Today's Image of the Day from the European Space Agency features the spiral galaxy UGC 11397 in the constellation Lyra (The Lyre).



The light captured in this striking image traveled for 250 million years before reaching the NASA/ESA <a href="https://www.earth.com/news/35-years-of-hubble-the-telescope-that-changed-our-view-of-the-universe/">Hubble Space Telescope</a>.



“At first glance, UGC 11397 appears to be an average spiral galaxy: it sports two graceful spiral arms that are illuminated by stars and defined by dark, clumpy clouds of dust,” noted ESA.



“What sets UGC 11397 apart from a typical spiral lies at its center, where a supermassive black hole containing 174 million times the mass of the Sun is growing.”&nbsp;



<h2 class="wp-block-heading" id="h-a-hidden-powerhouse">A hidden powerhouse</h2>



As the <a href="https://www.earth.com/news/largest-oldest-black-hole-jet-ever-seen-is-size-of-three-milky-ways-j1601-3102/">black hole</a> consumes gas, dust, and even entire stars from its surroundings, the infalling material heats up dramatically, producing a dazzling display of energy.&nbsp;



These emissions span the electromagnetic spectrum - from gamma rays to radio waves - and can flare or fade unpredictably.&nbsp;



“But in some galaxies, including UGC 11397, thick clouds of dust hide much of this energetic activity from view in optical light,” explained ESA.



“Despite this, UGC 11397's actively growing black hole was revealed through its bright X-ray emission - high-energy light that can pierce the surrounding dust.”&nbsp;



Its distinctive signature has earned UGC 11397 the classification of a Type 2 Seyfert galaxy. This category describes active galaxies whose central regions are obscured in visible light by a doughnut-shaped cloud of dust and gas.



<h2 class="wp-block-heading" id="h-galaxy-and-black-hole-growth">Galaxy and black hole growth</h2>



“Using Hubble, researchers will study hundreds of galaxies that, like UGC 11397, harbor a supermassive black hole that is gaining mass,” noted ESA.&nbsp;



“The Hubble observations will help researchers weigh nearby supermassive black holes, understand how black holes grew early in the universe’s history, and even study how stars form in the extreme environment found at the very center of a galaxy.”



Studying <a href="https://www.earth.com/news/hidden-galaxies-discovery-would-upend-current-understanding-of-universe/">galaxies</a> like UGC 11397 also offers insight into the mysterious relationship between supermassive black holes and their host galaxies.&nbsp;



Despite residing at the heart of galaxies, these black holes influence their surroundings on a much larger scale, often regulating the formation of stars and even shaping the structure of the galaxy itself.



<h2 class="wp-block-heading" id="h-tracing-black-hole-origins">Tracing black hole origins</h2>



One of the key questions astronomers hope to answer is how these black holes grow so massive in the first place.&nbsp;



While some appear to have formed gradually over billions of years, others - especially those in the early universe - seem to have reached enormous sizes much more quickly. 



Observations of galaxies such as UGC 11397 provide crucial data to test different growth scenarios.



<h2 class="wp-block-heading" id="h-a-clearer-picture-of-cosmic-evolution">A clearer picture of cosmic evolution</h2>



By combining Hubble’s observations with data from other telescopes, including those that detect X-rays and radio waves, researchers can build a more complete picture of how matter behaves around black holes.&nbsp;



This multi-wavelength approach is essential for studying objects obscured by dust, like Type 2 Seyfert galaxies, where optical views alone can be misleading.



Hubble’s sharp vision also allows astronomers to examine the surrounding galactic disk and spiral arms in high detail. 



These structures hold clues about recent star formation, galactic dynamics, and how gas flows toward the center - fueling both star birth and black hole growth.



<h2 class="wp-block-heading" id="h-black-hole-energy-in-active-galaxies">Black hole energy in active galaxies</h2>



In many active <a href="https://www.earth.com/news/thousands-of-galaxies-revealed-in-a-single-webb-image/">galaxies</a>, the energy released by the central black hole can blast out powerful winds or jets that affect star formation. These feedback processes can either shut down or stimulate the creation of new stars, depending on the conditions.&nbsp;



Understanding when and how this feedback occurs is another major goal of Hubble’s ongoing studies.



UGC 11397 is just one of many galaxies being surveyed as part of broader efforts to trace the cosmic history of <a href="https://www.earth.com/news/black-holes-turn-into-white-holes-and-blast-out-matter-and-time-runs-backwards/">black hole</a> activity.&nbsp;



Projects such as these are helping scientists map how common active galactic nuclei are, how their properties evolve over time, and how they relate to galaxy mergers and other large-scale events.



The wealth of information gathered from galaxies like UGC 11397 is not only deepening our understanding of black holes but also refining models of galaxy formation and evolution.&nbsp;



With each new observation, astronomers are piecing together the vast and complex puzzle of how galaxies and their central engines co-evolve across cosmic time.



Image Credit: ESA/Hubble &amp; NASA, M. J. Koss, A. J. Barth



-----



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/">Eric Ralls</a> and Earth.com.



-----

Graceful spiral galaxy hides a dark secret

Today's Image of the Day from the European Space Agency features the spiral galaxy UGC 11397 in the constellation Lyra (The Lyre). The light captured in this striking image traveled for 250 million years before reaching the NASA/ESA Hubble Space Telescope. “At first glance, UGC 11397 appears to be an average spiral galaxy: it sports two graceful spiral arms that are illuminated by stars and defined by dark, clumpy clouds of dust,” noted ESA. “What sets UGC 11397 apart from a typical spiral...

Today's Image of the Day from the European Space Agency features the barred spiral galaxy NGC 3783, which is located about 130 million light-years away in the constellation Centaurus. 



NGC 3783 is also the most prominent of a galaxy group (by the same name) that contains 47 galaxies.&nbsp;



<h2 class="wp-block-heading" id="h-what-are-galaxy-groups">What are galaxy groups?</h2>



“Like galaxy clusters, galaxy groups are aggregates of gravitationally bound galaxies. Galaxy groups, however, are less massive and contain fewer members than <a href="https://www.earth.com/news/titanic-galaxy-cluster-collision-defies-all-current-understanding-of-the-universe/" target="_blank" rel="noreferrer noopener">galaxy clusters</a> do: where galaxy clusters can contain hundreds or even thousands of constituent galaxies, galaxy groups do not typically include more than 50,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



“The Milky Way is actually part of a galaxy group, known as the Local Group, which contains two other large galaxies (Andromeda and the Triangulum galaxy), as well as several dozen satellite and dwarf galaxies.”



<h2 class="wp-block-heading" id="h-a-blue-giant-star">A blue giant star</h2>



The bright object that appears to the right of the galaxy is the star HD 101274. “The perspective in this image makes the star and the galaxy look like close companions, but this is an illusion. HD 101274 lies only about 1,530 light-years from Earth, meaning it is about 85 thousand times closer than NGC 3783,” explained ESA.&nbsp;



The star is part of the NGC 3766 cluster, sometimes referred to as the Pearl Cluster, which is known for its richness in bright stars and its relatively young age.



Characterized by its high temperature and luminosity, HD 101274 is categorized as a blue giant star.



<h2 class="wp-block-heading" id="h-significance-of-blue-giants">Significance of blue giants</h2>



Blue giants are massive stars that have left the main sequence phase of stellar evolution and are burning helium or heavier elements in their cores. These stars are known for their short lifespans relative to smaller stars due to their rapid consumption of nuclear fuel.



