Over the years bikers have been known for their very bold and chunky jewelry which often represents speed and power. They are fond of a macabre image that represents death or mortality. The riders are very weird; the jewelry makes them look scarier granted that they have scary symbols like the skull. The jewelry worn by bikers is nothing new, as a matter of fact, many people find such dark symbols fascinating.

The skull is an attractive design incorporated to biker-related culture. It has gained its popularity once more promulgated by the styles and designs in the jewelry market today. The skull imagery has been adapted in fashion by many designers and has remained relevant over the years. Many biker clubs incorporate skulls as their logos to express their love and admiration for skulls.

The dangerous symbols used to make biker jewelry appeal to many people due to its mystery. Human beings are known to fear things that they do not understand, a skull being a symbol of death can be feared. From ancient times there are many cultures that attract people to using these pieces of jewelry. With the changing time, there has been an improvement in the manufacturing of this jewelry.

Skull rings and biker rings have also gained popularity. They have a rich symbolism, fascinating aesthetic and its association to a dangerous subculture. Many people who are not afraid of taking style to another level are not scared of trying these rings given that they are stylish and unique. The materials used like 316L stainless steel ensures these rings have a higher quality and greater details compared to the ones made from previous years.

Many view riding a motorcycle a rather dangerous activity and crime related due to many outlaw biker gangs associated with it. It is fit to see the skull in the biker subculture, used by many biker clubs as patches and identifications for years. Skulls seen in this subculture context incorporate other symbols like winged skulls and the grim reaper. The symbolism and modifications add on to the original meaning of the skull making them fashionable throughout the years.

There is an advantage in selling edgy jewelry like the skull rings and biker rings; the design is interesting, and customers are awed by its unusual style. Other pieces of jewelry like pendants, bracelets, necklaces and cufflinks can also get matched to the skull. Bracelets can have links with few skulls or one skull. One can have the whole ensemble for fashion goals and good, captivating looks.

Rings are known for their small size that rarely clashes with outfits, unlike necklaces or bracelets. They are seen to be very popular accessories; even men who are not jewelry enthusiasts can still be persuaded to wear a ring particularly if it is a skull or biker ring. They attract male customers and also women who have an interest in dark and edgy jewelry.

Biker jewelry is available in the market, and one can purchase them via online shops. They are very fashionable and keep you looking good.

If evil is the current style it gets manifested in an art form like tattooing. Many people are crazy about this style and sometimes for not depicting anything bad. Some people might want to display their power and might through evil tattoos, while others may just want to give evil tattoo a humorous twist. There is nothing that is good or evil-it is just the symbolic meaning. Some of these symbols may thus include Satan, Prince of darkness, devil horns and skulls.

Tattoos are depictive of human emotions and feelings. So, they may sometimes be indicative of a person's dark side. Many people find it not only fascinating but fashionable. They make a strong visual impact and a few individuals also believe that evil tattoos may ward off evil itself. If you too want to explore the wickedness within yourself and turn it into a form that is attention catching, try out any of the following types.

Designs for dark evil tattoos

Skull: These may be an obvious choice in depicting something evil. It is symbolic of evil if you get a skull and crossbones tattoo. The type of skull tattoos that girls generally prefer is the tribal skull design, which does not require any more design additions as the broad strokes they include are enough to make them look wild. In a simple skull design though, you might add some elements, like fire, in the background. Another popular option is the Mexican skull in which a variety of designs are available.

Grim reaper: This dark and mysterious form of tattoo is the most common type for men. It might also be one of the scariest too. This one would look best done in a classic form, while you may add a shadowy background or a skull and crossbones to make it look scarier.

Vampire: Teenagers are often fascinated by vampire tattoos. You may keep this design simple with its traditionally displayed teeth and get it made on your arm or back, or you may get a biting vampire on your neck.

Occult: These tattoos often get associated with witchcraft. So, think before you go for an occult one. Some famous symbols that people get in this type are an evil eye, the number 13, an athame, a pentacle or a lion eating a fish. A fusion of this tattoo type with the tribal style can be something unique as the tribal tattoo colors can make an occult tattoo stand out from the crowd.

So, there could be different designs to choose from. Whether it is bad or humorous, an evil tattoo still looks quite unique with all its wickedness. Whenever you get an evil tattoo body, always remember to understand its significance and then get it inked. Do not simply go by its design, as there is more to just getting a tattoo inked on your body.

