惯性聚合 高效追踪和阅读你感兴趣的博客、新闻、科技资讯
阅读原文 在惯性聚合中打开

推荐订阅源

Cloudbric
Cloudbric
E
Exploit-DB.com RSS Feed
SecWiki News
SecWiki News
Forbes - Security
Forbes - Security
N
News | PayPal Newsroom
S
Security @ Cisco Blogs
Schneier on Security
Schneier on Security
V
V2EX - 技术
S
Secure Thoughts
W
WeLiveSecurity
Google DeepMind News
Google DeepMind News
C
CERT Recently Published Vulnerability Notes
NISL@THU
NISL@THU
S
Securelist
S
Security Archives - TechRepublic
Know Your Adversary
Know Your Adversary
V
Vulnerabilities – Threatpost
Security Latest
Security Latest
Recent Commits to openclaw:main
Recent Commits to openclaw:main
G
GRAHAM CLULEY
H
Hacker News: Front Page
Microsoft Azure Blog
Microsoft Azure Blog
I
Intezer
Google Online Security Blog
Google Online Security Blog
美团技术团队
阮一峰的网络日志
阮一峰的网络日志
T
The Exploit Database - CXSecurity.com
钛媒体:引领未来商业与生活新知
钛媒体:引领未来商业与生活新知
Webroot Blog
Webroot Blog
Jina AI
Jina AI
Engineering at Meta
Engineering at Meta
P
Proofpoint News Feed
The Cloudflare Blog
I
InfoQ
L
LangChain Blog
U
Unit 42
P
Proofpoint News Feed
S
Schneier on Security
S
Security Affairs
Y
Y Combinator Blog
T
Tenable Blog
N
News and Events Feed by Topic
MyScale Blog
MyScale Blog
量子位
Google DeepMind News
Google DeepMind News
Cyberwarzone
Cyberwarzone
博客园 - 聂微东
D
Darknet – Hacking Tools, Hacker News & Cyber Security
GbyAI
GbyAI
AWS News Blog
AWS News Blog