<a href="https://www.earth.com/news/dark-stars-scientists-discover-a-new-type-of-star-powered-by-dark-matter/" target="_blank" rel="noreferrer noopener">Stars</a> like HD 101274 are important for astronomers because they help in studying the properties of stellar populations in clusters and the dynamics of stellar evolution in different environments. 



Observations of blue giant stars can provide valuable insights into the characteristics of their atmospheres, internal structures, and the processes occurring within and around them.



<h2 class="wp-block-heading" id="h-active-galactic-nucleus-of-ngc-3783">Active galactic nucleus of NGC 3783</h2>



One of the most interesting aspects of NGC 3783 is that it harbors an active galactic nucleus. This means that its central region is exceptionally luminous, likely due to the presence of a supermassive black hole. 



The black hole is actively accreting material, which emits a substantial amount of radiation as it spirals inward and heats up.



The galaxy has been studied extensively in the ultraviolet and X-ray light spectra to understand better the properties of the accretion disk around the black hole and the complex dynamics of the material surrounding it. 



These studies are crucial for understanding the physics of active galactic nuclei and the role they play in <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">galaxy evolution</a>.



According to ESA, NGC 3783 is a&nbsp;Type I Seyfert galaxy. “In this image it is recorded by Hubble in incredible detail, from its glowing central bar to its narrow, winding arms and the dust threaded through them, thanks to five separate images taken in different wavelengths of light," noted ESA.



“In fact, the galactic center is bright enough to Hubble that it exhibits diffraction spikes, normally only seen on stars such as HD 101274.”



<h2 class="wp-block-heading" id="h-massive-collection-of-galaxy-clusters">Massive collection of galaxy clusters</h2>



The NGC 3783 group is part of the larger Hydra-Centaurus Supercluster, which itself is a massive collection of <a href="https://www.earth.com/news/shapes-of-one-million-galaxies-hint-at-the-universes-origins/" target="_blank" rel="noreferrer noopener">galaxies</a> and galaxy clusters located primarily in the constellations of Hydra and Centaurus.



The NGC 3783 group consists of several galaxies that are gravitationally bound and interact with each other. These interactions can influence the galaxies' evolution through mechanisms like tidal forces and merger events, which can trigger star formation, fuel central black holes, and reshape the galaxies' structures.



Studying the NGC 3783 group helps astronomers understand how <a href="https://www.earth.com/news/ceers-2112-ancient-galaxy-looks-strikingly-similar-to-ours/" target="_blank" rel="noreferrer noopener">galaxies</a> evolve together in a common gravitational environment, offering insights into the dynamics and evolution of structures on cosmic scales.



Image Credit: ESA/Hubble &amp; NASA



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Luminous spiral galaxy and a blue giant star

Today's Image of the Day from the European Space Agency...

Lake Powell reaches its annual peak Today's Image of the Day from <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> features Lake Powell, the second largest water reservoir in the United States, which is spread out across southeastern Utah and northeastern Arizona.

The lake received a boost of meltwater from heavy snowfall in the <a href="https://www.bing.com/search?q=rocky+mountains&amp;form=EDGEAR&amp;qs=PF&amp;cvid=674644e4da2f4b95a90bd9fb9ff4d6f4&amp;cc=US&amp;setlang=en-US&amp;elv=AY3%21uAY7tbNNZGZ2yiGNjfNcI5dP9v9G08gsHOyyYrAtD1gVjqkPwg%211UuyVqyZnxL6RIjN797ckZTtgm%21WEzLIBP7qVBF1BHMDzp*JqDYHj&amp;plvar=0&amp;PC=HCTS">Rocky Mountains</a> earlier this year. However, the effects of global warming, long-term droughts, and increased water demand have left the lake much lower than its full capacity. Lake Powell reaches its annual peak

This image shows Lake Powell near its annual peak on August 31, 2019.

Lake Powell is a man-made reservoir on the Colorado River, straddling the border between Utah and Arizona, United States. Most of Lake Powell, along with Rainbow Bridge National Monument, is located in Utah. It is a major vacation spot visited by approximately two million people every year. It is the second largest man-made reservoir by maximum water capacity in the United States behind Lake Mead, storing 24,322,000 acre feet (3.0001×1010 m3) of water when full. However, due to high water withdrawals for human and agricultural consumption, and because of subsequent droughts in the area, Lake Mead has fallen below Lake Powell in size several times during the 21st century in terms of volume of water, depth and surface area.

--

By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Image Credit: NASA Earth Observatory 

&nbsp;

Lake Powell reaches its annual peak

Lake Powell reaches its annual peak Today's Image of the...

The population of Quito has exploded in size Today's Image of the Day from <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> shows Quito, the capital of Ecuador, which is located in the foothills of the active volcano Pichincha.

Quito is a modern city that was once a crossroads for trade routes through the Andes, the capital of the Incan empire, and a 16th century Spanish colony.

The city now has about two million residents, and exploded in size annually by 3.8 percent from 2000 to 2013.

In 2008, the city was designated as the headquarters of the Union of South American Nations.
The historic centre of Quito is one of the largest, least-altered and best-preserved in the Americas.[ Quito and Kraków, Poland, were the first World Cultural Heritage Sites declared by UNESCO, in 1978. The central square of Quito is located about 25 kilometres (16 mi) south of the equator; the city itself extends to within about 1 kilometre (0.62 mi) of zero latitude. A monument and museum marking the general location of the equator is known locally as la mitad del mundo (the middle of the world), to avoid confusion, as the word Ecuador is Spanish for equator

--

By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Image Credit: NASA Earth Observatory 

&nbsp;

The population of Quito has exploded in size

The population of Quito has exploded in size Today's Image...

Proglacial lake borders the Humboldt Glacier Today's Image of the Day from <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> features a proglacial lake that has formed on the edge of the Humboldt Glacier in northwest Greenland.

The water is also bordered by Washington Land, a deglaciated peninsula that appears reddish-brown.

NASA scientist John Sonntag captured this photograph on September 4, 2019 during an airborne campaign for NASA’s Operation IceBridge. Proglacial lake borders the Humboldt Glacier

“We get to observe the ice surface along the margin without last winter’s snowfall on top, as is usually the case during our spring campaigns,” wrote IceBridge project scientist Joe MacGregor. “That’s both scientifically valuable and - admittedly - often more visually compelling."

The Humboldt Glacier borders the Kane Basin in North West Greenland. Its front is 110 km (68 mi) wide. It has been retreating in the period of observation spanning 1975–2010.
Humboldt Glacier fringes the coast of Peabody Bay from north to south. The McGary Islands lie off the glacier at the southern end of the bay.

Humboldt Glacier (Danish: Humboldt Gletscher) is one of the major glaciers in northern Greenland.
The glacier is named after German naturalist Alexander von Humboldt and is the widest tidewater glacier in the Northern Hemisphere.

--

By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Image Credit: NASA Earth Observatory 

&nbsp;

Proglacial lake borders the Humboldt Glacier

Proglacial lake borders the Humboldt Glacier Today's Image of the...

Tropical Cyclone Hikaa reaches the Arabian Peninsula Today's Image of the Day from <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> features Tropical Cyclone Hikaa, which brought damaging winds and rain into the Arabian Peninsula.

