[20-Feb-2022 02:14:48 UTC] PHP Fatal error: Uncaught Error: Call to undefined function add_action() in /home/australi/public_html/wp-content/plugins/js_composer/include/autoload/vendors/cf7.php:8 Stack trace: #0 {main} thrown in /home/australi/public_html/wp-content/plugins/js_composer/include/autoload/vendors/cf7.php on line 8 [21-Feb-2022 01:47:50 UTC] PHP Fatal error: Uncaught Error: Call to undefined function add_action() in /home/australi/public_html/wp-content/plugins/js_composer/include/autoload/vendors/woocommerce.php:19 Stack trace: #0 {main} thrown in /home/australi/public_html/wp-content/plugins/js_composer/include/autoload/vendors/woocommerce.php on line 19 [20-Feb-2022 05:33:37 UTC] PHP Fatal error: Uncaught Error: Call to undefined function add_action() in /home/australi/public_html/wp-content/plugins/js_composer/include/autoload/vc-pages/settings-tabs.php:27 Stack trace: #0 {main} thrown in /home/australi/public_html/wp-content/plugins/js_composer/include/autoload/vc-pages/settings-tabs.php on line 27 Lauren – Australian Science http://australianscience.com.au Independent Initiative for Advancement of Science and Research in Australia Tue, 31 Aug 2021 10:17:42 +0000 en-US hourly 1 Entelognathus: The Fish with the First Modern Face http://australianscience.com.au/biology/entelognathus-the-fish-with-the-first-modern-face/ Wed, 16 Oct 2013 00:06:10 +0000 http://www.australianscience.com.au/?p=12299 Hundreds of millions of years ago, armoured fish dominated the oceans, lakes and rivers of


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Entelognathus primordialis via Flinders Indaily

Hundreds of millions of years ago, armoured fish dominated the oceans, lakes and rivers of the world. These now-extinct creatures belonged to a class called Placoderms, meaning ‘plate-skinned’ in Greek. They had armoured plates covering their head and thorax, and they were the first creatures to develop teeth, pelvic fins, and most importantly, jaws. Jaws enabled them to become predators, which is thought to be a significant step towards the development of complex creatures like humans.

But for years, there’s been debate over whether placoderms are the ancestors of modern jawed vertebrates, because placoderms have a simple jaw made of one single bone while modern vertebrates have jaws made out of a more complex set of bones. There seemed to be something missing in the transition—evolutionary scientists have long puzzled over what happened in between the placoderms dying out and modern jawed vertebrates springing up. Now, though, a new discovery has shown that placoderms are, in fact, the ancestors we’ve been looking for.

In the suburbs of Yunnan in south-west China, a team of scientists recently found an exquisitely preserved fossil of a 419-million-year-old armoured fish. They dubbed it Entelognathus, meaning ‘complete jaw’. Entelognathus primordialis was part of the placoderm family. Around 20 centimetres long, it had bony plates around its head and front, just like a placoderm, but its jaw and facial structure were nothing like the placoderms. Entelognathus boasted a jaw composed of a complex arrangement of smaller bones. It had the same distinctive three-bone system that is still found in chewing vertebrates today: the lower jaw bone (the dentary bone), the two upper jaw bones (for holding the front teeth), and the maxilla (for holding the canines and the teeth further back in the cheek).

Image via nature.com
Image via nature.com

Entelognathus provides evidence that placoderms were actually the ancestors of all 30,000 species of living fish fauna today. The discovery adds to the list of “missing links

Cite this article:
Fuge L (2013-10-16 00:06:10). Entelognathus: The Fish with the First Modern Face. Australian Science. Retrieved: May 03, 2024, from http://australianscience.com.au/biology/entelognathus-the-fish-with-the-first-modern-face/

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From fables to Facebook: Why do we tell stories? http://australianscience.com.au/psychology/from-fables-to-facebook-why-do-we-tell-stories/ http://australianscience.com.au/psychology/from-fables-to-facebook-why-do-we-tell-stories/#comments Tue, 18 Jun 2013 00:33:20 +0000 http://www.australianscience.com.au/?p=10450 Throughout human history, stories have existed across all cultures in all forms, from ballads, poems,


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Cave Painting
Cave painting, Lascaux, France, 15,000-10,000 BC

Throughout human history, stories have existed across all cultures in all forms, from ballads, poems, songs to oral history, plays, novels. Some narratives have evolved along with the human species—we are consistently drawn back to ancient parables, fables and fairytales, constantly reworking them into modern contexts.

Narrative is a gift unique to the human species, but how as it survived for so long? Is it a by-product of evolution or essential to survival? What drove us to painstakingly inscribe portraits on rocky walls in ochre and charcoal, to compose and listen to lengthy ballads of heroes’ tales, to nosily read people’s Facebook statuses about their day, to devour novels and films like we’re hungry for fictional worlds? Neuroscience and developmental psychology have begun to answer these questions, embarking on the ambitious task of explaining why we tell stories.

