Showing posts with label Science. Show all posts
Showing posts with label Science. Show all posts

Saturday 25 January 2020

How Stars Shines and What is Nearest Star?

Every bright star is a sun, like our own sun. This means that stars are giant globes of glowing gas. They are extremely hot that if a piece of steel were placed there, it would disappear in a puff or gas! In many of the starts, the gases are very thin. This is because the particles, or atoms, of matter n the gas are so far apart.
But the stars do have matter in them. We may be acquainted with, for example, that the sun contains more than 60 of the chemical elements present in the earth. So, among the elements in the sun are hydrogen, helium, iron, calcium, and magnesium.
Therefore, in the cooler stars, the matter may be more almost liquid, somewhat like the boiling iron in a blast furnace. In some very old and cold starts, the matter may be so compactly packed that a cubic inch of it would weigh a ton. Such stars are called “dead” or “dark” stars.
Astronomers can find out all this by using instruments called “Spectroscopes”. The spectroscope studies the light a star gives, and forms this we can learn what kinds of matter it contains and how hot it is. The different colors of the stars, white, blue, yellow or red indicate what chemical elements are present in them.
Hence, the different temperatures of starts also cause differences in the light they give in their spectrum. In this way the temperature of a star can be determined.

How Many Stars Can We See at Night?

Wow, that is amazing question; myriad stars are visible on the sky in the night. This is the true impression we get of the sky when we look up in the sky at night and see the stars. But it may astonish you to know that only about 6,000 stars can be seen without a telescope.
That does not mean a human can look up and count six thousand stars. However, the one-fourth of these 6,000 stars is too far south to be able to be seen in Western Europe. And of the stars that can be seen from any one place on earth. Only one-half are visible at one time as the others are below the horizon.
What’s more, many of the stars close to the horizon cannot be seen because of haze or light pollution. So what do we end p with? If you started to count the stars that you could see, you would perhaps not be able to count many stars, may be around 1,000.
Photographs can be taken of the same sky by a camera attached to a telescope. Many more stars can be counted on a photograph of a particular spot in the sky than the unaided eye can see there. And with a time exposure, even more stars will be added.
At last, by using a very powerful telescope it would be possible to photograph more than 1,000,000,000 stars. Once a star is being noticed in the sky it must be given a name or a classification number.
Moreover, long time ago, people in the lands of Arabs, the Greeks, the Romans, and the Chinese were star gazing and gave them names to the brightest stars and to other stars that were in some way amazing. More than one hundred stars were given names.
And human beings wanted to have a catalogue of the stars that were recognized. The first ever which is known for star catalogue listed 1,025 stars and dated from about A.D. 137. A modern catalogue of the stars lists more than 500,000 stars.

What Are The Nearest Stars?

Sometimes we can measure something and yet have no real understanding of what that measurement means. When it comes to distance in the universe, for example, we are able to measure them. But our minds cannot really grasp what that means in terms of our life.
For distance in the universe, a special unit of measurement was set up, that was called “the light year”. A light year is simply the distance a ray of light will travel in a year. Since light travels about 186,000 miles a second, so in one year it will travel a distance of nearly six billion miles.
The closest star to us is “Proxima Centauri”, and this is about four and a third light years away. That means a distance of 26 billion miles. This star can be seen from the Southern Hemisphere. The nearest star in the Northern Hemisphere is Sirius. It is eight light years away.
The farthest stars we can see with the naked eye are about 8,000,000 light years away. When we look through powerful telescope, we can see stars thousand times farther away. Through such telescope stars are thousand trillion miles away can be seen. The light from these stars started out a thousand millions years ago on its way to the earth.

What Makes the Stars Shine?

A star is a ball of very hot gas which shines by its own light. Planets as you know, and our moon, too shine only by light reflected from the sun. And planets shine with a steady light while stars appear to twinkle. This is due to the substances in the air between the star and the earth.
Hence, the unsteady air bends the light from the star, and then it seems to twinkle. The question is why does our sun shine so brightly? Because it is also a star not a very big or bright star at that! However, to be compared to all the other stars in the sky, it might be measured medium sized and medium-bright.
Furthermore, there are millions of stars that are smaller than our sun. And numerous stars are several hundred times larger than the sun. No matter, they look small only because they are so far away. Ever since the days of the Greek astronomers some 2,000 years ago or brightness!
Another way of grouping stars in according to their spectra or the kind of light that comes from the stars. By studying the difference in these spectra, the astronomer may find out about the colors, and temperature, and even the chemical composition of the stars.

Why Are Some Stars Brighter Than Others?

Therefore, when we look up at the sky, we do not see too many differences among the stars. Some look a bit bigger, some are brighter than others. But we really cannot get a good idea of the great differences that exist among them.
One way of classifying stars is by their spectra is a breakdown of the light given off. So, in this way, stars range from blue stars to red stars. Moreover, keep in mind that our sun is considered to be yellow, and is in the middle of the series. Therefore, the blue stars are big, hot and radiant.
Their surface temperatures may be as high as 27,750 degrees or more. The sun is medium bright and has a surface temperature of about 6,000 degrees. However, the red stars are rather cool and have surface temperatures of 1,650 degrees or less. Hence, you can see that some stars are very much brighter than other stars. But, because of their great distance from the earth we are not aware of it.
Therefore, the brightness of a star is called its “magnitude”. A star of any given magnitude is about to and a half times fainter than a star of the magnitude above it. So, magnitude is a sort of weighing machine for measuring brightness. The stars fainter than the sixth magnitude are the brightest, and there are concerning 20 such stars we know of. But there are at least a thousand million stars that are only of the twentieth magnitude.
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Monday 20 August 2018