Stars do not live forever–they send their brilliant stellar fires out into space for millions to billions of years, but they are doomed roiling, glaring spheres of gas. When stars run out of their necessary supply of nuclear-fusing fuel, they are ready for their inevitable meeting with the Grim Reaper. Massive stars blast themselves to pieces in violent and brilliant core-collapse (Type II) supernovae, while small stars like our Sun may–or may not–pass away in relative peace. Small stars, like our Sun, can also go supernova–just like the big guys–but the conditions must be right in order for them to give this sort of brilliant farewell performance to the Cosmos. When a small sun-like star perishes in the noisy blast of a brilliant Type Ia supernova, it leaves behind a lingering ghost, which is termed a white dwarf star- the erstwhile small star’s relic core. A new study published in the August 10, 2019 issue of The Astrophysical Journal proposes that these ghostly remains of stars long gone still haunt stars that are living today.

A Type Ia supernova is an explosion that ignites in binary stellar systems in which a duo of sister stars are in orbit around one another–and one of the stars is a white dwarf. The other star can by anything from a giant star to an even smaller white dwarf. The fatal blast in this type of binary system occurs because the stellar ghost has been gravitationally sipping up its sister star’s material, causing it to acquire enough mass to go critical. A second explosive scenario, also taking place in a binary system, occurs when a duo of white dwarf stars crash into one another.

White dwarfs are not all the same. These dense stellar ghosts can range from 50% of the mass of our Sun, to almost 50 times its mass. Solitary small stars like our Sun, die a quiet death. After a lonely small sun-like star has run out of its necessary hydrogen fuel to fuse, it puffs its beautiful multicolored shimmering layers of gas into the space between stars. However, its lingering core (the white dwarf) has remained intact, and it rests in peace at the heart of this lovely shroud of glimmering gas.

By studying the “fossil” relics of long-dead exploded white dwarfs, a team of astronomers, led by Dr. Evan Kirby of the California Institute of Technology (Caltech) in Pasadena, have found that white dwarfs in the early Universe frequently blasted themselves to pieces at lower masses than they do today. This discovery suggests that a white dwarf can explode as the result of a variety of triggers, and it does not necessarily have to reach critical mass before the fatal blast.

Fatal Attractions Among The Stars

All of the stars in the observable Universe, both large and small, live out their entire nuclear-fusing main-sequence “lives” by keeping a very delicate and necessary balance between two ancient foes–gravity and radiation pressure. The main-sequence refers to hydrogen-burning stars on the Hertzsprung-Russell Diagram of Stellar Evolution. Main-sequence stars still have enough nuclear-fusing hydrogen fuel to keep themselves bouncy against the crush of their own gravity.

The outward push of a star’s radiation pressure forces everything away from the star, while simultaneously gravity tries to mercilessly pull everything inward. The radiation pressure of a star is the result of the process of nuclear-fusion which commences with the burning of hydrogen, the lightest and most abundant atomic element in the Cosmos, into helium–which is the second lightest. This process of stellar nucleosynthesis continually fuses increasingly heavier and heavier atomic elements out of lighter ones. Indeed, all of the atomic elements heavier than helium–termed metals in the jargon of astronomers–formed within the searing-hot nuclear-fusing cores of the billions of stars inhabiting our vast Universe. Alternatively, the heaviest metals of all–such as gold and uranium–form in the spectacular supernova explosions heralding the death of a star.

Many supernovae are triggered when a lone, especially massive star runs out of its necessary supply of nuclear-fusing fuel, and rips itself apart in a spectacular core-collapse explosion. The progenitor of a core-collapse (Type II) supernova is usually a massive star that contains an extremely heavy core that weighs-in at about 1.4 times solar mass. Smaller stars normally do not die this way. In fact, smaller stars live much longer than more massive stars. This is because less massive stars are not as hot, and hence burn their fuel more slowly, than their heavier stellar kin. Small stars of our Sun’s mass generally last for about 10 billion years. More massive stars, however, live fast and die young–frequently living for millions (as opposed to billions) of years.

Like all stars, our Sun is doomed to run out of its necessary hydrogen fuel. It is a middle-aged star of about 4.56 billion years of age, and it can continue to fuse hydrogen in its core for another 5 billion years, or so.