When the storm made landfall over Oman on September 24, it had maximum wind speeds of up to 80 miles per hour. Tropical Cyclone Hikaa reaches the Arabian Peninsula

It is not very common for cyclones to reach the Arabian Sea in the North Indian Ocean. However, in 2018, three significant cyclones pushed all the way up to the Arabian <a href="https://en.wikipedia.org/wiki/Arabian_Peninsula">Peninsula</a>. 

The image was captured by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s <a href="http://www.earth.com/image/sunglint-on-the-mediterranean-sea/">Terra</a> satellite as the outer bands of Hikaa moved over Oman.

Arabian Peninsula is the largest peninsula in the world, at 3,237,500 km2 (1,250,000 sq mi). The Peninsula consists of six countries: Kuwait, Oman, Qatar, Saudi Arabia, the United Arab Emirates, and Yemen. The peninsula formed as a result of the rifting of the Red Sea between 56 and 23 million years ago, and is bordered by the Red Sea to the west and southwest, the Persian Gulf to the northeast, the Levant to the north and the Indian Ocean to the southeast. The peninsula plays a critical geopolitical role in the Arab world due to its vast reserves of oil and natural gas.

--

By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Image Credit: NASA Earth Observatory 

&nbsp;

Tropical Cyclone Hikaa reaches the Arabian Peninsula

Tropical Cyclone Hikaa reaches the Arabian Peninsula Today's Image of...

Arctic sea ice continues its downward trend Today's Image of the Day from <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> shows shrinking sea ice in the Arctic, which reached its annual summer minimum on September 18, 2019.

According to <a href="https://en.wikipedia.org/wiki/NASA">NASA</a>, the extent of ice cover this year has tied 2007 and 2016 as the second lowest in the satellite record, which covers the last four decades. Arctic sea ice continues its downward trend

In 2019, the Arctic sea ice cap shrank to 1.6 million square miles as a result of increasing air and water temperatures.

"This year’s minimum shows that there is no sign that the sea ice cover is rebounding,” said Claire Parkinson, a senior scientist at NASA’s Goddard Space Flight Center. “The long-term trend for the Arctic sea ice extent has been definitively downward.”

The Arctic Ocean is the smallest and shallowest of the world's five major oceans. It is also known as the coldest of all the oceans. The International <a href="http://www.earth.com/news/hydroxychloroquine-is-not-an-effective-covid-19-treatment/">Hydrographic</a> Organization (IHO) recognizes it as an ocean, although some oceanographers call it the Arctic Sea. It is sometimes classified as an estuary of the Atlantic Ocean, and it is also seen as the northernmost part of the all-encompassing World Ocean.

 --

By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Image Credit: NASA Earth Observatory 

&nbsp;

Arctic sea ice continues its downward trend

Arctic sea ice continues its downward trend Today's Image of...

Phytoplankton blooms persist in the North Atlantic Ocean Today's Image of the Day from <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> features blooms of phytoplankton in the North Atlantic Ocean, which have been unusually persistent and far-reaching this month. 

In the ocean near Newfoundland, Canada, the floating organisms had an abundance of sunlight, warm water, and nutrients which allowed them to thrive. Phytoplankton blooms persist in the North Atlantic Ocean

“This is not our typical fall phytoplankton bloom, which would be made up of diatoms,” said marine biologist Cynthia McKenzie of Fisheries and Oceans Canada. She explained that the late bloom is likely a result of “several weeks of sunlight - pretty rare for us in September - and higher than normal temperatures."

The widespread bloom even survived Hurricane Dorian, which stormed through the region in early September. The Atlantic Ocean occupies an elongated, S-shaped basin extending longitudinally between <a title="Europe" href="https://en.wikipedia.org/wiki/Europe">Europe</a> and <a title="Africa" href="https://en.wikipedia.org/wiki/Africa">Africa</a> to the east, and the <a title="Americas" href="https://en.wikipedia.org/wiki/Americas">Americas</a> to the west. As one component of the interconnected <a title="World Ocean" href="https://en.wikipedia.org/wiki/World_Ocean">World Ocean</a>, it is connected in the north to the <a title="Arctic Ocean" href="https://en.wikipedia.org/wiki/Arctic_Ocean">Arctic Ocean</a>, to the <a title="Pacific Ocean" href="https://en.wikipedia.org/wiki/Pacific_Ocean">Pacific Ocean</a> in the southwest, the <a title="Indian Ocean" href="https://en.wikipedia.org/wiki/Indian_Ocean">Indian Ocean</a> in the southeast, and the <a title="Southern Ocean" href="https://en.wikipedia.org/wiki/Southern_Ocean">Southern Ocean</a> in the south (other definitions describe the Atlantic as extending southward to <a title="Antarctica" href="https://en.wikipedia.org/wiki/Antarctica">Antarctica</a>). The Atlantic Ocean is divided into two parts, by the <a title="Equatorial Counter Current" href="https://en.wikipedia.org/wiki/Equatorial_Counter_Current">Equatorial Counter Current</a>, with the North(ern) Atlantic Ocean and the South(ern) Atlantic Ocean at about <a title="8th parallel north" href="https://en.wikipedia.org/wiki/8th_parallel_north">8°N</a>

"I thought the hurricane would have had an effect, but if anything it seems to have fueled its continuation,” said McKenzie. “Most of the heavy wind was on the western part of Newfoundland, so what we had was some wave action which may have brought more nutrients to the bloom from further down in the water column.”

The image was captured on September 1, 2019 by the Moderate Resolution Imaging Spectroradiometer (MODIS) on <a href="https://www.earth.com/video/exciting-nasa-missions-coming-in-2021/">NASA’s</a> Aqua satellite.

 --

By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Image Credit: NASA Earth Observatory 

&nbsp;

Phytoplankton blooms persist in the North Atlantic

Phytoplankton blooms persist in the North Atlantic Ocean Today's Image...

Tropical Storm Imelda brings extreme rainfall to Texas Today's Image of the Day from <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> maps the extreme rainfall in southeast Texas from Tropical Storm Imelda.

The system pulled in heat and moisture from the Gulf of Mexico before moving very slowly over Houston and Beaumont, causing damaging flash floods.

The brightest areas on the map represent the highest rainfall amounts, with some places receiving as much as 30 inches from September 17 to September 20, 2019. 

The data comes from the Integrated Multi-Satellite Retrievals for the Global Precipitation Measurement (GPM) mission.Tropical Storm Imelda was the fifth-wettest tropical cyclone on record in the continental United States, causing devastating and record-breaking floods in southeast Texas. The eleventh tropical cyclone and ninth named storm of the 2019 Atlantic hurricane season, Imelda formed out of an upper-level low that developed in the Gulf of Mexico and moved westward. Little development occurred until the system was near the Texas coastline, where it rapidly developed into a tropical storm before moving ashore shortly afterward on September 17. Imelda weakened after landfall, but continued bringing large amounts of flooding rain to Texas and Louisiana, before dissipating on September 21.

--

By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Image Credit: NASA Earth Observatory 

&nbsp;

Tropical Storm Imelda brings extreme rainfall to Texas

Tropical Storm Imelda brings extreme rainfall to Texas Today's Image...

Today's Image of the Day from <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> features Kuwait Bay, where one of the world's largest bridges has been constructed to connect Bay Island North and Bay Island South.

