Potential signs of life on distant planets

   Faraway world could be home to life, signs sound exciting   

Astronomers can’t visit neighboring planets, let alone distant star-forming regions. So, how do they see what is out there? Astronomers observe the cosmos with telescopes that collect all different wavelengths of electromagnetic energy. For astrochemistry, they typically use radio telescopes. These satellite-dishlike instruments are used to “see” radio waves, which have wavelengths much longer than the human eye can perceive. likewise, JWST is so powerful that it can analyse the chemical composition of the planet's atmosphere from the light that passes through from the small red Sun it orbits. K2-18b is two-and-a-half times the size of Earth and is 700 trillion miles, or 124 light years, away from us - a distance far beyond what any human could travel in a lifetime. It was found that the atmosphere seems to contain the chemical signature of at least one of two molecules which are associated with life: dimethyl sulphide (DMS) and dimethyl disulphide (DMDS). On Earth, these gases are produced by marine phytoplankton and bacteria.

     

 

Astronomers can use telescopes to find specific molecules in the atmospheres of neighboring planets, in nebulae, clouds of interstellar dust and gas, hundreds or thousands of light-years away, or in galaxies beyond the far reaches of the Milky Way. So far, astronomers have found more than 350 molecules in the spaces between and around stars in just under a hundred years, the first such molecule was reported in 1937. Each year, the cosmic chemical stockroom grows by anywhere from a handful to a couple of dozen new finds. Many of these molecules are precursors to biomolecules, meaning they might provide hints about life’s origins elsewhere in the cosmos. Scientists have found new but tentative evidence that a faraway world orbiting another star may be home to life. A team studying the atmosphere of a planet called K2-18b has detected signs of molecules which on Earth are only produced by simple organisms. This is promising that chemicals associated with life have been detected in the planet's atmosphere by Nasa's James Webb Space Telescope (JWST). But independent astronomers stress that more data is needed to confirm these results.

With this ongoing boom in astrochemical census data, there is a lot to be excited about. Sometimes, however, this excitement can be premature. Finding molecules in places people will likely never visit is no simple task, so vetting and sometimes correcting these observations is a continual process, especially for molecules whose signals aren’t as strong. The Taurus molecular cloud is a relatively close star-forming region at 450 light-years away. It has been the site of many astromolecule discoveries. The Robert C. Byrd Green Bank Telescope in West Virginia is a radio telescope which has been used in the discovery of many astromolecules. When molecules freely tumble around as gases in space, they rotate, and this motion releases energy in the form of photons, or electromagnetic particles. Different types of rotations require different levels of energy. Each photon carries that energy with it to a telescope, which records its signal. The more photons of a given energy, the stronger the signal. If a radio telescope records all of the expected signals for a given molecule, its spectrum, then astronomers can confidently say that they have detected that molecule. Infrared telescopes, such as the James Webb Space Telescope, or telescopes that detect visible light, such as the Hubble Space Telescope, can also be used for astrochemistry. Both kinds of telescopes, however, collect chemical signals, which are often more difficult to distinguish from one another.

 This is the strongest evidence yet there is possibly life out there and can realistically say that we can confirm this signal in the coming years. Researchers were surprised by how much gas was apparently detected during a single observation window. The amount we estimate of this gas in the atmosphere is thousands of times higher than what we have on Earth. So, if the association with life is real, then this planet will be teeming with life. If we confirm that there is life on K2-18b, it should basically confirm that life is very common in the galaxy. This is a very important moment in science, but also very important to us as a species. If there is one example, and the universe being infinite, there is a chance for life on many more planets. Behind every discovery of a new molecule in space is months or even years of work to capture a chemical’s “fingerprints,” or its spectrum. Computer models of astrophysically interesting chemicals are used to predict what their spectra would look like. In the lab, the chemicals are injected into a glass tube held under vacuum to mimic conditions in space. Using sensitive instruments, we can record what a radio telescope would see if it were looking at only that molecule. Astronomers had already found some of these molecules in space, but team was also looking at molecules that we predicted might exist somewhere in space.

Team of scientists worked to adjust the computer inputs over and over until the simulated spectra matched the experimental data. When simulated spectra matched the experiments, that meant that the simulated spectra reliably modeled what a molecule’s fingerprint looks like in space. Reliable model spectra allow astronomers to detect chemical features at frequencies beyond what they can measure in the laboratory. The laboratory measurements are done precisely so that astronomers can be confident in their detections. Even with powerful radio telescopes and thorough experiments, some detections aren’t quite as clear as astronomers would like them to be. Sometimes, the signals are too faint for astronomers to be totally confident that they represent the molecules they think they do. Other times, there are too many molecule signals crowded together, causing different signals to blend. Scientists have detected molecules relevant to biological processes back on Earth in comets and the atmospheres of other planets. These detections are exciting, but most scientists exercise caution to avoid jumping to conclusions because those molecules generally can exist outside of living things.