When small stars, like our sun, finally have managed to fuse most of their necessary hydrogen fuel into heavier things, they first swell into glaring, bloated red giant stars. This evolved sun-like star at this late stage of development contains a worn-out heart composed of helium, surrounded by a shell in which there is still a small amount of hydrogen left to be burned into helium. This shell begins to travel outward, and the dying heart of the small star grows ever larger, as the star ages. At last, the helium heart begins to shrink. As it does so, its temperature soars at its center to the point that the helium is fused into the even heavier metal carbon. The star ends up with a very small, but extremely hot heart, that produces more energy that it did when it was still a hydrogen-burning star on the main-sequence. The star is now doomed, and its outer layers of gas are now swollen and red. The temperature at the glaring surface of this bloated red giant is cooler than it was when it was still a young star.

When small stars are like our Sun, and live alone, they die gently and beautifully–leaving their relic cores behind as white dwarf stars. However, when the star has company, explosive things can happen in the form of a Type Ia blast. These brilliant explosions hurl the former star’s newly forged elements out into space where they may be incorporated into later generations of stars.

Nevertheless, it is still uncertain why some white dwarfs go supernova while others of their kind do not. In the early decades of the 20th-century, the great Indian-American astrophysicist Subramanyan Chandrasekhar (1910-1995) determined that if a white dwarf possessed more than 1.4 times solar-mass, it would explode in a Type Ia supernova. This particular mass is called the Chandrasekhar mass, and although Chandrasekhar’s calculations explained one means by which some of the more massive white dwarfs explode, it did not explain why other white dwarfs of smaller mass also blow themselves up.

Ancient Stellar Ghosts Haunt Stars Today

Observing Type Ia supernovae must be accomplished quickly. This is because they flare into existence, and then dim to darkness, within only a few months. In order to study supernovae that have long since faded, and the stellar white dwarf ghosts that created them, Dr. Kirby and his colleagues used a technique informally named galactic archaeology.

The term galactic archaeology refers to the search for lingering chemical signatures of ancient explosions in other, more youthful stars. When a white dwarf explodes in a Type Ia supernova, it “pollutes” its galactic surroundings with the elements forged during the blast–metals like nickel and iron. Then those heavy atomic elements wander through space, eventually to be incorporated into any newly forming baby stars located in that region. This is comparable to the way that fossils currently provide scientists with important clues about animals that have long been extinct. The quantities of nickel and iron show how massive their long-gone predecessors must have been.

Using the Keck II telescope in Hawaii, Dr. Kirby and his team first went on the hunt for certain ancient galaxies, that had run out of material to form baby stars during the first billion years of the Universe’s existence. The astronomers discovered that most of the stars within these galaxies had relatively low nickel content. This was a tattle-tale clue that the white dwarf ghosts that provided them with nickel must have been of relatively low mass–likely lower than the Chandrasekhar mass.

However, the team of galactic archaeologists found that the nickel content was higher in more recently formed gas. This means that, as time passed after the Big Bang, white dwarfs started to explode with higher masses.

It is important for scientists to understand the mysterious processes that trigger Type Ia supernovae. This is because the explosions themselves have been successfully used as tools for making cosmological measurements. No matter how they exploded, most Type Ia supernovae display a well-known relationship between luminosity and the time it takes for them to dim.

“We call Type Ia supernovae ‘standardizable candles’,” Dr. Kirby commented in an August 6, 2010 Caltech Press release.

“If you look at a candle at a distance it will look dimmer than when it is up close. If you know how bright it is supposed to be up close, and measure how bright it is at a distance, you can calculate that distance. Type Ia supernovae have been very useful in calculating things like the rate of expansion of the Universe. We use them all the time in cosmology. So, it’s important to understand where they come from, and characterize the white dwarfs that make these explosions,” he added.

The scientists plan to study elements other than nickel next, and are planning to target manganese in particular. Manganese production is extremely sensitive to the mass of the supernova that churns it out, and therefore provides a precise way to validate conclusions derived from the nickel content.

The research paper is published under the title “Evidence for Sub-Chandrasekhar Type Ia Supernovae from Stellar Abundances in Dwarf Galaxies”.

When the decision to revive the sitcom Roseanne was made, one of the problems had to do with the character of Dan Connor. The husband of the title character, played by actor John Goodman, had been declared dead after a heart attack in the finale of the last season two decades ago.

The writers, much like Hollywood versions of Victor Frankenstein, found a creative way to bring Dan back to life. It was probably not a difficult procedure, for the Roseanne panel had a plethora of precedents to examine for ideas.

Here are nine other popular TV sitcom characters who have been mistakenly declared dead, either through bureaucratic errors or chicanery.

Hawkeye Pierce in MASH

“The Late Captain Pierce” is the title of an episode where Alan Alda’s character has to prove he still exists, even though the army has declared him as deceased.