The 30-mile Sheikh Jaber Al-Ahmad Al-Sabah Causeway opened in May after five years of planning and more than three billion dollars in costs.

Construction companies made an effort to preserve the ecosystem near the bay, specifically for green tiger shrimp. To lure the shrimp away from the site, an alternative breeding area was created with 1,000 rock and reef blocks. 

The photograph was captured on September 8, 2019 by the Operational Land Imager on Landsat 8.

  --

By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Image Credit: NASA Earth Observatory 

&nbsp;

Massive bridge opens in Kuwait Bay

Today's Image of the Day from NASA Earth Observatory features...

How did life on Earth begin? People have been asking that for ages. The answers remain scattered across rocks, oceans, and ancient landscapes. One clue hides in an essential ingredient for life - phosphorus.



Phosphorus is everywhere in living things. It holds together DNA and RNA. It forms the framework of cell membranes. No life can grow or function without it. 



Yet, phosphorus mostly stays trapped in rocks. It hides inside phosphate minerals, which barely dissolve in water. That raises an old and puzzling question: how did early Earth get enough phosphorus to <a href="https://www.earth.com/news/scientists-discover-one-simple-rule-that-explains-all-life-on-earth-bioregions/">spark</a> life?



Yuya Tsukamoto and Takeshi Kakegawa from <a href="https://www.tohoku.ac.jp/en/" target="_blank" rel="noreferrer noopener">Tohoku University</a> took that question seriously. They decided to look where most people wouldn’t - deep under the sea, in rocks that are billions of years old.



<h2 class="wp-block-heading" id="h-key-element-for-life-on-earth">Key element for life on Earth</h2>



The researchers focused on the Pilbara Craton in Western Australia, which holds some of the oldest known seafloor rocks. 



The rocks are an astonishing 3.455 billion years old. The team's discovery wasn’t subtle. It jumped out from the data.



"We analyzed 3.455-billion-year-old basaltic seafloor rocks in drill core samples recovered from the Pilbara Craton, Western Australia, discovering that P was significantly leached from the hydrothermally altered rocks compared to the least altered rocks," explained Tsukamoto.



He noted that further mineralogical analyses indicated that phosphate minerals had undergone dissolution in rocks where P was depleted. 



Simply put, hot fluids moved through these rocks and pulled phosphorus out. That phosphorus didn’t just disappear. It entered the surrounding seawater, turning parts of the ocean into phosphorus-rich zones.



<h2 class="wp-block-heading" id="h-tracking-the-source-of-phosphorus">Tracking the source of phosphorus </h2>



The rocks alone didn’t tell the whole story. The team wanted to understand what made this phosphorus release possible. They uncovered two kinds of hydrothermal fluids that shaped this <a href="https://www.earth.com/news/third-state-of-existence-beyond-life-and-death-confirmed-by-scientists/">process</a>.



One type was hot, rich in sulfur, and capable of breaking down minerals quickly. The other was more surprising - mildly acidic to alkaline fluids at lower temperatures. 



These fluids were common in the Archean era because Earth’s atmosphere back then was filled with carbon dioxide. That unique atmosphere made these fluids react in unexpected ways with the rocks.



The result? Massive amounts of dissolved phosphate in the water. The numbers were shocking. These fluids could carry up to 2 millimolar phosphate - nearly 1,000 times higher than what’s found in modern seawater.



Suddenly, early <a href="https://www.earth.com/news/luca-last-universal-common-ancestor-progenitor-all-life-on-earth/">Earth</a> wasn’t a barren place. Its oceans were filled with phosphorus.



<h2 class="wp-block-heading" id="h-earth-s-oceans-held-elements-for-life">Earth’s oceans held elements for life</h2>



This wasn’t just a chemistry experiment. The results changed how scientists think about early Earth. The researchers calculated how much phosphorus these underwater systems could release. 



The findings were stunning. The amount of phosphorus released into the oceans by these hydrothermal systems could match, or even exceed, the amount entering modern oceans through rivers and weathering of land rocks.



"Importantly, this study provides direct evidence that submarine hydrothermal activity leached P from seafloor basaltic rocks and quantifies the potential P flux from these hydrothermal systems to the early ocean," adds Tsukamoto.



Imagine ancient oceans filled with nutrients. These phosphorus-rich waters may have supported some of Earth’s earliest microbial life. 



The ancient communities didn’t need a vast, lush <a href="https://www.earth.com/news/rocks-reveal-the-turning-point-when-oxygen-changed-earth-forever/">planet</a>. It only needed these hidden underwater environments to get started.



<h2 class="wp-block-heading" id="h-hot-springs-and-hidden-worlds-on-land">Hot springs and hidden worlds on land</h2>



The study also pointed to something beyond the oceans - hot springs on land. Hydrothermal systems aren’t just found under the sea. They exist on land too, in places like hot springs.



These environments might have also released phosphorus on early Earth. That means life’s building blocks weren’t limited to deep-sea vents. They could have existed in steaming pools on land.



This opens the door for more discoveries. Scientists now plan to study how phosphate behaves in rocks across different periods of Earth’s history. By tracing phosphorus through time, they hope to unlock new chapters of Earth’s story.



The message is clear: Life’s ingredients may have come from places on Earth we’ve only just begun to explore. Deep beneath the waves, within rocks touched by ancient fluids, the story of life may have quietly begun.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/abs/pii/S0016703725003266?via%3Dihub" target="_blank" rel="noreferrer noopener">Geochimica et Cosmochimica Acta</a>.



-----



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by <a href="https://www.earth.com/author/eralls/">Eric Ralls</a> and Earth.com.



-----

Earth may have always held the key ingredients for life

How did life on Earth begin? People have been asking...

cinco-microhabitos-neurociencia-aprender-mas-rapido-recordar-mej

Varicose veins bulge and twist across the calves of up to 30 percent of adults, a reminder that blood sometimes pools instead of flowing home to the heart. When sluggish blood flow lingers, clots can form and, in rare cases, travel to the lungs or brain.



Centuries ago physicians in China brewed teas from <a href="https://www.missouribotanicalgarden.org/PlantFinder/PlantFinderDetails.aspx?kempercode=z990" target="_blank" rel="noreferrer noopener">Ginkgo biloba</a> leaves to sharpen memory. Today researchers wonder whether the same ginkgo leaves might support weary leg veins and cut the risk of small, yet dangerous, blood clots.



<h2 class="wp-block-heading" id="h-why-circulation-can-falter">Why circulation can falter</h2>



Blood rising from the feet must fight gravity, and faulty valves can leave veins stretched and valves leaky. The lingering pressure distends vein walls, encourages <a href="https://www.earth.com/news/fasting-helps-the-body-fight-inflammation-and-chronic-diseases/">inflammation</a>, and slows platelet aggregation, the first step toward clotting.



Slow venous return creates the setting for deep‑vein thrombosis as well as the aching, throbbing symptoms many patients feel after a day of standing. 



That overlap has pushed vascular specialists toward plant‑based compounds that might tone the vein wall and limit sticky platelets.



After logging stroke cases at Xuanwu Hospital in Beijing, neurologist <a href="https://www.researchgate.net/scientific-contributions/Xiangqian-Huang-2265510495" target="_blank" rel="noreferrer noopener">Xiangqian Huang</a> of <a href="https://ccmu.cucas.cn/" target="_blank" rel="noreferrer noopener">Capital Medical University</a> began probing ginkgo’s effects on clot behavior in the brain, work that now informs leg‑vein research.



