NASA’s Curiosity rover unearths largest organic molecules ever detected on Mars

In a stunning new development, NASA scientists have confirmed that the Curiosity rover has discovered the largest organic molecules ever found on the Martian surface. The groundbreaking analysis of an existing rock sample, “Cumberland,” within Curiosity’s onboard lab revealed the presence of decane, undecane, and dodecane – compounds with 10, 11, and 12 carbon atoms respectively.

These molecules are believed to be fragments of preserved fatty acids, key building blocks of life as we know it on Earth. While non-biological origins are possible, the size of these newly detected molecules significantly boosts the potential for the preservation of complex biosignatures on the red planet.

This discovery builds upon years of tantalizing findings by Curiosity, including the detection of smaller organic molecules, organic salts, and the measurement of total organic carbon comparable to Earth’s most extreme environments. The new data suggests that larger, more complex organic compounds could have survived for billions of years despite harsh Martian conditions.

The network of cracks in this Martian rock slab called “Old Soaker” may have formed from the drying of a mud layer more than 3 billion years ago. The view spans about 3 feet (90 centimeters) left-to-right and combines three images taken by the MAHLI camera on the arm of NASA’s Curiosity Mars rover.
Credits: NASA/JPL-Caltech/MSSS

Lead author Caroline Freissinet emphasized the significance, stating, “Our study proves that, even today, by analyzing Mars samples, we could detect chemical signatures of past life—if it ever existed on Mars.”

Scientists are particularly intrigued by the carbon chain length of the presumed fatty acids (11-13 carbons), as non-biological processes typically yield shorter chains. This raises the exciting possibility of longer-chain fatty acids, often associated with biological activity, being present.

While the exact origin of these molecules remains under investigation, this major breakthrough reinforces the critical need for Mars Sample Return missions to conduct in-depth analysis with advanced Earth-based instruments.

“We are ready to take the next big step and bring Mars samples home to our labs to settle the debate about life on Mars,” declared Dr. Daniel Glavin.

This latest discovery marks a significant leap in our understanding of Martian organic chemistry and further fuels the compelling narrative that Mars may have once harbored the conditions necessary for life. The search for evidence of past life on the red planet has just intensified.

NASA Mars Mission Successful, Marco Cubesats separate, InSight Rover landing soon

NASA launched its next Mars mission with a stationary lander InSight and for the first time carrying a payload of two CubeSats.

InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport), the first mission to explore Mars’ deep interior, was launched at 7:05 a.m. EDT on May 5, 2018, from Vandenberg Air Force Base on a ULA Atlas V rocket.

The main purpose of the mission is to probe shape of the rocky planets of the inner solar system more than four billion years ago.

If the mission is successful, the technology will provide NASA the ability to quickly transmit status information about the main spacecraft after it lands on Mars, where its two landers — Opportunity and Curiosity rovers have been examining the Red Planet’s surface.

The twin communications-relay CubeSats, built by NASA’s Jet Propulsion Laboratory, Pasadena, California, are demos of Mars Cube One (MarCO) technology, developed by university students, but launched only into Earth orbit, not deep space in the past.

The basic CubeSat unit is a box roughly 4 inches (10 centimeters) square. Larger CubeSats are multiples of that unit. MarCO’s design is a six-unit CubeSat – about the size of a briefcase — with a stowed size of about 14.4 inches (36.6 centimeters) by 9.5 inches (24.3 centimeters) by 4.6 inches (11.8 centimeters).

“MarCO-A and B are our first and second interplanetary CubeSats designed to monitor InSight for a short period around landing, if the MarCO pair makes it to Mars,” said Jim Green, director of NASA’s planetary science division. “However, these CubeSat missions are not needed for InSight’s mission success. They are a demonstration of potential future capability. The MarCO pair will carry their own communications and navigation experiments as they fly independently to the Red Planet.”

During InSight’s entry, descent and landing (EDL) operations, the lander will transmit information in the UHF radio band to NASA’s Mars Reconnaissance Orbiter (MRO) flying overhead. MRO will forward EDL information to Earth using a radio frequency in the X band, but cannot simultaneously receive information over one band while transmitting on another. Confirmation of a successful landing could take one hour to reach Earth.

MarCO’s softball-size radio provides both UHF (receive only) and X-band (receive and transmit) functions capable of immediately relaying information received over UHF.

The two CubeSats will separate from the Atlas V booster after launch and travel along their own trajectories to the Red Planet. MarCO’s first challenges are to deploy two radio antennas and two solar panels.

The high-gain, X-band antenna is a flat panel engineered to direct radio waves the way a parabolic dish antenna does. MarCO will be navigated to Mars independently of the InSight spacecraft, with its own course adjustments on the way.

If the MarCO mission succeeds, it entails many such “bring-your-own” communications relay option for use by future Mars missions. This technology demonstration could lead to many other applications to explore and study our solar system.