temperature, Meteora cells became visible and remained alive for a few days. In these transient Meteora-enriched samples, we also observed some of the protist species described by Hausmann et al.
Methods
Sample collection: Sediment samples from the shallow marine lagoon Malo Jezero (42°47′05.9″N 17°21′01.3″E) in the island of Mljet (Croatia, Mediterranean Sea) were collected in July 2014. Samples were taken from the upper layer of the sediment in the shore of the lagoon with a sterile 15 ml Falcon tube at a depth of 10 cm below the water surface. Samples were then stored at −20 °C until further analysis.
Cell growth, microscopy, and cell micromanipulation: Frozen sediment samples were thawed and
CRediT Authorship Contribution Statement
Luis Javier Galindo: Conceptualization, Investigation, Writing – original draft. Purificación López García: Conceptualization, Supervision, Resources, Funding acquisition, Writing – review & editing. David Moreira: Conceptualization, Supervision, Resources, Funding acquisition, Writing – review & editing.
Acknowledgements
We thank Miguel Iniesto for help in searching Meteora-like sequences in several databases. This work was funded by the European Research Council Advanced Grants ProtistWorld (No. 322669) and Plast-Evol (No. 787904) and the Horizon 2020 research and innovation program under the Marie Skłodowska-Curie ITN project SINGEK (http://www.singek.eu/; grant agreement no. H2020-MSCA-ITN-2015-675752).
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