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Rh-Null blood or the Golden blood Rh-Null phenotype is a rare blood group characterized by the lack of expression of all Rh a
Rh-Null blood or the Golden blood Rh-Null phenotype is a rare blood group characterized by the lack of expression of all Rh antigens (D, C, c, E and e) on the red cells. The phenotype is further classified into the regulator and amorph type based on underlying genetic defect. The clinical significance of its recognition is that such patients suffer from Rhnull syndrome associated with osmotically fragile red cells called stomatocytes with subsequent chronic haemolytic anaemia of varying degree. Another importance is that such subjects readily form alloantibodies on exposure to Rh antigens. We report herein rare Rhaull phenotype in a young pregnant female which was detected as a part of routine antenatal work-up for red cell antibody screening and identification.

The theory of relativity (In a bit simple) The theory of relativity usually encompasses two interrelated physics theories by
The theory of relativity (In a bit simple) The theory of relativity usually encompasses two interrelated physics theories by Albert Einstein: special relativity and general relativity, proposed and published in 1905 and 1915, respectively. Special relativity applies to all physical phenomena in the absence of gravity. General relativity explains the law of gravitation and its relation to the forces of nature. It applies to the cosmological and astrophysical realm, including astronomy. The theory transformed theoretical physics and astronomy during the 20th century, superseding a 200-year-old theory of mechanics created primarily by Isaac Newton. It introduced concepts including 4-dimensional spacetime as a unified entity of space and time, relativity of simultaneity, kinematic and gravitational time dilation, and length contraction. In the field of physics, relativity improved the science of elementary particles and their fundamental interactions, along with ushering in the nuclear age.

Expansion Of The Universe The expansion of the universe is the increase in distance between any two given gravitationally unb
Expansion Of The Universe The expansion of the universe is the increase in distance between any two given gravitationally unbound parts of the observable universe with time. It is an intrinsic expansion whereby the scale of space itself changes. The universe does not expand "into" anything and does not require space to exist "outside" it. This expansion involves neither space nor objects in space "moving" in a traditional sense, but rather it is the metric that changes in scale. As the spatial part of the universe's spacetime metric increases in scale, objects become more distant from one another at ever-increasing speeds. To any observer in the universe, it appears that all of space is expanding, and that all but the nearest galaxies recede at speeds that are proportional to their distance from the observer. While objects within space cannot travel faster than light, this limitation does not apply to the effects of changes in the metric itself. The objects beyond the horizon are unobservable.

Spaghettification In astrophysics, spaghettification (sometimes referred to as the noodle effect) is the vertical stretching
Spaghettification In astrophysics, spaghettification (sometimes referred to as the noodle effect) is the vertical stretching and horizontal compression of objects into long thin shapes (rather like spaghetti) in a very strong, non-homogeneous gravitational field. It is caused by extreme tidal forces. In the most extreme cases, near a black hole, the stretching and compression are so powerful that no object can resist it. Within a small region, the horizontal compression balances the vertical stretching so that a small object being spaghettified experiences no net change in volume.

Ball Lightning Ball lightning is a rare and unexplained phenomenon described as luminescent, spherical objects that vary from
Ball Lightning Ball lightning is a rare and unexplained phenomenon described as luminescent, spherical objects that vary from pea-sized to several meters in diameter. Though usually associated with thunderstorms, the observed phenomenon is reported to last considerably longer than the split-second flash of a lightning bolt, and is a phenomenon distinct from St. Elmo's fire. Some 19th-century reports describe balls that eventually explode and leave behind an odor of sulfur. Descriptions of ball lightning appear in a variety of accounts over the centuries and have received attention from scientists. An optical spectrum of what appears to have been a ball lightning event was published in January 2014 and included a video at high frame rate. Laboratory experiments have produced effects that are visually similar to reports of ball lightning, but how these relate to the supposed phenomenon remains unclear.

Dark energy Dark energy makes up approximately 68% of the universe and appears to be associated with the vacuum in space. It
Dark energy Dark energy makes up approximately 68% of the universe and appears to be associated with the vacuum in space. It is distributed evenly throughout the universe, not only in space but also in time – in other words, its effect is not diluted as the universe expands. The even distribution means that dark energy does not have any local gravitational effects, but rather a global effect on the universe as a whole. This leads to a repulsive force, which tends to accelerate the expansion of the universe. The rate of expansion and its acceleration can be measured by observations based on the Hubble law. These measurements, together with other scientific data, have confirmed the existence of dark energy and provide an estimate of just how much of this mysterious substance exists.

