Microheliella maris (Microhelida ord. n.), an Ultrastructurally Highly Distinctive New Axopodial Protist Species and Genus, and the Unity of Phylum Heliozoa

A new heliozoan, Microheliella maris, has sufficiently distinctive ultrastructure to merit a new order, Microhelida. Its 18S and 28S rRNA genes were sequenced earlier under the informal name ‘marine microheliozoan’; we here sequenced its Hsp90 gene. A three-gene tree suggests that it is distantly related to centrohelids and others in chromist subkingdom Hacrobia; but it is too divergent to be placed accurately by few genes. Unlike centrohelids, its central spherical centrosome has two concentric granular shells and a dense core devoid of a trilaminar central disc. Microtubules radiate from the centrosomal shells. Unlike centrohelids, axopodia have only three microtubules, fixed basally by dense plasma membrane anchors, and bear terminal and lateral haptosome-like extrusomes. As in the heliomonad Heliomorpha, the centrosome is embedded in a nuclear cavity, and centrosomal microtubules traverse the nucleus inside cytoplasmic channels. A novel filogranular network interconnects mitochondria, ER, and plasma membrane. The microbody is attached to the nucleus and mitochondrion, which has vermicular tubular cristae. We group Microhelida and Heliomonadida, purged of dissimilar flagellates, as a new tubulicristate class Endohelea within phylum Heliozoa. Previously misassigned GenBank 18S rDNA sequences reveal Microhelida as diverse and ancient. We discuss principles underlying the biogenesis and diversity of axopodial patterns.