Storytelling is one of our most fundamental communication methods, for an obvious reason: narrative helps us cognise information. Telling intelligible, coherent stories to both ourselves and others helps our brains to organise data about our lives and our world. But when we ask why stories are so effective at helping us cognise information, the answers are surprising: it seems that somewhere in the otherwise ruthless process of natural selection, evolution has wired our brains to prefer storytelling over other forms of communication.

Good stories engage us. When we hear plain, bloodless facts, the language processing centres of our brain light up and we decode words into meaning—but when we’re told a story, not only are language processing centres lit up, but also a vast array of other regions distinct from those centres. For example, if you tell a friend a story about a dinner party at which you ate delicious roast pork, their sensory cortex will light up; or if you tell them about the game of football, their motor cortex will become active. The parts of the brain they would use if actually experiencing the event light up, even though they are only being told about it.

This is particularly interesting when considering the effect that literary techniques have on our brain activity. In a 2006 study published in NeuroImages, Spanish researchers asked participants to read both neutral words (such as chair and key) as well as words with strong odour associations (such as coffee, perfume, lavender and soap). Brain scans using an fMRI machine showed that when they read the odour-associated words, their primary olfactory cortex lit up; but when they read the neutral words, that region remained dark. In another study at Emory University, texture metaphors such as “the singer had a velvet voice

Cite this article:
Fuge L (2013-06-18 00:33:20). From fables to Facebook: Why do we tell stories?. Australian Science. Retrieved: May 03, 2024, from http://australianscience.com.au/psychology/from-fables-to-facebook-why-do-we-tell-stories/

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Searching for Life on Titan http://australianscience.com.au/space/searching-for-life-on-titan/ http://australianscience.com.au/space/searching-for-life-on-titan/#comments Wed, 13 Feb 2013 07:53:51 +0000 http://www.australianscience.com.au/?p=6997 Discovered in 1655 by Dutch astronomer Christiaan Huygens, Titan is one of Saturn’s 62 moons,


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Titan against Saturn. Credit: NASA
Titan against Saturn. Credit: NASA

Discovered in 1655 by Dutch astronomer Christiaan Huygens, Titan is one of Saturn’s 62 moons, named for a race of giants in Greek myth who were Saturn’s brothers and sisters. Over 5000 km in diameter, it’s roughly twice the size of our own Moon and is one of the largest moons in our solar system, second only to Jupiter’s Ganymede. It’s even bigger than the planet Mercury, and is covered with an orange haze that shields the secrets of its surface. That alone makes it interesting, but a glimpse into the workings of the planet makes it more intriguing still—astronomers even believe Titan could harbour life.

In the 1980s, the Voyager 1 and 2 spacecraft flew past Titan; in the 2005 Huygens probe parachuted through its atmosphere and landed on the surface; and the Cassini spacecraft still studies Titan from its orbit around Saturn. Their images and measurements have revealed a vibrant alien world beneath the haze—complete with rivers, lakes, and ice volcanoes.

Credit: NASA
Credit: NASA

Titan is an incredibly frigid place, with an average temperature of -178 degrees Celsius (-289 Fahrenheit)—too brutally cold for life as we know it, but still of incredible interest to astrobiologists. It’s the only moon known to have an atmosphere—a thick and cloudy one, composed primarily of nitrogen—and it also exhibits weather and changing seasons. The orange haze that shrouds its surface is made up of trace gases such as benzene and hydrogen cyanide, and at the pole closest to the sun, sunlight heats the toxic orange haze and makes it circulate towards the other pole, so the gases concentrating there. Since a year on Titan lasts almost 30 Earth years, each season is 7 years long.

Titan's seasonal changes. Credit: NASA
Titan’s seasonal changes. Credit: NASA

However, unlike Earth, its weather system is methane-based—and aside from Earth, Titan is the only object in the solar system to have permanent bodies of liquid on its surface, including an enormous river system that flows 400km across the moon’s surface to meet a large sea.

River network on Titan. Credit: Cassini
River network on Titan. Credit: Cassini

The darkness of the river in the image indicates a smooth surface, which in turn indicates that the river is not a dry bed, but filled with liquid—but this liquid is likely methane or ethane, which are more closely related to gasoline than water. Even though the mechanics seem to be similar, Titan’s weather would be alien to us because the skies fall with methane rain and lakes and oceans pool with liquid methane—but still, this presents possibilities of methane-based life.

Credit: Cassini.
Credit: Cassini.

It is also suspected that Titan harbours cyrovolcanoes, which spew water ice and hydrocarbons into the atmosphere instead of lava. Speculations began after NASA’s Cassini spacecraft captured images of a landform on Titan’s surface called Sotra Facula. The images showed three conical features with material flowing from them, their peaks up to 1,500 metres tall, as well as several pits equally as deep. Researchers gravitated towards the idea that these landforms were cyrovolcanoes, as it would help explain a long-standing mystery of Titan’s thick, methane- and nitrogen-filled atmosphere. Calculations show sunlight would have broken the methane down long ago if something hadn’t been replenishing it, and a cyrovolcano is a good candidate—it could erupt methane, dragging it from the planet’s interior into the atmosphere.

Sotra Facula. Credit: APOD.
Sotra Facula. Credit: APOD.

