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Molecular Drivers of RNA Phase Separation
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Abstract
RNA molecules are essential in orchestrating the assembly of biomolecular condensates and membraneless compartments in cells. Many condensates form via the association of RNA with proteins containing specific RNA binding motifs. However, recent reports indicate that low-complexity RNA sequences can self-assemble into condensate phases without protein assistance. Divalent cations significantly influence the thermodynamics and dynamics of RNA condensates, which exhibit base-specific lower-critical solution temperatures (LCST). The precise molecular origins of these temperatures remain elusive. In this study, we employ atomistic molecular simulations to elucidate the molecular driving forces governing the temperature-dependent phase behavior of RNA, providing new insights into the origins of LCST. Using RNA tetranucleotides and their chemically modified analogs, we map RNA condensates’ equilibrium thermodynamic profiles and structural ensembles across various temperatures and ionic conditions. Our findings reveal that magnesium ions promote LCST behavior by inducing local order-disorder transitions within RNA structures. Consistent with experimental observations, we demonstrate that the thermal stability of RNA condensates follows the Poly(G) > Poly(A) > Poly(C) > Poly(U) order shaped by the interplay of base-stacking and hydrogen bonding interactions. Furthermore, our simulations show that ionic conditions and post-translational modifications can fine-tune RNA self-assembly and modulate condensate physical properties.
Author Summary
RNA molecules are essential for organizing membraneless compartments that play critical roles in cellular processes. While many of these condensates form through interactions between RNA and proteins, recent studies have shown that certain RNA sequences can self-assemble into condensates without protein assistance. This ability is influenced by the sequence composition of RNA and the presence of ions like magnesium. Using detailed molecular simulations we carried out systematic study to reveal how temperature and ionic conditions affect RNA condensation. We discovered that magnesium ions play a key role in driving RNA molecules to condense at lower temperatures by promoting structural changes within the RNA. Our findings also revealed that the stability of RNA condensates varies depending on the RNA sequence, with guanine-rich sequences being the most stable. Additionally, we demonstrated how chemical modifications and ionic conditions can fine-tune the properties of RNA condensates. This study provides new insights into how RNA forms condensates and highlights potential strategies to control their behavior, which could have implications for understanding cellular organization and developing new therapies.
Title: Molecular Drivers of RNA Phase Separation
Description:
Abstract
RNA molecules are essential in orchestrating the assembly of biomolecular condensates and membraneless compartments in cells.
Many condensates form via the association of RNA with proteins containing specific RNA binding motifs.
However, recent reports indicate that low-complexity RNA sequences can self-assemble into condensate phases without protein assistance.
Divalent cations significantly influence the thermodynamics and dynamics of RNA condensates, which exhibit base-specific lower-critical solution temperatures (LCST).
The precise molecular origins of these temperatures remain elusive.
In this study, we employ atomistic molecular simulations to elucidate the molecular driving forces governing the temperature-dependent phase behavior of RNA, providing new insights into the origins of LCST.
Using RNA tetranucleotides and their chemically modified analogs, we map RNA condensates’ equilibrium thermodynamic profiles and structural ensembles across various temperatures and ionic conditions.
Our findings reveal that magnesium ions promote LCST behavior by inducing local order-disorder transitions within RNA structures.
Consistent with experimental observations, we demonstrate that the thermal stability of RNA condensates follows the Poly(G) > Poly(A) > Poly(C) > Poly(U) order shaped by the interplay of base-stacking and hydrogen bonding interactions.
Furthermore, our simulations show that ionic conditions and post-translational modifications can fine-tune RNA self-assembly and modulate condensate physical properties.
Author Summary
RNA molecules are essential for organizing membraneless compartments that play critical roles in cellular processes.
While many of these condensates form through interactions between RNA and proteins, recent studies have shown that certain RNA sequences can self-assemble into condensates without protein assistance.
This ability is influenced by the sequence composition of RNA and the presence of ions like magnesium.
Using detailed molecular simulations we carried out systematic study to reveal how temperature and ionic conditions affect RNA condensation.
We discovered that magnesium ions play a key role in driving RNA molecules to condense at lower temperatures by promoting structural changes within the RNA.
Our findings also revealed that the stability of RNA condensates varies depending on the RNA sequence, with guanine-rich sequences being the most stable.
Additionally, we demonstrated how chemical modifications and ionic conditions can fine-tune the properties of RNA condensates.
This study provides new insights into how RNA forms condensates and highlights potential strategies to control their behavior, which could have implications for understanding cellular organization and developing new therapies.
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