Unlocking the Mystery: How the Venus Flytrap Snaps Shut

Venus flytrap closing

How Venus Flytraps Capture Prey

Credit: Jeanne Bourdier, Corentin Maurier

The intriguing mechanism behind how Venus flytraps close quickly to ensnare insect prey has seen substantial investigation.

The Venus flytrap (Dionaea muscipula) reacts instantly when its sensitive hairs are stimulated twice, leading to a swift trap closure. This plant is known for its ability to capture various insects, including a tiny frog. However, the exact workings of this fascinating process have remained elusive to scientists since the days of Charles Darwin.

Many experts believe that the closure mechanism involves a rapid transfer of water through the trap’s tissues, causing one side to contract while the other expands, thereby facilitating the quick closure. To test this theory, Yoel Forterre and a team from the University of Aix-Marseille, France, investigated the water’s transit time across both isolated cells and tissue in the trap.

They found that water movement took approximately 30 to 60 seconds, leading researchers to conclude that this mechanism would be too slow, as trap closure typically occurs within a second.


Subsequently, researchers observed that the trap’s surface texture changed to a bumpier state after activation, indicating a reduction in cell wall stiffness. They employed fine probes to measure mechanical forces within the epidermal cells to examine if this softening contributed to the trap’s closure.

“When the trap is stimulated, we found that the outer epidermal layer’s cell walls softened almost instantaneously,” stated Forterre. Upon triggering the hairs, electrical signals and waves of calcium ions travel throughout the leaf. He likened these signals to the plant’s version of neural impulses, enabling rapid communication regarding the touch contact from the trigger hairs to distant cells within moments.

Upon receiving these signals, the outer surface of the trap quickly decreases in mechanical stiffness, releasing internal stress and allowing pressurized inner cells to contract further on one side. Consequently, the outer edge expands while the inner surface remains hard, bending the trap shut.

Despite these findings, researchers still lack clarity on the specific molecules responsible for these swift changes in cell wall dynamics. “We grasp the initial sensing mechanism and the final trapping movement, but understanding the molecular connections between these events remains elusive,” emphasized Forterre.

Professor Sergei Shabara from the University of Western Australia expressed skepticism about the proposed mechanism, arguing that water might not flow continuously through the cells as suggested. He believes cell wall stiffness adaptations could take several minutes instead of being instantaneous. “Although the methodology of this study is impressive, it does not definitively rule out water movement as a driving force,” stated Shabara.

Nevertheless, Forterre highlighted that their measurements regarding tissue swelling time support the idea that water transport across the trap is too slow to account for rapid closure, emphasizing the unexpectedly swift decrease in cell wall stiffness.

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Source: www.newscientist.com

Hubble Space Telescope Snaps Photo of NGC 346 in Ultraviolet Light

The Hubble team has released a striking new photo taken with the NASA/ESA Hubble Space Telescope of NGC 346, an open star cluster in one of our Milky Way galaxy’s closest neighbors.



This Hubble Space Telescope image shows the open star cluster NGC 346, located about 210,000 light-years away in the constellation Sigurd. Image courtesy of NASA/ESA/C. Murray, Space Telescope Science Institute/Gladys Kober, NASA, and The Catholic University of America.

NGC 346 is located in the constellation Tucana and is about 210,000 light-years away.

Also known as ESO 51-10, Kron 39, and Lindsay 60, the star cluster was discovered on August 1, 1826, by Scottish astronomer James Dunlop.

NGC 346 is part of the Small Magellanic Cloud, a dwarf galaxy that is a satellite of the Milky Way galaxy.

The cluster was formed approximately 3 million years ago, has a diameter of 150 light years, and a mass 50,000 times that of the Sun.

“NGC 346’s hot stars are unleashing torrents of radiation and energy outflows that are eating away at the dense gas and dust of the surrounding nebula N66,” Hubble astronomers said in a statement.

“Dozens of hot, blue, high-mass stars shine within NGC 346, and the cluster is thought to contain more than half of the known high-mass stars in the entire Small Magellanic Cloud.”

The Hubble Space Telescope has previously observed NGC 346, but this new image shows the cluster in ultraviolet light, along with visible light data.

“Ultraviolet light helps us understand star formation and evolution, and Hubble is the only telescope capable of sensitive ultraviolet observations thanks to its sharp resolution and its location above the ultraviolet-blocking atmosphere,” the astronomers write.

“These particular observations were collected to learn more about how star formation shapes the interstellar medium – the gas distributed throughout seemingly empty space – in metal-poor galaxies like the Small Magellanic Cloud.”

“Elements heavier than hydrogen and helium are called ‘metals’, and the Small Magellanic Cloud has a lower metal content than most of the Milky Way.”

“This situation serves as an excellent example of a galaxy similar to those that existed in the early universe when there were few heavy elements to take up.”

Source: www.sci.news