Sometimes, however, the excitement overshadows the caution and leads to premature conclusions. Scientists often get excited when new molecules, especially biologically relevant molecules, are potentially present, and they want to share those findings with the world. Some researchers are also concerned about being the first to publish a new result, especially because a lot of telescope data is publicly available after a brief proprietary period. Perhaps one of the most exciting nondiscoveries in astrochemistry was that of glycine in interstellar space more than 20 years ago. Glycine is the simplest amino acid, a type of molecule essential for life as we know it. Finding this molecule in a nebula would change how scientists think about the evolution of life’s ingredients. Later studies showed that key signals were missing in the initial report of glycine. As a result, astrochemists now generally agree that glycine had not been found in star-forming nebulae. More recently, another molecular discovery has been scrutinized: the potential detection of phosphine in Venus’ atmosphere. Unlike with glycine, scientists have not yet agreed on whether phosphine, which is associated with some biological processes on Earth, is indeed present on Venus.

Initial reports of phosphine on Venus spurred chatter about biosignatures and evidence of potential life on Earth’s much hotter sister planet. However, later studies by other scientists couldn’t confirm the initial results. Over the past five years, scientists have continued to try to confirm or definitively refute Venusian phosphine. When reading about discoveries of new molecules in interstellar space or on other planets, how can you be confident in the detections you are reading about? It’s important to watch out for flashy headlines that claim signs of life have been found elsewhere in the universe. Molecule discoveries that rely on only one or two signals being detected are generally less reliable than those based on five or more signals. For discoveries which tease hints of life on other worlds, other scientists are almost certainly going to try to reproduce the results. If you wait a few months for the initial fanfare to die down, you can do a web search to see what new results have come out to support, or refute, the original claim about the discovery. 

The research suggests K2-18b could have an ocean which could be potentially full of life - though he cautioned scientists "don't know for sure". The team's work will continue to focus on looking for life on other planets: "Keep watching this space." There are lots of "ifs" and "buts" at this stage. Firstly, this latest detection is not at the standard required to claim a discovery. For that, the researchers need to be about 99.99999% sure that their results are correct and not a fluke reading. In scientific jargon, that is a five sigma result. These latest results are only three sigma, or 99.7%. Which sounds like a lot, but it is not enough to convince the scientific community. However, it is much more than the one sigma result of 68% the team obtained earlier, which was greeted with much scepticism at the time. Even with that certainty, there is still the question of what is the origin of this gas. On Earth it is produced by microorganisms in the ocean, but even with perfect data we can't say for sure that this is of a biological origin on an alien world because loads of strange things happen in the Universe and we don't know what other geological activity could be happening on this planet that might produce the molecules. Suggesting life may exist on another planet was "a big claim if true". So we want to be really, really thorough, and make more observations, and get the evidence to the level that there is less than a one-in-a-million chance of it being a fluke. 

Everything we know about planets orbiting other stars comes from the tiny amounts of light that glance off their atmospheres. So it is an incredibly tenuous signal that we are having to read, not only for signs of life, but everything else. With K2-18b part of the scientific debate is still about the structure of the planet. These alternative interpretations have also been challenged by other groups on the grounds that they are inconsistent with the data from JWST, compounding the strong scientific debate surrounding K2-18b. Decades from now, we may look back at this point in time and recognise it was when the living universe came within reach. This could be the tipping point, where suddenly the fundamental question of whether we're alone in the universe is one we're capable of answering.

Muhammad (Peace be upon him) Name

 

ALLAH Names

 

Importance of Human Eyebrows

 Reasons for having Eyebrows

Most people think far more about how their eyebrows look than what they do. Despite all of our plucking, waxing, shaping, or re-drawing them into place, our eyebrows are specifically designed for function rather than form. Your eyebrows serve an essential function when it comes to eye and vision health: they are one of your eyes’ first means of protection. From rigid brow ridges to expressive arches, your eyebrows tell a story of how human faces evolved to signal emotion, identity and social intent. We tend to forget that our eyebrows are even there. They sit above the eyes, doing their work without much fanfare, until, of course, they’re gone. Shave them off, and your face becomes strangely unfamiliar, if not totally unplaceable. This disturbance tells us that our eyebrows are doing far more work for us than we consciously note. For a long time, the standard explanation for their existence was straightforward. Eyebrows help keep sweat and debris out of the eyes. But in evolutionary biology, explanations that feel obvious often turn out to be incomplete. And when researchers began to look more closely at eyebrows, a richer picture emerged.