Archie Bunker in All in the Family

America’s most lovable bigot found himself in a struggle with the government, trudging through red tape to prove that his heart was still beating.

Abe Simpson in The Simpsons

In an episode called “The Old Man and the Key” after the famous novel by Ernest Hemingway, Grandpa has been erroneously declared dead by his nursing home.

Peter Griffin in Family Guy

The Grim Reaper comes for Peter believing he has died, but Old Scratch ends up injuring his ankle instead of claiming the head of the Griffin family.

Tom Silby in The Andy Griffith Show

In a side story of the classic episode called “Opie’s Charity”, a Mayberry citizen believed have died two years ago, returns to tell the Sheriff that he had merely left his wife after another spat. Instead of suffering the humility of a runaway husband, his wife had chosen to declare him dead and even carried out an elaborate funeral for him.

George Costanza in Seinfeld

George Steinbrenner and the rest of the front office of the New York Yankees believe that their employee has passed away, since the title character’s best friend (played by Jason Alexander) had left his car unmoved in the parking lot for a week. This classic episode is called “The Caddy.”

Thurston Howell the Third in Gilligan’s Island

After hearing he has lost his entire fortune, the millionaire (played by Jim Backus) is thought to have committed suicide when the castaways find his hat floating on the lagoon.

Fish in Barney Miller

Abe Vigoda’s unforgettable character in the police station runs into a huge problem when he finds his name in the obituary column in the “Discovery.”

Drew Carey in The Drew Carey Show

He was in a coma in an airing called “Drew’s Life After Death”, but when a doctor sends a death certificate Drew’s loved ones assume that he has passed on.

Our Sun is doomed to eventually die after it has “lived” brilliantly and beautifully for about 10 billion years. The good news is that, because our Sun currently is a bit less than 5 billion years of age, it can still go on blissfully burning its supply of life-sustaining nuclear-fusing hydrogen fuel for another 5 billion years before the Grim Reaper comes to call. Solitary stars of our Sun’s mass all perish the same way–first ballooning in size to become enormous, swollen, crimson red giant stars before tossing their outer shimmering rainbow of multicolored gaseous layers into interstellar space–leaving behind only a dense Earth-sized relic core termed a white dwarf star to bear witness to the tragedy. In July 2019, an international team of astronomers announced that they had observed a rare dynamic event for the first time, when they witnessed the death of a distant red giant star. This observation provides a sneak preview of our Sun’s inevitable and sad demise.

Dr. Meredith Joyce, an astronomer based at The Australian National University (ANU) co-led the study with Dr. Laszlo Molnar and Dr. Laszlo Kiss from the Konkoly Observatory of the Hungarian Academy of Sciences. Dr. Joyce noted in a July 26, 2019 ANU Press Release that the star observed, dubbed T Ursae Minoris (T UMi), was similar to our Sun.

“This has been one of the rare opportunities when the signs of ageing could be directly observed in a star over human timescales. We anticipate our Sun and TMi will end their lives much more quietly and slowly compared with a supernova–a powerful and luminous explosion,” Dr. Joyce continued to explain.

The new findings strengthen the prediction that our dying Sun will become a red giant, before evolving into an expanding and glowing ring-shaped shell of gas in five billion years, leaving behind only a small white dwarf stellar corpse.

“It will become much bigger as it approaches death–eating Venus, Mercury and possibly the Earth in the process–before shrinking to become a white dwarf,” Dr. Joyce added.

The Life-Cycle Of Lonely Stars Like Our Sun

Stars are a lot like people. They are born, and then go on to enjoy a playful childhood and active youth–but, eventually, stars calm down when they evolve into glaring adults. However, the inevitable occurs when a star grows old and dies. Stars that are more massive than our Sun end their stellar lives when they explode in brilliant, violent supernova blasts. After the catastrophe, the erstwhile massive star leaves behind a dense, city-sized object termed a neutron star. Neutron stars are so dense that a teaspoon full of neutron star material can weigh as much as a herd of zebra. However, the most massive stars in the Universe have a different fate. When these especially massive stars run out of their necessary supply of life-sustaining nuclear-fusing fuel, they collapse into the oblivion of a black hole of stellar mass.

Less massive stars, like our Sun, come to the end of the stellar road more peacefully, without the brilliant grand finale fireworks display of their more massive stellar counterparts. When stars like our Sun live alone, without a binary companion, they first evolve into red giants that ultimately blow off their outer layers to become white dwarfs encircled by a beautiful shell of multicolored gases.