However, these intriguing surface features could have also been created by weather and meteorite strikes than by volcanic activity, and it is difficult to tell without further data. Researchers believe cyrovolcanoes might be fairly common on the frigid moons of the outer planets—one has been confirmed on another of Saturn’s moons, Enceladus—which is incredibly interesting, because volcanic activity would prove that Titan is an active world, and could increase the likelihood that this huge, distant moon may harbour life. While searing lava destroys life on Earth, ice volcanoes on Titan would provide a way to mix complex chemicals from the surface and the interior. It could bring life forms up to the surface so our instruments have a better chance of detecting them—because fascinatingly, Titan seems to have subsurface oceans.

Further data from Cassini indicates that Titan has a layer of liquid water under its icy outer shell. The evidence is tidal—as Titan orbits Saturn, the planet’s powerful gravitational pull stretches and deforms the moon, like pulling and stretching an elastic band. If Titan were solely composed of rock, this stretching would only cause bulges (tides) of about 1 metre, but instead the moon experiences tides of about 10 metres—suggesting that its interior is not entirely solid. This ocean may not be enormous or deep; just a liquid layer between the solid mantle and the external icy shell would be enough to compress and bulge as Cassini has observed. Since Titan’s ice surface is composed mostly water ice, researchers believe its ocean could be liquid water.

However, just the presence of an ocean alone does not indicate life—researchers think that life is more likely to occur when the water comes into contact with rock, and we can’t currently tell if this exists beneath the surface.

Possible scenario for internal structure of Titan. Credit: NASA
Possible scenario for internal structure of Titan. Credit: NASA

Another intriguing phenomenon is the hydrogen gas flows through its atmosphere, and yet there is a lack of the chemical on the planet’s surface—so how did it disappear? One theory suggests that hydrogen-breathing, methane-based life forms consume the gas, similar to how we consume oxygen on Earth.

Liquid water, a possibly active interior, complex chemistry, a thick atmosphere, seasons, weather… All of these factors reflect the environment of life as we know it, so researchers have long thought that Titan is an excellent candidate to harbour life. None of these factors alone are solid evidence for life—they are just conditions necessary for it—but Titan is a fascinating place deserving of further study. Since its nitrogen-rich atmosphere is similar to Earth, just significantly colder, it also demonstrates how atmospheres of cold moons and planets behave, and thus allows us to speculate about how the atmospheres of exoplanets far from their stars might behave.

But our questions about Titan will remain unanswered until we obtain sufficient evidence to draw conclusions—but to do this, we need data. Two possible missions have recently been proposed. The first is the Titan Mare Explorer (TiME), which would have sent a floating buoy to land in Titan’s methane sea and measure the chemistry and organic composition, study the sea’s interaction with the atmosphere, and basically perform the first nautical exploration of this extraterrestrial ocean. It also would have observed Titan’s methane cycle to help us compare it to the water cycle on Earth. TiME was proposed to launch in 2016, but unfortunately it lost its funding to a Mars mission.

Artist's concept for the TiME lander. Credit: NASA/ESA
Artist’s concept for the TiME lander. Credit: NASA/ESA

Another possibility, however, is the Titan Saturn System Mission (TSSM), which is a proposed exploration of Saturn, Titan, and Enceladus—focusing on the complex phenomena the Cassini spacecraft has already noted. It is proposed to launch in 2020 and reach Titan by 2029, and during its 4-year-tenure, it would spend time circumnavigating Titan and studying its astrobiological potential. The mission consists of an orbiter and two Titan exploration probles—one that’s basically a hot air balloon, and another that land on the methane seas. One of the proposals for this second lander is the lake-lander of the discarded TiME mission, which will hopefully be included. TSSM, if it goes ahead, would be the first mission to extensively survey the organic chemistry and climate of the land, sea, and air of another world.

If life is detected on Titan, it would undoubtedly be moving and crucial to us as a species—not only because it’s the first extraterrestrial life we have detected, but also because it would behave differently to the water-based, oxygen-breathing life we’ve developed here. Even if life has not yet developed on Titan, the chemistry for life to form is present, so just give the moon four billion years…and who knows?

Cite this article:
Fuge L (2013-02-13 07:53:51). Searching for Life on Titan. Australian Science. Retrieved: May 03, 2024, from http://australianscience.com.au/space/searching-for-life-on-titan/

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Tasting colours and seeing sound: Synaesthesia http://australianscience.com.au/history/tasting-colours-and-seeing-sound-synaesthesia/ http://australianscience.com.au/history/tasting-colours-and-seeing-sound-synaesthesia/#comments Wed, 07 Nov 2012 00:30:18 +0000 http://www.australianscience.com.au/?p=5210 “One hears a sound but recollects a hue, invisible the hands that touch your heartstrings,


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Kandinsky: “Composition 8”

One hears a sound but recollects a hue, invisible the hands that touch your heartstrings,

Cite this article:
Fuge L (2012-11-07 00:30:18). Tasting colours and seeing sound: Synaesthesia. Australian Science. Retrieved: May 03, 2024, from http://australianscience.com.au/history/tasting-colours-and-seeing-sound-synaesthesia/

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