Universe Today

Reading the Galaxy's Past The Shape of a Black Hole Written in Rock Titan's Hidden Blanket Did Life Start When Impacts Created Vast Hydrothermal Systems in Earth's Crust? Meet REMORA: The Autonomous Space Fleet Built to Tag and Track Asteroids Watch the Moon Occult Venus in the Daytime for North America on June 17th Astrochemical Model Digs Into the Universe's Missing Sulfur Building in Space With Laser "Origami" On The Hunt For Cosmic Dawn And The Universe’s Very First Stars David Kipping Has a New Take on the Existence of Advanced Life in the Universe... and the Numbers are Not Encouraging! This is How Supermassive Black Holes Feed Themselves NASA’s Proposed EVE Mission Aims to Solve the Radius Valley Mystery Where Not to Look in the Search for ET Reading the Moon in X-rays Why Can't the Universe Be Cyclic? Part 4: When a Good Idea Meets Bad Data Orbiting Stars Give Clues to a Quiescent Black Hole's Mass Magnetic Fields Help Binary Stars Form and Black Holes Merge A Rare Meteorite Just Revealed a Lost, Mars-Sized Planet from the Dawn of the Solar System Neptune’s Weirdest Moon Nereid Might Be the Lone Survivor of an Ancient "Moonpocalypse" Space Telescopes Are Now Overwhelmed by Satellite Trails Why Can't the Universe Be Cyclic? Part 3: The Ekpyrotic Universe and Its Bouncing Branes Catch Comet 220P McNaught in Outburst The Hidden Physics Complicating Interstellar Lightsails Student Astronomer Identifies Source of Mysterious Cosmic Signals Why Can't the Universe Be Cyclic? Part 2: The Awkward Triumph of Inflation The SETI Institute Releases Technosignature Report on 3I/ATLAS Why Can't the Universe Be Cyclic? Part 1: The Lure of the Eternal Universe A “Green” Dual-Mode Engine is About to Give CubeSats the Best of Both Worlds SETI Panel Revises Recommendations for Dealing With 'Disclosure Day' NASA Bids Farewell to MAVEN Mars Mission in Public Teleconference Astronomers Make "Live" Observation of a Nearby Protoplanetary Disk's Rotation The Cosmic Web Like You've Never Seen it Before They've Been Searching for the Milky Way's Black Hole Wind for 50 Years and Finally Found It What Happens to a Star That Captures A Primordial Black Hole? New Cloud-Detecting Method Will Help Astronomers Characterize Exoplanets Even Without A Magnetosphere, Mars Can Still Deflect Some Solar Wind The Unexpected Brightness 'Gap' in an Ancient Globular Cluster Cosmic Tryst: Venus Meets Jupiter at Dusk A Brief-ish History of SETI. Part IX: What Have We Found? A New Map of Stars Shows That the Small Magellanic Cloud is Expanding Here's Why So Many Massive Galaxies in the Early Universe Stop Forming Stars Exoplanetary Weather Watchers Find Strong Evidence of Magnetic Fields Asteroid Dirt is "Fluffier" Than We Thought Blue Origin Issues Official Statement on New Glenn Explosion Astronomers Uncover Statistical Evidence for Recoiling Supermassive Black Holes The Next-Generation Very Large Array Prototype (ngVLA) Gathers its First Light Flash-Melted Glass from Chang'e-5 Reveals a High Levels of Iron on the Moon How Early Earth's Unlikely Chemical Hero Appeared Mars Hid its Warm, Wet Crystals Underground Could the Milky Way’s Missing Mass Be Hiding in a Swarm of Interstellar Comets? Ceres’ Surface Is Much More Complex Than Previously Thought Are the JWST's Early Overrmassive Black Holes Just Normal-Range Outliers? Astrobiology's Looming Statistical Crisis The Filamentary Funnels That Form Stars How Heavy Can a Neutron Star Get? Jupiter Created the Birthplace of Rocky Bodies in the Early Solar System How a Giant Moon and a Steam Atmosphere Built the Recipe for Life A Faster Way To Forecast Alien Weather Longest-period young transiting exoplanets discovered Roman Telescope's massive infrared mirror is ready to fly JWST Finds Methane Atmosphere on Temperate Exoplanet Blue Origin's Lunar Lander Just Passed Its Toughest Test Yet The Loudest Planet Wins A Brief-ish History of SETI. Part VIII: Paradox? What Paradox? The Galaxy That Forgot to Spin Did We Invent Dark Energy for Nothing? It Took a Cosmic Village to Shape Early Galaxies Lasers at the Lunar Poles Could Help Astronauts Navigate Who You Send to the Moon Matters More Than You Think MAVEN Spacecraft Finds New Plasma Squeezing at Mars The Sun is Changing and We Don’t Know Why ESA Selects Two New Scout-Class Missions 20,000 Eyes on the Universe The Flash Memory That Space Can't Destroy We Can Now Weigh Galaxies Using Dead Stars As Scales JWST Studies a Dark and Airless Super-Earth Earthly Hors d'oeuvres For Hungry Red Dwarfs The Name N159 Doesn't Do This Brilliant Star-Forming Region Justice An Orbiting Satellite Triad Reveals Motions Inside Earth Just Like Stars, Open Clusters Can Form Binary Pairs Astrophysical Calibration Could "Autotune" Gravitational Wave Detection Something Just Passed Between Us and a Distant Star. When Spacetime Crystallises, a Black Hole is Born The Weirdness of Early Universe SMBHs Gets Even Weirder A Natural Chemistry Laboratory in Protostar Shock Waves A New Model Helps Astronomers Study How Merging Black Holes Ring Why the Second Full Moon of May is a ‘Blue Minimoon’ NASA TESS Reveals Epic All-Sky Map of Distant Worlds Astronomers Observe the Most Chemically Primitive Galaxy in the Early Universe Where Are All the Intermediate Mass Black Holes? Microlensing Fast Radio Bursts Might Reveal Them When the Sun Tries to Explode and Fails The Sun Just Did Something Nobody Expected and it Kept Going For 19 Days Three Stars, One Extraordinary System and a Drama Still to Come The Definitive Census of Multiple Star Systems Within 10 Parsecs Are Satellite Megaconstellations Accidentally Geoengineering the Earth? The Risk of Stellar Flybys and GJ 710 How Mars Can Help Us Understand 'Marginal' Exoplanets Ultrahigh-energy Cosmic Rays May Be Ultraheavy in Origin NASA's Next-Generation AI Processor Passes Early Testing
Astronomers Find a Four-Carbon Sugar in Deep Space
Andy Tomaswick · 2026-06-10 · via Universe Today