<h2 class="wp-block-heading" id="h-ginkgo-leaves-and-blood-flow">Ginkgo leaves and blood flow</h2>



Ginkgo extract made <a href="https://www.earth.com/news/drinking-from-plastic-bottles-linked-to-high-blood-pressure-and-heart-problems/">blood platelets</a> less sticky when triggered by one type of chemical but didn’t have much effect when triggered by another. 



Dr. Xiangqian Huang and the team also noticed that blood took slightly longer to clot after treatment with the extract.



The leaf contains natural compounds that seem to interact with enzymes responsible for forming clots. 



In a 2025 animal <a href="https://pubmed.ncbi.nlm.nih.gov/40462336/" target="_blank" rel="noreferrer noopener">study</a>, researchers found that ginkgo reduced damage inside blood vessels in rats with clotting problems and slightly increased the time it took for their blood to clot. 



<h2 class="wp-block-heading" id="h-insights-from-a-beijing-stroke-ward">Insights from a Beijing stroke ward</h2>



Huang’s real‑world study followed 99 patients for five days. Among stroke survivors who received ginkgo plus baby <a href="https://www.earth.com/news/daily-aspirin-use-strongly-tied-to-colorectal-cancer-prevention/">aspirin</a>, arachidonic‑acid platelet aggregation fell more than in peers on aspirin alone, while major bleeding did not rise.



Minor nose or gum bleeds surfaced in four of thirty‑three combination patients, a signal that enhanced anticoagulation deserves monitoring. No severe hemorrhages occurred, suggesting short‑term safety when doses stay low.



The design also enrolled participants with internal jugular venous stenosis, a group whose <a href="https://www.earth.com/news/artificial-sweetener-erythritol-sugar-substitute-linked-to-blood-clots-heart-disease/">clots</a> mirror those in leg veins. 



In that arm ginkgo alone curbed blood platelet stickiness within 24 hours, and the effect held steady through day five.



<h2 class="wp-block-heading" id="h-aspirin-ginkgo-and-blood-clots">Aspirin, ginkgo, and blood clots</h2>



A team of <a href="https://pubmed.ncbi.nlm.nih.gov/17982321/" target="_blank" rel="noreferrer noopener">scientists</a> led by <a href="https://med.stanford.edu/profiles/christopher-gardner" target="_blank" rel="noreferrer noopener">Christopher Gardner</a> from <a href="https://med.stanford.edu/" target="_blank" rel="noreferrer noopener">Stanford Department of Medicine</a> examined the potential adverse effects of concomitant aspirin and Ginkgo biloba on blood platelet function after giving the duo to older adults for four weeks. The worry was that the herbs might blunt or boost common drugs. 



Gardner and colleagues detected no dangerous bleeding, yet laboratory tests showed additive platelet inhibition, suggesting that low‑dose pairings could protect high‑risk patients who cannot tolerate stronger pharmaceuticals. 



Doctors, however, should adjust regimens around surgeries or when other blood thinners enter the mix.



Because the leaf targets arachidonic‑acid pathways that aspirin already touches, the partnership makes pharmacologic sense. 



Still, anyone taking nonsteroidal anti‑inflammatory drugs should discuss timing and dosage to avoid stacking identical mechanisms.



<h2 class="wp-block-heading" id="h-helping-legs-feel-lighter">Helping legs feel lighter</h2>



Deep veins are not the only place where endothelial cells detach under strain. 



In a classic double‑blind trial, scientists found that a capsule combining ginkgo, troxerutin, and heptaminol cut circulating endothelial cell counts by 14.5 percent in patients with chronic varicose veins, placebo achieved only 8.4 percent.



<a href="https://www.ncbi.nlm.nih.gov/books/NBK26848/" target="_blank" rel="noreferrer noopener">Endothelial cells</a> are early barometers of vein injury, so their decline hints at real structural healing. 



Participants also reported reduced ankle swelling and night cramps, benefits echoed by later Russian and Italian studies that tracked leg circumference.



Modern <a href="https://journals.sagepub.com/home/phl" target="_blank" rel="noreferrer noopener">phlebology</a> still relies on compression stockings and laser ablation, yet many sufferers ask for gentler first steps. 



A standardized ginkgo formula, already licensed for vascular disorders in parts of Europe, may slot neatly between lifestyle changes and invasive procedures.



<h2 class="wp-block-heading" id="h-blood-clot-prevention-with-ginkgo">Blood clot prevention with ginkgo</h2>



Yang’s rat data showed lighter <a href="https://www.earth.com/news/cause-of-strokes-cervical-artery-dissection-has-increased-400-percent-since-2005/">clots</a>, higher nitric‑oxide levels, and longer clotting times after gavage with 60 milligrams per kilogram of extract. 



Nitric oxide relaxes vessel walls and counters platelet stickiness, aligning with human data from stroke and vein clinics.



<a href="https://pubmed.ncbi.nlm.nih.gov/26030402/" target="_blank" rel="noreferrer noopener">Network‑pharmacology</a> maps place AKT1, ALB, and TNF at the center of ginkgo’s target web. Those same genes regulate inflammation, suggesting that the tree’s reach extends beyond platelets to the very lining of our veins.



Because oxidative stress weakens venous valves, the antioxidant side of the extract warrants equal attention. 



Flavonols scavenge free radicals, potentially slowing the progressive dilation that makes early spider veins blossom into rope‑like cords.



<h2 class="wp-block-heading" id="h-talking-with-your-doctor">Talking with your doctor</h2>



Ginkgo supplements crowd store shelves, yet extracts used in clinical trials are highly standardized. Look for<a href="https://pubmed.ncbi.nlm.nih.gov/12757407/" target="_blank" rel="noreferrer noopener"> EGb 761</a> or products specifying at least 24 percent flavonol glycosides and 6 percent terpene lactones.



Patients on warfarin, <a href="https://www.ahajournals.org/doi/10.1161/JAHA.120.017559" target="_blank" rel="noreferrer noopener">direct oral anticoagulants</a>, or upcoming dental work should alert their clinicians before starting any form of ginkgo. 



Health professionals may stagger doses, check clotting labs, or advise pausing the herb to keep bleeding risk low.



For those with aching calves and a family history of clots, discussing ginkgo as an adjunct to compression or low‑intensity exercise could make sense. 



Evidence remains preliminary, yet the plant’s dual action on platelets and vein walls is steadily moving from bench to bedside.



Future multicenter trials ought to track long‑term safety and measure quality‑of‑life changes such as heaviness, itch, and nightly restlessness. If findings stay positive, an ancient tree might soon earn a modern role in vascular medicine.



The study is published in <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC11803947/" target="_blank" rel="noreferrer noopener">Thrombosis Journal</a>.



-----



Like what you read?<a href="https://www.earth.com/subscribe/"> Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



Check us out on<a href="https://www.earth.com/earthsnap/"> EarthSnap</a>, a free app brought to you by<a href="https://www.earth.com/author/eralls/"> Eric Ralls</a> and Earth.com.



-----

Leaves from this popular tree may improve circulation and prevent blood clots

Varicose veins bulge and twist across the calves of up...

Astronomers poring over new data from the James Webb Space Telescope have reported the most compelling hints yet that “dark stars,” cosmic behemoths fed by dark matter, really existed. 



