The CEO of Rocket Lab explains why we need to go “soon”


Venus, a planet close to Earth with a planet of hot gases, can host a possible sign of life. The recent discovery has excited some of the most important figures of private spaceflight.

In a study published on Monday in the journal Nature astronomy, Scientists announced that they detected traces of phosphine gas in the Venus atmosphere. Gas is generally associated with life on Earth. But at about 1,000 degrees Fahrenheit, the surface of Venus is not conducive to life in the way we are used to – and the team cannot explain how the gas was found. Lead author Jane Greaves described the discovery as “very unexpected and very exciting”.

For Peter Beck, CEO of private spaceflight firm Rocket Lab, the search focused its attention on Venus as a destination. While SpaceX CEO Elon Musk outlines plans to build a city on Mars, and Blue Origin founder Jeff Bezos intends to build floating space cities, Beck plans a Venus trip instead.

“Today’s research highlights why we need to leave, and soon,” Beck explains In the shlokas.

Personal interest in Venus – The decisive initiative also announced the intention to look forward to Venus. On Tuesday, the private space science organization funded by Russian investor Yuri Milner announced plans to finance a research study for the possibility of life on the planet.

In a statement on the initiative’s website, Milner emphasized the importance of search discovery:

“It would be really important to find life anywhere beyond the earth. And if there is a non-negligible chance that it is right next to Venus, then exploring that possibility is an essential priority for our civilization. “

Meanwhile, Beck has talked about his passion for Venus. In August 2020, he said during a livestream that he is “madly in love with Venus,” with plans to host a private mission to the planet in 2023. The mission will target an aerial environment 30 miles above the surface, where conditions are close to those found on Earth.

Peter Beck.Kimberly White / Getty Images Entertainment / Getty Images

“I have always been fond of Venus,” Beck said. In the shlokas.

“It has long been envisaged that its environment can potentially support some form of life, and I’ve always been eager to send an inquiry to find out. More than just searching for life, though, Venus is a very good Earth analogue for migration. Climate change, so I believe we can learn a lot from Venus’s past and apply it to Earth’s future. ”

Venus has attracted the attention of fans interested in the emerging new space race, a race with a more prominent role for private firms. A map shared on Reddit last month showed what the planet would look like if the Earth’s surface covered the same amount of water. Mapp followed from previous maps that applied the same treatment to Mars. Both planets have been the subject of discussion around terraforming, a human-driven change of atmosphere and surface.

For now, the only earthly visitor near Venus is Akatsuki, a Japanese space probe. It contributes to the study of the planet’s gravity waves, equatorial jet streams and the physics of its clouds.

While Rocket Lab is one of the major companies in this new space race, Beck’s focus for Venus is the Photon spacecraft. The company’s satellite design support has been launched at a variety of altitudes.

Beck said, “About a year ago when work began on our mission for NASA to lunar orbit, we were ready to design a photon spacecraft capable of a mission to the moon, but Venus would also say Huh.” “The development of that spacecraft and mission is now going well. The first mission of Venus will be a private one which will closely monitor the possibilities of life with atmospheric probes, but it will not be the only mission of Venus.”

Read the summary of Monday’s paper below:

Measurement of trace gases in planetary atmospheres helps us to detect the chemical conditions present on Earth. Our nearest neighbor Venus has cloud decks that are temperate but hyperactive. Here we report the apparent presence of phosphine (PH3) gas in the atmosphere of Venus, where any phosphorus must be oxidized. There is no other plausible detection of single-line millimeter-waveband spectral detections (quality up to ~ 15)) from JCMT and ALMA telescopes. ~ 20 ppb abundance estimates at atmospheric PH3. The presence of PH3 is unclear after exhaustive studies of steady-state chemistry and photochemical pathways, along the currently known abiotic production routes in Venus’s atmosphere, clouds, surface and subsurface, or from lightning, volcanic, or meteorite distributions. PH3 may arise from the presence of life in unknown photochemistry or geochemistry, or by analogy with the biological production of PH3 on Earth. Other PH3 spectral features should be sought, while in situ clouds and surface samples can investigate the sources of this gas.