The UFO Shaped Lenticular Clouds

Lenticular Clouds are also called Altocumulus lenticularis are stationary lens-shaped clouds that form in the troposphere. It is usually in perpendicular alignment to the wind direction. Lenticular clouds can be separated into ACSL, (Altocumulus Standing Lenticularis) or SCSL (Stratocumulus Standing Lenticular), and CCSL, (Cirrocumulus Standing Lenticular). Because of their rare shape, they’ve been observed as an explanation for some UFO (Unidentified Flying Object), sightings. As air flows along the surface of the Earth, it comes across obstacles. However, our atmosphere, the envelope of air surrounding of planet, is always in motion. We have a tendency to to think of the motion of our atmosphere as horizontal across the ground, namely wind. Though, air can move vertically as well. Also Read: Glowworms Transform Cave into a Fascinating Starry Sky
Source: CP



Saturday 27 September 2014

Water is The Vital Source to Increase the Life on Earth & Other Planets



Everyone knows the importance of water on planet earth; no one can survive without water. So water was a vital source to increase the life on Earth and also imperative to evaluating the possibility of life on other planets. However to identifying the original source of Earth’s water is important to understanding how life-fostering environments come into being and how unlikely they’re to be found elsewhere. New work from a team, including Carnegie’s Conel Alexander, observed that plenty of our solar system’s water perhaps originated as ices that formed in interstellar space. However; water is found throughout our solar system, not just on Earth, but on icy comets and moons and in the shadowed basins of Mercury. Thus water has been found included in mineral samples from meteorites, the Moon, and Mars.

Comets and asteroids in specific, being basic objects, deliver a natural “time capsule” of the conditions during the early days of our solar system. Their ices can tell experts regarding the ice that encircled the Sun after its birth, the origin of which was an unanswered question until now. In its youth, the Sun was surrounded by a proto-planetary disk, the so-called solar nebula, from which the planets were born. But it was unclear to scientists whether the ice in this disk created from the Sun’s own parental interstellar molecular cloud, from which it was created, or whether this interstellar water had been damaged and was recreated by the chemical reactions taking place in the solar nebula.

A Graduate Student Created First Man Made Bilological Leaf Which Can Produce Oxygen Just Like a Plant

A graduate student Julian Melchiorri has created a biological leaf. That has the ability to absorb water and carbon dioxide to produce oxygen just like a plant. Julian did this by suspending chloroplasts in a mixture made out of silk protein. He believed it can be used for several things but the most incredible one is the thought that it could be used for long distance space travel. Plants do not grow in space, but this synthetic material can be used to produce oxygen in a hostile environment. The silk Leaf is composed of chloroplasts suspended in silk proteins, for the express purpose of long-distance space travel.  

 He says; plants don't grow in zero gravity. Therefore; "NASA is researching diverse ways to create oxygen for long-distance space journeys to let us live in space. This material could allow us to explore space much further than we can now. This incredible finished product functions like a plant in the sense that it is biological and produces oxygen, but its synthetic packaging makes it more likely to be able to survive in extraterrestrial environments.

Interestingly just like a real plant, it only requires light and water to survive and photosynthesize:  Because Silk Leaf is the first man-made biological leaf and it is very light, low energy-consuming, entirely biological. Therefore; it is really very convenient and can extend even further, as making lamps out of Silk Leaf kills two birds with one stone. My idea was to increase the efficiency of nature in a man-made environment. I created some lighting out of this material, using the light to illuminate the house but at the same time to create oxygen for us.


Thursday 24 July 2014

An extraterrestrial spacecraft lurking in a satellite’s orbit nearby Earth would be able to see city lights and pollution in our atmosphere. But what if it searched for signs of life on Earth from afar

An extraterrestrial spacecraft lurking in a satellite’s orbit nearby Earth would be able to see city lights and pollution in our atmosphere. But what if it searched for signs of life on Earth from afar? This question has great pertinence to those searching for other Earths outside of our solar system. NASA’s Keppler space telescope is among a fleet of telescopes and spacecraft searching for rocky planets alike to our own. Once the size and location of these worlds are plotted, the next step is examining the chemical composition of their atmospheres.

Tuesday 1 July 2014

NASA Releases Stunningly Colorized Photograph of Our Sun



NASA's SDO (Solar Dynamics Observatory) has just released this stunning, painterly image of the Sun. The Solar Dynamics observatory was designed to assist us to know about the Sun's influence on Earth and near-Earth space by studying the solar atmosphere. In this lovely image, NASA's sun-gazing spacecraft spotted an unusual series of eruptions, forced by fast "puffs" from the Sun's outermost atmosphere (the corona), to interplanetary space. It starts on January 17, 2013, the puffs took place about once every 3 hours, and then after twelve hours, larger eruptions occurred.

Nathalia Alzate a solar scientist at the University of Aberystwyth in Wales said; if you look at the corona in intense ultraviolet light we can review the source of the puffs is a series of energetic jets and related flares. The jets are localized, disastrous releases of energy that spew material out from the sun into space. These swift changes in the magnetic field cause flares, which release an enormous amount of energy in a very limited time in the form of super-heated plasma, high-energy radiation and radio bursts. The large, slow structure is unwilling to erupt, and does not originate to smoothly propagate outwards until numerous jets have occurred. 

We still need some time to evaluate whether these’re shock waves, formed by the jets, passing through and driving the slow eruption, or whether magnetic reconfiguration is driving the jets letting the bigger, slow structure to slowly erupt. Many thanks to latest advances in observation and in photo processing techniques we can throw light on the way jets can lead to small and fast, or big and slow, eruptions from the Sun. She continues; this spectacular photograph is a combination of three wavelengths of light. It shows one of the multiple jets that led to a series of slow coronal puffs. The striking photo has been colorized in red, green and blue.