A new <a href="https://arxiv.org/pdf/2505.06101" target="_blank" rel="noreferrer noopener">analysis</a> of five ultra‑distant objects shows spectra and shapes that match simulations of dark <a href="https://www.earth.com/news/tiny-star-giant-gas-planet-toi-6894b-breaks-current-planetary-formation-rules/">stars</a> rather than ordinary fusion‑powered suns.



The candidates sit more than 13 billion light‑years away, meaning their light left them when the universe was only a few hundred million years old. 



The dark star <a href="https://arxiv.org/abs/0705.0521" target="_blank" rel="noreferrer noopener">concept</a> was first introduced in 2007 by Katherine Freese and colleagues at the <a href="https://www.utexas.edu/" target="_blank" rel="noreferrer noopener">University of Texas at Austin</a>.



<h2 class="wp-block-heading" id="h-dark-matter-powering-giant-stars">Dark matter powering giant stars</h2>



Dark matter accounts for about 85 percent of the <a href="https://www.earth.com/news/planet-forming-disks-surrounding-stars-often-last-much-longer-than-expected/">universe</a>’s mass but reveals itself only through gravity. Two decades of underground detectors have yet to capture a single dark‑matter particle, yet its invisible pull sculpts galaxies and galaxy clusters.



Freese proposed that in the first halos of gas, self‑annihilating dark‑matter particles could generate heat faster than the gas could cool, inflating stars that grow to millions of solar masses without ever igniting fusion. 



Once the local dark‑matter reservoir ran out, the stars would collapse, possibly forming black holes hefty enough to seed the earliest quasars.



Webb's infrared vision extends far enough redward to catch such ancient, swollen <a href="https://www.earth.com/news/massive-new-super-earth-kepler-725c-found-in-habitable-zone-around-its-star/">stars</a>, and its sensors have already revealed dozens of unexpectedly bright objects in the epoch known as Cosmic Dawn.



<h2 class="wp-block-heading" id="h-webb-spotted-strange-ancient-stars">Webb spotted strange ancient stars</h2>



Freese’s team studied <a href="https://science.nasa.gov/missions/webb/nasas-webb-sees-galaxy-mysteriously-clearing-fog-of-early-universe/" target="_blank" rel="noreferrer noopener">JADES‑GS‑z11‑0, JADES‑GS‑z13‑0</a> and three even more distant specks, finding that each could be explained by a single dark star rather than a whole infant galaxy.



“If it’s real, then I don’t know how else you’d explain it other than with a dark star,” said Freese. A second clue comes from a tentative absorption dip at rest‑frame <a href="https://ned.ipac.caltech.edu/level5/Sept15/Johnson/Johnson4.html" target="_blank" rel="noreferrer noopener">1,640 Å</a>, the signature of <a href="https://arxiv.org/abs/1110.6202" target="_blank" rel="noreferrer noopener">He II</a>, that appears in one spectrum and is predicted only for dark‑star atmospheres.



<h2 class="wp-block-heading" id="h-some-doubt-the-dark-star-idea">Some doubt the dark star idea</h2>



Daniel Whalen of the <a href="https://www.port.ac.uk/" target="_blank" rel="noreferrer noopener">University of Portsmouth</a> studies massive stars forming without dark matter. He is not convinced about the existence of dark stars.



"They ignore an entire body of literature on the formation of supermassive primordial stars, some of which could give signatures very similar to the signatures that they show,” said Whalen. 



Whalen argues that rapid gas accretion alone can inflate stars to a million suns, and that Webb’s photometry cannot yet distinguish between such hot leviathans and Freese’s cooler, puffier dark stars.



<h2 class="wp-block-heading" id="h-dark-stars-may-explain-early-black-holes">Dark stars may explain early black holes</h2>



The debate matters because JWST and Chandra recently found a black hole in <a href="https://www.nasa.gov/missions/chandra/nasa-telescopes-discover-record-breaking-black-hole/" target="_blank" rel="noreferrer noopener">galaxy UHZ‑1</a> whose mass approaches ten billion Suns just 500 million years after the big bang. Traditional growth models struggle to build such giants so fast. 



A dark star collapsing after millions of years would supply a head start that ordinary <a href="https://astronomy.swin.edu.au/cosmos/*/Population+III" target="_blank" rel="noreferrer noopener">Population III stars</a> cannot match.



Supermassive primordial stars could also create big seeds, but they rely on rare <a href="https://www.earth.com/news/first-direct-image-cosmic-web-filaments-hidden-highways-universe-framework/">conditions</a> - pristine gas streams and intense ultraviolet fields - that may not occur often enough to explain the abundance of early quasars.



<h2 class="wp-block-heading" id="h-light-signals-may-prove-dark-stars">Light signals may prove dark stars</h2>



The dark star candidates give off light that’s much cooler and puffier than expected from galaxies or fusion‑based suns, which means their spectral energy distribution should look unique. 



One telltale feature would be an absorption dip caused by <a href="https://physics.nist.gov/PhysRefData/Handbook/Tables/heliumtable4.htm" target="_blank" rel="noreferrer noopener">singly ionized helium</a>, known as He II, at 1,640 Å. If confirmed, this dip could act like a fingerprint. In the Webb spectrum of <a href="https://esawebb.org/images/jades4/" target="_blank" rel="noreferrer noopener">JADES‑GS‑z14‑0</a>, researchers spotted a faint signal that lines up with where the He II dip should appear.



However, the signal‑to‑noise ratio was just 2.4, which is barely above the threshold of what’s considered statistically meaningful. That makes it too early to declare the case closed. 



On top of that, observations from <a href="https://www.almaobservatory.org/en/home/" target="_blank" rel="noreferrer noopener">ALMA</a> spotted oxygen nearby, which shouldn't be present in pure dark stars. This could mean the dark star is part of a system with other stars, or something more complex is going on.



<h2 class="wp-block-heading" id="h-future-research">Future research</h2>



One wrinkle is that ALMA detects oxygen in one candidate’s vicinity, implying metal‑rich companions that classic dark‑star theory does not expect. 



Future deep spectra will need to confirm whether the He II feature is genuine and whether metals truly permeate the system.



Webb keeps adding targets, and the <a href="https://roman.gsfc.nasa.gov/" target="_blank" rel="noreferrer noopener">Roman Space Telescope</a> will survey wider areas, potentially catching hundreds of dark‑star‑like objects at redshifts beyond 14. 



For now, dark stars remain an intriguing, if unproven, explanation for several mysteries in the early universe.



The study is published in the journal <a href="https://arxiv.org/html/2505.06101v1" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



Image Credit: Pierluigi Rinaldi / Rafael Navarro-Carrera / Pablo G. Pérez-González



-----



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by <a href="https://www.earth.com/author/eralls/">Eric Ralls</a> and Earth.com.



-----

Signs of 'dark stars' discovered in the early universe

Astronomers poring over new data from the James Webb Space...

Pregnancy is one of nature’s most intricate achievements. At its core lies a delicate exchange between mother and fetus, where two genetically distinct bodies maintain close contact and constant communication. 



This connection happens at the fetal-maternal interface - the meeting point between a baby’s placenta and the mother’s uterus - and it plays a critical role in allowing pregnancies to last long enough for full fetal development.



A new study by researchers from the <a href="https://www.univie.ac.at/en/">University of Vienna</a> explores how this unique interface came to be. 