All stars, regardless of their mass, are kept brilliantly bouncy as a result of an enduring battle between gravity and radiation pressure. Gravity tries to pull all of the star’s material in, while radiation pressure tries to push everything out. This delicate balance between the two eternal foes goes on from stellar-birth to stellar-death. In the end, when the old star runs out of its necessary supply of nuclear-fusing fuel, it can no longer churn out radiation pressure to counteract the relentless and merciless pull of its own gravity As a result, gravity wins the war, and the star is doomed.

Today, our Sun is a lonely star, but it was probably not born that way. Our Star probably formed as a member of a heavily populated open cluster, along with thousands of other newborn, fiery sibling stars. Our Sun was either gravitationally evicted from its natal cluster due to interactions with others of its fiery kind or it simply peacefully floated away into the space between stars approximately 4.5 billion years ago. Likewise, our Sun’s long-lost siblings are thought to have migrated to more remote regions of our Milky Way Galaxy, never to return.

Our entire Solar System emerged from the tattered remains left over from the nuclear-fusing ovens of previous generations of dead ancient stars. Our Sun–like others of its kind–was born within a dense, cold blob tucked tenderly within the whirling, swirling, ruffling folds of a churning dark, giant molecular cloud. The dense blob ultimately collapsed under the intense pull of its own gravity, thus giving birth to a hot, glaring baby star (protostar). Within the secretive depths of these enormous and beautiful clouds, that float like lovely, eerie phantoms throughout our Galaxy in huge numbers, fragile threads of material tangle themselves up together, and the resulting clumps grow ever larger and larger for hundreds of thousands of years. Then, pulled inward by the relentless crush of gravity, the hydrogen atoms existing within the clumps rapidly and dramatically fuse. This process of nuclear fusion triggers a violent conflagration that will rage with brilliant fury for as long as the new star lives–for that is how a star is born.

Currently, our Sun is experiencing an active, nuclear-fusing midlife. It is classified as a main-sequence (hydrogen-burning) small star on the Hertzsprung-Russell Diagram of Stellar Evolution. As stars go, it isn’t special. There are eight major planets and an assortment of smaller bodies in orbit around our Sun, which is located in the distant suburbs of a typical, though magnificent, large spinning, starlit pinwheel in space–our barred-spiral Milky Way Galaxy.

Today, our Sun is still sufficiently youthful and bouncy to go on burning hydrogen in its heart by way of nuclear fusion–which continually creates heavier and heavier atomic elements out of lighter ones (stellar nucleosynthesis). But our Sun’s looks will change when it finally begins to run out of its necessary supply of hydrogen fuel. At this point, our Sun will evolve into an elderly star. In the dying heart of our Sun, there will exist a core of helium that is encased within a shell composed of hydrogen that is still in the process of being fused into helium. Eventually, the shell will begin to travel outward, and the core will grow larger as our Sun grows older. The helium core itself will ultimately shrivel under the intense pull of its own weight–until, finally, it grows seething-hot enough to trigger a new stage of nuclear-fusion. At this point, the atoms existing in our dying Star’s helium core will begin to be fused into the heavier atomic element, carbon. In another five billion years, our Star will possess a small and searing-hot core that will be emitting more energy than it does now. The outer gaseous layers of our doomed Sun will have ballooned to hideous proportions, and it will no longer be the same Star we are familiar with today. Alas, it will have experienced a sea-change into a ghastly red giant that will go on to engulf and incinerate Mercury, then Venus, and then (possibly) Earth. The temperature at the surface of our Star, in its future red giant phase, will be quite a bit cooler than it is now–which will account for its comparatively cool red hue. Nonetheless, our evolved Star will still be hot enough to convert the currently frigid, icy inhabitants of the distant Kuiper Belt–such as the dwarf planet Pluto–into delightful tropical havens of refuge for what may (or may not) be left of humanity. The dying hot heart of our Sun will continue to shrivel, and since it can no longer produce radiation by way of nuclear fusion, all further evolution will be governed only by the force of gravity. Our Star will then finally hurl off its outer layers–but its core will stay in one piece. All of our Sun’s material will finally collapse into this small relic body–the newly-formed white dwarf. The baby white dwarf will be encircled by a lovely expanding shell of multicolored gases termed a planetary nebula. White dwarfs radiate away the energy of their collapse, and our future white dwarf Sun will likely be composed of carbon and oxygen atomic nuclei swimming around in a swirling sea of degenerate electrons. The equation of state for degenerate matter is “soft”. This means that any mass added to the body will cause it to grow smaller in size. Continuing to add mass to a white dwarf causes it to shrink further, even as its central density grows larger. Our Sun’s radius will finally shrink to only a few thousand kilometers. Our Sun, and other stars like it, will grow progressively cooler over time when they evolve into white dwarfs.

