Recent observations of Venus have yielded new evidence of a compound in its atmosphere that could indicate the presence of life, according to findings that potentially lend weight to controversial past discoveries.
Phosphine, a toxic gas that astrobiologists have proposed could be associated with the presence of life on rocky planets, was initially detected in Venus’s atmosphere in a surprise discovery four years ago. Now, new observations potentially strengthen those past findings, hinting at the presence of biosignatures that, if confirmed, could mean life forms are able to thrive in the planet’s harsh environment.
A Controversial Discovery on Venus
The initial detection of phosphine in Venus’s oxidized atmosphere was reported in September 2020, when a team of scientists led by Jane Greaves of Cardiff University said they had found evidence of the toxic molecule. The discovery initially led to debate over the possibility that life could exist on Venus, since phosphine is normally associated with organisms that thrive in low-oxygen environments.
The team’s announcement received considerable media attention, and also led to controversy that culminated in rebukes from some in the scientific community. Arguably, the sharpest criticism was leveled by the organizing committee of the International Astronomical Union (IAU) Commission F3 on Astrobiology, who even questioned the ethics of Greaves and her team over the manner in which the discovery was revealed.
“It is an ethical duty for any scientist to communicate with the media and the public with great scientific rigour and to be careful not to overstate any interpretation which will be irretrievably picked up by the press,” the commission wrote in an official statement released at the time.
The commission added it “would like to remind the relevant researchers that we need to understand how the press and the media behave before communicating with them.”
Initial follow-up attempts to detect the compound again were unsuccessful. However, last year, Greaves and her team succeeded in detecting phosphine in deeper portions of the planet’s atmosphere during observations made with the James Clark Maxwell Telescope (JCMT) at Mauna Kea Observatory, Hawaii. Additional detections with NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) also suggested the presence of phosphine, which may originate either within or from below the clouds on Venus.
Hellbound and Down 