The research sheds new light on how cellular communication and cooperation evolved over millions of years to support successful pregnancies in <a href="https://www.earth.com/news/ancient-mammals-bulked-up-to-deal-with-drastic-changes/">placental mammals</a>, including humans.



<h2 class="wp-block-heading" id="h-what-mammals-teach-us-about-pregnancy">What mammals teach us about pregnancy</h2>



The team examined single-cell transcriptomes - snapshots of active genes in individual cells - across six mammalian species. 



The species included humans, macaques, mice, guinea pigs, the tenrec (an early placental mammal), and the opossum (a marsupial whose evolutionary path diverged before complex placentas emerged). 



The goal was to understand how the different cells at the fetal-maternal interface evolved and how their communication systems work.



The experts focused on two major players: placenta cells from the <a href="https://www.earth.com/news/the-battle-of-the-sexes-begins-in-the-womb/">fetus</a> that invade maternal tissue, and uterine stromal cells from the mother that respond to this invasion. These interactions need to be tightly controlled. 



If the connection is too weak, the fetus may not get the nutrients it needs. But if it's too strong, the mother's immune system might recognize the fetus as foreign and attack it.



<h2 class="wp-block-heading" id="h-the-genetic-memory-behind-pregnancy">The genetic memory behind pregnancy</h2>



Using powerful molecular tools, the team uncovered genetic signatures tied to specific cell types and their unique functions. 



One striking discovery was a shared genetic signature linked to the invasive behavior of fetal placenta cells - and this signature has remained in place for over 100 million years.



This challenges the long-held idea that these invasive cells are unique to <a href="https://www.earth.com/news/human-development-has-a-pause-button/">humans</a>. Instead, they appear to be a deeply rooted feature of mammalian biology. 



Meanwhile, maternal cells weren’t standing still either. In placental mammals (but not in marsupials), new forms of hormone production emerged. 



These hormonal innovations likely played a key role in extending pregnancy durations, giving developing babies more time in the womb. It also suggests that the evolution of pregnancy might have been shaped by a give-and-take between mother and fetus.



<h2 class="wp-block-heading" id="h-cooperation-or-conflict">Cooperation or conflict?</h2>



To understand the tug-of-war - or possible teamwork - between <a href="https://www.earth.com/news/moms-pass-a-unique-set-of-breast-milk-antibodies-to-her-baby/">mother</a> and fetus, the researchers tested two evolutionary theories.



The first theory, called the “disambiguation hypothesis,” proposes that over time, certain hormonal signals became clearly assigned to either the mother or the fetus. This helps prevent confusion or manipulation between the two. 



The results backed this theory up: hormones like WNT proteins, immune signals, and steroid hormones could be clearly traced to one source or the other.



<h2 class="wp-block-heading" id="h-coordination-between-mother-and-fetus">Coordination between mother and fetus</h2>



The second theory, known as the “escalation hypothesis,” sees pregnancy as an arms race. Here, the <a href="https://www.earth.com/news/pregnancy-stress-may-have-lasting-effects-on-fetal-development/">fetus</a> might ramp up growth signals while the mother tries to keep them in check.



Some evidence supported this theory, especially with genes like IGF2 that control growth. But overall, the data pointed more toward cooperation than conflict.



“These findings suggest that evolution may have favored more coordination between mother and fetus than previously assumed,” said Daniel J. Stadtmauer, lead author of the study. 



“The so-called mother-fetus power struggle appears to be limited to specific genetic regions. Rather than asking whether pregnancy as a whole is conflict or cooperation, a more useful question may be: where is the conflict?”



<h2 class="wp-block-heading" id="h-understanding-the-origins-of-pregnancy">Understanding the origins of pregnancy</h2>



The real breakthrough came from combining two techniques: single-cell transcriptomics and evolutionary modeling. 



This allowed the team to compare gene activity in different<a href="https://www.earth.com/news/the-hidden-struggles-of-pregnant-humpback-whales/"> species</a> and even make predictions about what those interactions looked like in long-extinct ancestors.



“Our approach opens a new window into the evolution of complex biological systems - from individual cells to entire tissues,” said Silvia Basanta, co–first author of the study. 



The research not only offers insights into how pregnancy evolved, but it could also help us better understand - and perhaps one day improve - how we treat complications during pregnancy.



By zooming in on the cellular scale, the team has given us a clearer picture of the deep evolutionary roots of one of life's most remarkable biological collaborations.



The full study was published in the journal <a href="https://www.nature.com/articles/s41559-025-02748-x">Nature Ecology &amp; Evolution</a>.



-----



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by <a href="https://www.earth.com/author/eralls/">Eric Ralls</a> and Earth.com.



-----

Ancient secrets of a modern miracle: How pregnancy evolved

Pregnancy is one of nature’s most intricate achievements. At its...

Drones deliver packages, inspect bridges, and shoot video, but their high‑pitched whine still irritates neighbors and wildlife. Engineers want rotor shapes that hush the noise without draining batteries.



One possible design comes from a 15th‑century notebook by <a href="https://www.leonardodavinci.net/" target="_blank" rel="noreferrer noopener">Leonardo da Vinci,</a> a continuous spiral rotor he called an “aerial screw." New simulations suggest that it can lift a modern drone while saving power.



Rajat Mittal of <a href="https://www.jhu.edu/" target="_blank" rel="noreferrer noopener">Johns Hopkins University</a> led a study that puts the Renaissance sketch to the test.



<h2 class="wp-block-heading" id="h-da-vinci-s-drone-idea">Da Vinci’s drone idea</h2>



Leonardo da Vinci pursued flight long before airplanes - sketching wings, parachutes, and the spiral screw that inspired the helicopter dream. His notebooks show careful airflow doodles even though the science of lift would not be formalized for centuries.



The spiral looks like an overgrown <a href="https://www.britannica.com/technology/Archimedes-screw" target="_blank" rel="noreferrer noopener">Archimedes' screw</a>, a water‑lifting helix from ancient Greece, except it twists upward to push air downward. Historians note that da Vinci often borrowed proven mechanical ideas for new purposes.



Human muscle could never spin the heavy canvas screw fast enough, so the contraption stayed on paper. Lightweight electric <a href="https://www.earth.com/news/earthcares-first-year-surprising-climate-clues-unveiled-from-space/">motors</a> and carbon‑fiber skins finally give the old idea a chance to rise. 



A small <a href="https://vfs.umd.edu/assets/downloads/2020_elico.pdf">prototype</a> built at the University of Maryland in 2020 confirmed the screw can generate lift, though efficiency data were thin. The new work attacks that gap with supercomputer fidelity.



<h2 class="wp-block-heading" id="h-testing-the-spiral-rotor">Testing the spiral rotor</h2>



Mittal’s team rebuilt the rotor in code and ran direct numerical simulations. The model tracked every swirl of air around the spiral as it hovered. 



The exercise probed aerodynamics and aeroacoustics at several Reynolds number values - a parameter that links size, speed, and viscosity. Matching those numbers to typical small drones let the results translate to real rotors.



“We were surprised,” said Mittal. The screw needed roughly 20 percent less mechanical <a href="https://www.earth.com/news/cloud-engineering-can-temporarily-cool-our-planet/">power</a> than a two‑blade prop to hold the same weight. 



Because the spiral presents more surface but turns slower, the simulation predicted a weaker pressure pulse and therefore a quieter signature. Earlier modeling of large‑area insect‑inspired rotors hinted at the same trend.