One way to think of your eyebrows is that they are nature’s sweatband. Have you ever had sweat drip into your eyes? The acid in sweat burns the eyes and causes irritation. If you’re sweating enough, without a means to wipe it away, steady drops of sweat cause you to blink rapidly and may also cause blurred or obstructed vision. Since sweat runs from your scalp and down your forehead, like mini rivers or streams, it also carries dirt, bacteria and other particulates along with it. The curved eyebrow arch is no coincidence, either. The curve wicks the moisture off the skin and around the arch, helping it drain along the sides of your face. Without eyebrows, all of this would run right into your eyes. Fortunately, your eyebrows serve as a “sweatband,” helping to block the flow of sweat and lift it off of your face where it can evaporate before it gets to your eyes. In addition, this action of wicking and lifting up of sweat also serves as a cooling function! Combine fossil evidence, facial anatomy and experimental psychology, and it becomes clear that our eyebrows do so much more than simply protect our eyes. To understand eyebrows, we need to start with a broader shift in human evolution, during which the face itself underwent a full transformation. Early hominins (think Homo heidelbergensis or Neanderthals) had faces that looked very different from ours. Their most striking feature was a pronounced, continuous brow ridge: a thick bar of bone sitting above the eyes. This structure likely already provided substantial protection, helping shield the eyes from debris and mechanical stress. In that sense, the basic “protective” role often attributed to eyebrows was, to a large extent, already accounted for by the brow bone.

The most compelling answer for the purpose of the eyebrows comes from a 2018 study, which reframes the human face as a tool for social communication. The reduction of the brow ridge reflects a transition in how early humans interacted. Earlier hominins’ prominent brow ridges may have served as a signal of dominance or aggression, albeit a relatively static cue. But modern humans, by contrast, rely heavily on dynamic signals and eyebrows are central to that system. Consider how much information a slight eyebrow movement can convey:

A furrow signals concern or confusion

A long raise signals shock

An asymmetrical lift signals skepticism

A quick raise signals recognition or greeting

These are fast and low-effort signals, and they travel well across distance and lighting conditions. Importantly, they’re also difficult to fake convincingly, which makes them useful in maintaining trust within social groups. Modern humans took a different path. In an early study, researchers document a coordinated set of changes in Homo sapiens, namely:

The retraction of the midface (the area around the nose and cheeks)

The reduction of the brow ridge

Beyond largely altering our appearance, these changes also fundamentally reshaped the functional landscape of the face. With the heavy brow ridge reduced, the soft tissue above the eyes gained a wider range of visible motion. Eyebrows could lift, knit and arch in ways that were previously constrained.

In addition to protecting your eyes from sweat, the eyebrows also serve as a filter. They catch particulate matter from dropping into your eyes or further down onto your face. Many of these particulates are very small and almost invisible to the naked eye, making it hard to believe that eyebrows are as necessary as they are. However, without your eyebrows filtering these particles away from your eyes, you’d be far more susceptible to eye allergies and infections. To be clear, eyebrows still offer moderate protection. Their shape and hair direction help channel sweat away from the eyes and catch small particles. But compared to the robust shielding once provided by a protruding brow ridge, this role appears secondary. It’s more of a retained benefit than the primary evolutionary driver. Notably, eyebrows are part of a much broader pattern of changes; they weren’t the product of an isolated tweak. Study emphasizes that increased eyebrow mobility accompanied broader facial reconfiguration. As the mid face retracted, the upper face became more open, visible, and dynamic. These changes include:

The emergence of the chin, a uniquely human feature, which may contribute to facial structure and possibly social signaling, though its function remains debated. 

The whitening of the sclera (the whites of the eyes), which makes gaze direction unusually easy to track compared to other primates.

And the eyebrows, now freed from the constraints of a heavy brow ridge, which became highly mobile and visually prominent.

These features form a coordinated system: a face that can be interpreted. But that kind of coordinated change usually signals a shift in function. Hence, the question then becomes: What new role requires a more expressive upper face? Today, most of us wear sunglasses to protect our eyes from harmful UV rays. However, sunglasses have only been around for about four hundred years. Prior to that, humans relied on hats, the shade, their hands and their eyebrows to help shield the eyes from direct sunlight.