Red Giants In General

Red giants are luminous giant stars of low to intermediate mass that weigh-in at the approximate equivalent of 0.3 to 8 times that of our Sun. These swollen stars represent a late phase of stellar evolution, and their outer atmospheres are both inflated and tenuous. This makes their radii large. The surface temperature of a red giant is about 8,500 degrees Fahrenheit–or lower, and their true colors are anywhere from yellow-orange to red. Many of the observed bright stars are red giants. This is because they are rather common denizens of our Galaxy, and they are also very luminous. For example, the red giant Arcturus is 36 light-years away, and Gamma Crucis is 88 light-years from Earth.

In general, red giants sport radii that are tens to hundreds of times greater than that of our Star. Despite the lower energy density of their envelope, red giants are much more luminous than our Sun because of their enormous size. Indeed, red giants have luminosities that can be as much as almost three thousand times that of our Star.

Another important feature that red giants have is that, unlike still-living sun-like stars whose photospheres display numerous small convection cells (solar granules), red giant photospheres have only a few large cells. This feature is responsible for causing the variations in brightness so common in these swollen stars.

Over the main-sequence “life” of a sun-like star, its supply of hydrogen in its core is slowly fused into helium. The doomed star’s main-sequence “life” comes to a tragtic end when almost all of the hydrogen in its core has been fused. Stars that are more massive than our Sun burn disproportionately faster, and thus spend less time on the main-sequence than their smaller stellar kin. The larger the star, the shorter its hydrogen-burning “life”.

Sneak Preview Of Our Sun’s Demise

The dying sun-like star T UMi was born about 1.2 billion years ago, sporting a mass approximately twice that of our Sun. It is situated in the Ursae Minoris (Little Bear) Constellation over 3000 light-years from Earth.

The international team of astronomers found that over the past few million years–as T UMi reached the last phase of “life” before its sea-change into a white dwarf–it has been experiencing a series of pulses, whereby its temperature, brightness, and size have fluctuated dramatically.

“Energy production in T UMi has become unstable. During this phase, nuclear fusion flares up deep inside, causing ‘hiccups’ that we call thermal pulses. These pulses cause drastic, rapid changes in the size and brightness of the star, which are detectable over centuries. The pulses of old stars like T UMi also enrich the entire Universe with elements including carbon, nitrogen, tin and lead,” Dr. Joyce explained in the July 26, 2019 ANU Press Release.

The astronomers have observed the star diminishing in temperature, size, and brightness over the past three deades.

Dr. Joyce continued to note that “We believe the star is entering one of its last remaining pulses, and we’d expect to see it expanding again in our lifetimes. The star will eventually become a white dwarf within a few hundred thousand years. Both amateur and professional astronomers will continue to observe the evolution of the star in the coming decades, which will provide a direct test of our predictions within the next 30 to 50 years.”

This research is published in the July 5, 2019 issue of The Astrophysical Journal.

Thanatophobia – the fear of death or dying is a phobia that is rarely talked about. Most people think they are alone in their suffering and don’t usually share their fears about the Grim Reaper. In reality, Death Anxiety affects most people at some time or another in their lives, but the degree of anxiety would largely depend on the individual. Some of us live in complete denial, preferring to think that we have an endless supply of tomorrows, while others are consumed with daily thoughts about their own mortality. None of us know for sure what will happen to us after we die, but when the fear of dying consumes your thoughts to the point that it interferes with your everyday life you may be suffering with Thanatophobia. The realization of one’s own mortality is a natural concern for most humans but obsessive fear and anxiety can take the joy out of living and even lead to full-blown panic attacks.

So what is it about this universal phenomenon that fills us with such dread? Most people would agree the most obvious answer is the “fear of the unknown.” Since we have never actually experienced death, how can we be sure what will be waiting for us on the other side? What if our concept of the afterlife is completely false and there is absolutely nothing – the ultimate disappointment? The loss of Self and ceasing to exist can be a terrifying prospect. If this is all there is to our existence, then our fear would seem to be justified. For some the “fear of dying alone” causes extreme anxiety. Ultimately you must pass through death alone but the passing may be made easier when surrounded by loved ones and familiar faces. Others fear leaving their loved ones behind to cope without them. They worry about how they will manage emotionally and financially as well as living out their lives without them.