The space between stars may seem like a barren desert, but over the past few decades scientists have been finding all sorts of interesting chemicals in it. From the precursors to proteins to the building blocks of cell membranes, there has been discovery after discovery of new molecules in the giant gas clouds between the stars. Now, a new paper available in pre-print on arXiv details the discovery of the first ever four-carbon sugar in the Interstellar Medium (ISM), and it is another brick on the path to understanding how life on Earth first developed.

The sugar in question is called erythrulose, a type of “ketose” sugar and one that is, you guessed it, made up of a chain with four carbons in it. Researchers found it in a famously rich molecular cloud known as G+0.693-0.027, seemingly named that way because they love to torture journalists writing about it. In searching for it they used two powerful radio telescopes - the 40m Yebes telescope and the 30m IRAM telescope, and sifted through the clouds' dense spectral lines to find their target.

And find it they did - to a level that the chances of those specific spectral lines showing up randomly only amounted to 0.2%. But what might actually be more interesting is what they didn’t find - any three-carbon sugars. The erythrulose was at least eight times more abundant than its three-carbon analogs, such as glyceraldehyde. Which then begs the question - how did a four carbon sugar form without any three-carbon sugars available to seed it?

Video describing interstellar space. Credit - SpaceTime YouTube Channel

To uncover this pathway, the researchers turned to advanced quantum chemical models and a type of simulation known as a Kinetic Monte Carlo (KMC) simulation. Through these tests, they found that erythrulose likely doesn’t build up one carbon atom at a time. Instead, it forms when two-carbon fragments such as glycoaldehyde and ethylene glycol combine on the icy surfaces of microscopic dust grains. In molecular clouds, those types of grains are constantly being bombarded by cosmic rays and atomic hydrogen, creating radical fragments that drive this reaction, resulting in a four-carbon sugar without the need for any three-carbon precursors.

That particular four-carbon sugar has dramatic implications for the origins of life. Modern biology uses DNA and RNA to store and transmit genetic information, both of which use a backbone of a five-carbon sugar known as ribose. Ribose, however, is notoriously difficult to synthesize in early-Earth conditions, so astrobiologists have hypothesized that, before modern DNA and RNA, there was a precursor genetic polymer that held the instructions for life.

A leading candidate for that precursor polymer is Threose Nucleic Acid, which uses a four-carbon sugar backbone called threose. And, in the presence of liquid water, ketose sugars like eryththrulose can readily transform into aldose sugars like threose. In other words, the four-carbon sugar that we just found in an interstellar cloud provides a direct chemical link to a possible precursor for DNA.

NASA video detailing the discovery of sugars on Bennu. Credit - NASA Video YouTube Channel

Critically, we already know that large amounts of these sugars were deposited on the Earth during the Late Heavy Bombardment, when early Earth was constantly being pummelled by space rocks. So that means that, by the time Earth’s oceans had cooled enough to support chemistry, plenty of erythrulose and other complex sugars were available to start reacting.

There were some uncertainties in the paper, such as an extremely low detection rate compared to the estimated rate from simulations, but that just means there’s more work to be done. This paper proves, with much certainty, that the potential precursors for the building blocks of life are actively being created in between the stars. All it would take is a delivery mechanism and some serendipity to kickstaff the biological process on a supportive planet, and now we are one step close to completing the picture that proves that.

Learn More:

I. Jimenez-Serra et al - Detection of a four-carbon sugar in interstellar space

UT - Scientists and Senators are Excited About the Sugars Found in the OSIRIS-REx Samples

UT - Sweet! Galactic Molecule Could Point to Alien Life

UT - Scientists Make a Game-Changing Find in the Bennu Asteroid