Earlier study situates this within a broader evolutionary trend toward increased cooperation and social tolerance. That is, as human groups grew larger and more interdependent, the ability to communicate subtle emotional states became more valuable. Faces that could signal emotions, rather than just dominance, would have had an advantage. Our eyebrows are part of a redesigned interface, in which we switched from having imposing faces to readable faces. The eyebrows are an essential part of human biology. Yes, they still perform a basic protective role. Their shape and position help divert sweat and debris away from the eyes. That function likely has deep evolutionary roots. As the human face became more open and readable, the ability to quickly and accurately recognize others’ faces took on new importance. Facial recognition became essential to social infrastructure. In a 2003 study, researchers wanted to uncover the role that eyebrows play and produced a result that still surprises people. Researchers took photographs of familiar faces and digitally altered them by removing either the eyes or the eyebrows in Adobe Photoshop. Participants were then asked to identify the faces. Intuition would lead you to believe that removing the eyes would be more disruptive. After all, eyes are often described as the most informative part of the face. But the results showed the opposite: removing the eyebrows caused a larger drop in recognition performance than removing the eyes.

The explanation lies in the kind of information different features provide. Eyes are rich in detail, in that they move, blink and shift direction. However, that same variability can also make them less reliable as stable identity markers. Eyebrows, on the other hand, offer more consistent, high-contrast shape information. Their thickness, curvature, spacing and symmetry become almost like a structural signature. You may have heard that the majority of communication occurs non-verbally through body language. This is why when you can ask your child, “How are you,” their “Fine,” may actually communicate the opposite based on tone, facial expression, and body posture. Eyebrows are a key player in facial expression. You can look at cartoon graphics of eyes and eyebrows, without any other features, and accurately determine emotions like anger, confusion, sleepiness, happiness or fear. The eyebrows’ angle, arch, and movement are important non-verbal communicators. Our human brains are naturally wired to read, assess and translate what eyes and eyebrows express without us having to think about it. And, while neural-divergent children and adults may not inherently understand, working with images of eye/eyebrow expressions helps them learn to read the feelings of those closest to them. Not only are eyebrows essential to human communication, but they also help us to recognize one another. A social study used manipulated photos by eliminating the eyes or the eyebrows, evaluating which features were the most recognizable. It turned out study participants could recognize an average of 60% of the individuals when the eyebrows were there (without eyes), but only 40% were recognizable when the eyebrows were gone, and only the eyes remained. That was not what they’d predicted, and it demonstrates how much eyebrows affect facial recognition between humans. 

Eyebrows allow us to:

Signal emotion quickly and precisely

Navigate social interactions with nuance

Recognize one another with surprising accuracy

There are even suggestions that eyebrows contribute to perceived attractiveness, supported by work on facial aesthetics and sexual dimorphism. Subtle differences in shape and thickness can significantly influence how faces are judged. This is further supported by the amount of effort some of us invest in them, often without fully articulating why. Across cultures, people shape, pluck, thread and enhance their eyebrows. Cosmetic procedures aim to refine their position and movement. These practices reflect an intuitive understanding that our eyebrows matter. In fact, they matter enough that when they disappear, the face feels wrong. Evolutionarily speaking, that’s a big clue, as features that carry little importance tend to fade into variability or disappear altogether. Yet eyebrows have done the opposite: they have become more defined, more mobile and more functionally integrated into how we communicate and perceive. They also play a key role in defining the geometry of the upper face. The distance between the eyes and the brows, the angle of the arch, the balance between left and right, all of these contribute to what researchers call configural processing: the brain’s ability to recognize faces based on spatial relationships between features. When you remove the eyebrows, that geometry completely collapses. The face becomes harder to “parse,” even though the eyes themselves remain. The findings suggest that your eyebrows are what anchor your face.

Like every feature of the human body (including the eyes and vision health), eyebrows come in a wide range of shapes, colors, and textures. There are a few things they have in common. For example, most eyebrows follow the natural shape of your brow bone, and eyebrow hairs are usually coarser than those on your arms or legs. And, while most are the same general hue as the hair on a person’s head, they may grow lighter with sun exposure or as a person ages, and the brows turn grey. However, genetics are the most responsible for whether you have two distinct eyebrows or a single connected brow (referred to as a “unibrow”), as well as your eyebrows’ thickness/thinness, color, fine/coarseness, or the individual hairs’ lengths. However, other factors affect your eyebrows and their function such as:

Consistent plucking/waxing of the eyebrows can permanently destroy hair follicles, which changes your brows’ shape and thickness).

Some people’s eyebrows get much thinner or seem to almost disappear as they age, while others (particularly men) grow thicker, bushier and longer.

Some autoimmune diseases, like alopecia, madarosis, or other health conditions, can reduce or eliminate eyebrows due to hair thinning or loss.

How you can (or can’t) move your eyebrows is also genetic. Some people can raise one eyebrow at a time, while others can’t do it no matter how hard they practice.

Any injury to the tissue on or around the brow line can cause permanent changes. This is common for people with scarring on or around their eyebrows or those with (or had) eyebrow piercings, depending on how the injuries affect the brows’ hair follicles.

Muhammad (Peace be upon him) Name