Whatever the reasons, death is unavoidable and comes to us all. Whether you are obsessed with the issue or choose to completely ignore it, a balance must be sought if we are to live our lives fully and completely.

So how do we deal with dying?

Some of us find comfort in religion and a strong belief in the afterlife. Others turn to science and the study of Near Death Experience desperately looking for some proof that we really do possess a soul that lives beyond the finality of death. Everyone, in their own way seeks an answer that will calm and soothe their fears. Studies show that deeply religious people fear death the least while the more skeptical were haunted by their death fears. However, atheists don’t worry at all – for obvious reasons. It has also been noted that the fear of dying also seems to lessen as we age.

It is our instinctive nature to resist and avoid death. Our bodies are geared toward

survival. To help us deal with our mortality maybe we should take a closer look at our fear of dying. Identifying our fears is the first step to facing them. Are we afraid to suffer? Are we afraid of the unknown? It is only by facing our fears that we are able to overcome them.

When you think about 40th birthday party invitations, you have a few things to consider. First of all, what sort of personality does the guest of honor have? Are they outgoing, shy, funny, sarcastic? You have options when it comes to invitations, from purchasing them from a traditional card shop, creating them yourself or purchasing them online. If you purchase invitations online, you have the option of creating your own invitations and customizing them. This can be especially funny if you have any really great photos of that person that are humorous.

The invitation could be based on a hobby that the birthday person is interested in, or a sport they like to play or watch. Maybe they really like a certain color. Over the Hill is a phrase that is pretty well used when it comes to a 40th birthday, so you will likely find plenty of invitations around that theme. Shape can come into play as well, such as the shape of the grim reaper or a coffin.

Writing your own invitation can be fun, you can make up a funny verse for the front. Don’t feel too pressured, just think of a few funny lines and personalize them to the birthday person. The personalization of invitations makes them all the more meaningful.

Information:

Don’t forget to include the pertinent information on the invitation. This information should include:

• The name of the guest of honor and the birthday (40)

• the location of the party – including directions and a street address;

• whether or not it is a surprise (no late arrivals) and where to park so the guest of honor won’t see guest’s cars;

• the time of the party and the expected time it will end (so people don’t stay until 6:00 a.m.);

• RSVP information so each guest can reply – phone number, email address and the date that they need to reply by;

• Any other information, such as wear a costume in a certain theme, bring a food dish, bring your own booze, etc.

You can order a lot of supplies that you will need to create unique invitations online or you can create them online and have them shipped to you. You may need to upload a photo of the guest of honor to place on the front of the invitation, but creating your own invitations a great way to personalize them and make your guest of honor feel special.

Skull tattoos may appear gruesome or scary to others but those who patronized this type of tat theme actually have special meanings attached to it. They are not just tattooed on them in order to appear tough or to appear funny. In this article, we will be looking at the several variations of skull tattoo designs and the symbolism attached to them.

The very plain skull tat is originally an old school art. It was even once an insignia for groups like bikers, prisoners or gang members during the early days. However, as body art evolves, modifications and alterations for skull tattoo also came into play. Originally, its image was scary but now you can find humorous ones as well as whimsical and colorful styles. Before, they were usually combined with symbols like dagger, crossbones, flames and rose. Nowadays, anything goes as long as it would look good on one's body or as long as it can deliver the message it wants to portray. Artists seem to be having a lot of fun portraying this symbol; from cartoon skulls to terrifying Grim Reaper to realistic skull drawings. Of course, don't forget the poison sign and the pirate symbol. It can also be noticed that this tat them is not only for the male population. The female tat enthusiasts are seem to be giving it a lot of attention and thoughts too through the portrayal of colorful sugar skulls or corpse bride tattoo.

Those who have skull tattoos look upon it as their protection from death or their talisman. It can also be a symbol of near death experience or one's survival from a fatal accident or illness. Other's even consider it as a lucky charm. Whatever meaning the wearer wants to attached to it, the important thing it the personal connection and symbolism it has to them.

Do you want to throw a 40th birthday party that truly celebrates the life of the guest of honor? Then it’s time to focus on that special person and make this a happy occasion. Here are the top dos and don’ts to help get you there.

1. DON’T procrastinate. Get started right away. Give yourself enough time to come up with ideas, do the planning, and order anything custom or personalized. Make sure all the details come together with time to spare.