<h2 class="wp-block-heading" id="h-spiral-rotors-can-reduce-drone-noise">Spiral rotors can reduce drone noise</h2>



Community annoyance rises sharply when drone flights repeat every few minutes, a NASA laboratory <a href="https://ntrs.nasa.gov/api/citations/20240001863/downloads/Vaughn_2024_03_ATWG_05_ASA_v3.pdf" target="_blank" rel="noreferrer noopener">study</a> found last year. People rated even modest noise harsher when it came in clusters. 



Complaints back that up; the <a href="https://www.faa.gov/noise/inquiries/noise-complaint-inquiry-policy" target="_blank" rel="noreferrer noopener">Federal Aviation Administration</a> logged 8,746 aircraft noise reports in the first quarter of 2025, with just 60 residents submitting 72 percent of them. Drones are included in the totals for many cities.



“It doesn’t have to be the da Vinci design to achieve this, but it is nice that da Vinci’s does,” said <a href="https://www.bu.edu/eng/profile/sheryl-grace-ph-d/" target="_blank" rel="noreferrer noopener">Sheryl Grace</a> of Boston University. 



A rotor that spins 1,500 revolutions per minute slower cuts broadband noise roughly in half, according to the new simulation. That drop matters more than raw loudness because the whine often falls in the most sensitive range of human hearing.



<h2 class="wp-block-heading" id="h-da-vinci-s-design-for-drone-deliveries">Da Vinci’s design for drone deliveries</h2>



Drone couriers face strict <a href="https://www.earth.com/news/study-consciousness-is-a-quantum-process-connecting-us-all-to-the-entire-universe/">noise</a> limits near hospitals, schools, and wildlife preserves. A built‑in silencer would lighten regulatory burdens without adding extra shrouds or foam. 



The spiral also trims energy burn, extending range or freeing capacity for heavier batteries. Efficiency gains remain welcome while lithium prices climb.



Challenges persist: forward flight introduces side loads the screw has not yet faced, and the spiral adds mass compared with thin blades. Structural tests will need to prove the membrane can survive sudden gusts. 



Even so, quieter fleets could reduce the buffer zones that push drone depots to industrial parks and away from customers, shrinking the road miles trucks must still cover.



<h2 class="wp-block-heading" id="h-future-plans-for-spiral-rotors">Future plans for spiral rotors</h2>



Mittal’s group plans to tweak pitch, taper, and turn count to squeeze more lift per square inch while keeping the low hum. The same code that vetted the classic shape can rank new variants in days instead of months. 



Lab prototypes will follow, spun by off‑the‑shelf hobby motors to compare thrust and decibels against standard props. Microphones will map the sound field in three‑dimensional space.



If the results stay promising, an industry partner could bolt a spiral onto a quadcopter for outdoor trials under current <a href="https://www.ecfr.gov/current/title-14/chapter-I/subchapter-F/part-107" target="_blank" rel="noreferrer noopener">Part 107 rules</a>. City officials watching Amazon’s recent delivery setbacks know neighbors care more about noise than novelty. 



Leonardo da Vinci never flew, yet his spiral might help future drones coexist with people and birds in crowded skies.



The study is published in the journal <a href="https://arxiv.org/html/2506.10223v1" target="_blank" rel="noreferrer noopener">arXiv</a>.



-----



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by <a href="https://www.earth.com/author/eralls/">Eric Ralls</a> and Earth.com.



-----

Leonardo da Vinci design solves modern drone noise problems

Drones deliver packages, inspect bridges, and shoot video, but their...

Scientists are transforming chocolate into a functional food by infusing it with probiotics and prebiotics, aiming to create a treat that satisfies cravings while supporting gut health. 



The challenge lies in maintaining chocolate's beloved texture and flavor while adding health benefits.



<figure class="wp-block-embed aligncenter is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio"><div class="wp-block-embed__wrapper">
https://youtu.be/Ug657J67iEo?si=w96YjGMsg939LD_3
</div></figure>



Probiotics - beneficial microbes that balance gut bacteria and aid digestion - are typically fragile and can be destroyed by stomach acid or processing. 



Prebiotics act as food for these microbes, helping them thrive. Together, they form "synbiotics," a powerful health combination.



Researchers Smriti Gaur and Shubhi Singh from India's Jaypee Institute of Information Technology took an innovative approach, using natural prebiotics like corn and honey instead of complex processing methods. 



They created five chocolate varieties: a control and four synbiotic versions containing different combinations of prebiotics, probiotics (Lactobacillus strains), and flavor enhancers (cinnamon or orange).



Laboratory simulations of human digestion showed the probiotics remained viable for over five hours, suggesting they could survive long enough to benefit gut health.



Taste tests were positive, with researchers particularly enjoying the orange-flavored variety, describing it as having "vibrant citrus notes" complementing the "rich cocoa" with a "luxurious" texture.



This research represents just the beginning. With further refinement of strains, textures, and flavors, chocolate could evolve beyond mere indulgence to become a functional food that nourishes while it delights.



The study is published in the journal <a href="https://pubs.acs.org/doi/10.1021/acsfoodscitech.4c00741" target="_blank" rel="noreferrer noopener">ACS Food Science &amp; Technology</a>.

Is chocolate the next nutritional powerhouse?

Scientists are transforming chocolate into a functional food by infusing...

<div class="wp-block-sendtonews-playerselector">[sendtonews key="0ynNMYkMKa-2340414-12187" type="single"]</div>



Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Nushagak Bay, a large estuary in southwest Alaska. Nushagak runs mainly north to south and exits in Bristol Bay, a large body of water in the Bering Sea.



"The bay is primarily fed by the Nushagak River, which begins in the Alaska Range and flows southwest approximately 450 km. The bay is also fed by several additional rivers including the Wood, Igushik, Snake and Weary rivers," says ESA.



"The dark colors of the Nushagak River are most likely due to tannins or lignins (chemical substances found in plants). Tannins and lignins from roots, leaves, seeds, bark and soil can leach into the water and give it a brown or even black colour. The sediments then flow southwards where it is mixed with the bluer waters of the bay."



Video/ Image Credit: ESA



---



By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Nushagak Bay in southwest Alaska

[sendtonews key="0ynNMYkMKa-2340414-12187" type="single"] Today’s Video of the Day from the...

<div class="wp-block-sendtonews-playerselector">[sendtonews key="G9bUoxcjr4-2511624-12187" type="single"]</div>



Today's Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> (ACS) reveals that proteins on flu viruses are actually flexible, tilting and waving in a “breath-like” motion. According to the experts, these proteins could be used to better defend against the flu.



"The main antigenic targets of influenza virus are two surface glycoproteins, hemagglutinin (HA) and neuraminidase (NA). Whereas the structural and dynamical properties of both glycoproteins have been studied previously, the understanding of their plasticity in the whole-virion context is fragmented," wrote the researchers.



To investigate, the team conducted detailed simulations of the influenza A H1N1 virion, or the swine flu. The experts concluded that the visualizations show many new vulnerable states of flu viruses, which could improve future vaccines and antiviral drugs.



Video/ Image Credit: American Chemical Society&nbsp;



---



By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Flu viruses are more flexible than expected

[sendtonews key="G9bUoxcjr4-2511624-12187" type="single"] Today's Video of the Day from the...

Graceful spiral galaxy hides a dark secret

News coming your way