2. DO send out great invitations. The right invites will grab your guest’s attention, set the tone for the party and generate excitement for the upcoming festivities. One good choice is photo birthday invitations with multiple pictures of the celebrant at different ages. Or, you could select a design that ties into your theme, highlights your guest of honor’s interests, is funny or nostalgic. Just make sure it communicates that this is an occasion that can’t be missed.

3. DO ask guests to contribute photos and stories about the guest of honor. Collect them all and put them in a memory book as a gift for the celebrant. Or, you could compile them into a PowerPoint presentation to be shown at the birthday party.

4. DON’T skip the birthday party favors. It’s a nice gesture to give your guests a little parting thank you gift for sharing this happy occasion. Look for something inexpensive, useful, unique and personalized; maybe even with a photo of the celebrant. This kind of keepsake serves as a nice reminder of the wonderful celebration to all who attended.

5. DON’T make fun of the fact that he or she is turning 40. An over the hill party, complete with Grim Reaper decorations and wrinkle cream gag gifts, may seem like a good idea, but some celebrants may be uncomfortable with the joke.

According to a recent study conducted by MetLife, 65% of the population wish they were under forty. So, instead of teasing him or her about this milestone, make this a celebration of another year of growth. Why not throw a party commemorating the 19th anniversary of their 21st birthday. Unless you are absolutely sure he or she has no qualms about their age, stay away from the jabs.

6. DO look into alternatives to traditional settings for this milestone. A 40th birthday party at a restaurant, rented hall or even at home can be wonderful. But if you’re looking for something unique, you might have the celebration at the zoo, botanical gardens, amusement park, ski lodge or beach. How about inviting guests to join you for a tour of a winery, day at the spa, or a hot air balloon ride? If there’s something that the guest of honor loves to do or has always wanted to try, think about building your plans around that activity.

7. DON’T rule out a smaller celebration. Take into consideration the guest of honor’s preferences. Would he or she love to be the center of attention at a big bash? Or is the celebrant the quiet type, who would enjoy a less crowded venue? You don’t have to go over the top to make this 40th birthday party memorable. Plan a dinner cruise with a few close friends or an all night movie marathon featuring his or her favorite movies. You can emphasize the quality over the quantity.

8. DO consider a theme party. Invite your guests to a fiesta for the celebrant who is spicy at 40, and they will anticipate a fun-filled occasion. This celebration could be a tropical luau, retro 70’s dance party complete with a spinning disco ball or a costume party where guests dress up as their true inner selves. Whatever direction you choose, everyone will imagine a lively night before they even get there. Going with a theme will help break the ice when guests arrive and will keep them talking long after the event is over.

So, plan in advance. Send out eye-catching, personalized invitations. Ask the guests to share pictures and memories, then send them home with cool party favors. Build the festivities around the celebrant’s personality and interests. Make it unique. And give that special person a 40th birthday party they will never forget.

Have you ever wondered what it would be like to see through Pinhead's eyes and witness the same cruel-evil world that he does with his pinhead contact lenses? Considered the darkest and most malevolent eyes of all the cenobites, some even deem Pinhead to have the darkest stare of all the horror films.

Pinhead Contacts make for a perfect add on for a pinhead look. In addition to the Hellraiser look, you will find that these lenses also go with the following costumes:

– Metaphysical or Fictional Type Creatures
– Devil -or- Demonic Force
– Grim Reaper
– Elf -or- Goblin

You can be be the ultimate rocker at any rock concert, the scariest at the next costume party, or the sickest freak at any Goth club by slipping in the Hellraiser Contact Lenses. You can also scare the hell out of your buddy's or family -or- have some fun with your companion with the Hellraiser Contacts.

You will immediately be an authority while wearing them. Pinhead Contacts that are very realistic, comfortable to wear and are considered the maximum quality in the FX contacts industry. They are safe to use and are FDA Regulated. Available for non-prescription use only.

Pinhead Story

As leader of the cenobites, Pinhead is everyone's favorite movie monster. Sternly out to collect souls, he has been summoned from an alternative dimension by a supernatural and mechanized small box, referred to as the Lament-Configuration.

Pinhead has frightened a lot households from all 8 of his movies. The original movie was a smash hit directed by Clive Barker, which was released in 1987.

Pinheads wicked acts is considered by monster connoisseurs on the same level as Freddy krueger, Jason Voorhees and Micheal Myers. His monstrous guise features a pale and colorless face complexion, long pins driven into his skull and face, low demonic type voice, and eyes that feature an over-sized black pupil with a blood red thin iris.