Law Of Conservation Of Energy In physics and chemistry, the law of conservation of energy states that the total energy of an
Law Of Conservation Of Energy In physics and chemistry, the law of conservation of energy states that the total energy of an isolated system remains constant; it is said to be conserved over time. Energy can neither be created nor destroyed; rather, it can only be transformed or transferred from one form to another. For instance, chemical energy is converted to kinetic energy when a stick of dynamite explodes. If one adds up all forms of energy that were released in the explosion, such as the kinetic energy and potential energy of the pieces, as well as heat and sound, one will get the exact decrease of chemical energy in the combustion of the dynamite.

Nuclear Energy Nuclear power is dirty, dangerous and expensive; not carbon-free; and encourages nuclear proliferation. A nucl
Nuclear Energy Nuclear power is dirty, dangerous and expensive; not carbon-free; and encourages nuclear proliferation. A nuclear power station itself does not emit greenhouse gasses like CO2.Yet nuclear power contributes to climate change; with every step in the whole fuel chain, needed to generate electricity in the end, many energy is used.For instance, the extraction of uranium and the enrichment of uranium are extremely energy-intensive processes. Life-cycle analysis of the whole fuel chain clearly shows the contribution of nuclear power to climate change.In a ground breaking study Sovacool et al screened 103 lifecycle studies of greenhouse gas equivalent emissions for nuclear power plants to identify a subset of the most current, original, and transparent studies. They calculated that while the range of emissions for nuclear energy over the lifetime of a plant reported from qualified studies examined is from 1.4 grams of carbon dioxide equivalent per kWh to 288 gCO2e/kWh, the mean value is 66 gCO2e/kWh.

Atmospheric Pressure Atmospheric pressure, also known as air pressure or barometric pressure (after the barometer), is the pr
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Atmospheric Pressure Atmospheric pressure, also known as air pressure or barometric pressure (after the barometer), is the pressure within the atmosphere of Earth. The standard atmosphere (symbol: atm) is a unit of pressure defined as 101,325 Pa (1,013.25 hPa), which is equivalent to 1,013.25 millibars,[1] 760 mm Hg, 29.9212 inches Hg, or 14.696 psi.[2] The atm unit is roughly equivalent to the mean sea-level atmospheric pressure on Earth; that is, the Earth's atmospheric pressure at sea level is approximately 1 atm. In most circumstances, atmospheric pressure is closely approximated by the hydrostatic pressure caused by the weight of air above the measurement point. As elevation increases, there is less overlying atmospheric mass, so atmospheric pressure decreases with increasing elevation.

Cosmic Dust Cosmic dust, also called extraterrestrial dust, space dust, or star dust is dust that occurs in outer space or ha
Cosmic Dust Cosmic dust, also called extraterrestrial dust, space dust, or star dust is dust that occurs in outer space or has fallen onto Earth. Most cosmic dust particles measure between a few molecules and 0.1 mm (100 μm), such as micrometeoroids. Larger particles are called meteoroids. Cosmic dust can be further distinguished by its astronomical location, intergalactic dust, interstellar dust, interplanetary dust, and circumplanetary dust. There are several methods to obtain space dust measurement. In the Solar System, interplanetary dust causes the zodiacal light. Solar System dust includes comet dust, planetary dust, asteroidal dust, dust from the Kuiper belt, and interstellar dust passing through the Solar System. Thousands of tons of cosmic dust are estimated to reach Earth's surface every year, with most grains having a mass between 10−16 kg (0.1 pg) and 10−4 kg (0.1 g). The density of the dust cloud through which the Earth is traveling is approximately 10−6 dust grains/m3.

The Blue Skinned Family A family of people with blue skin lived in Kentucky for many generations. The Fulgates of Troublesome
The Blue Skinned Family A family of people with blue skin lived in Kentucky for many generations. The Fulgates of Troublesome Creek are thought to have gained their blue skin through combination of inbreeding and a rare genetic condition known as methemoglobinemia. @Sci_Strangeries

A railgun (also spelled rail gun) is a linear motor device, typically designed as a weapon, that uses electromagnetic force t
A railgun (also spelled rail gun) is a linear motor device, typically designed as a weapon, that uses electromagnetic force to launch high-velocity projectiles. The projectile normally does not contain explosives, instead relying on the projectile's high kinetic energy to inflict damage. The railgun uses a pair of parallel conductors (rails), along which a sliding armature is accelerated by the electromagnetic effects of a current that flows down one rail, into the armature and then back along the other rail. It is based on principles similar to those of the homopolar motor.

The demon core was a spherical 6.2-kilogram subcritical mass of plutonium 89 millimeters in diameter, manufactured during Wor
The demon core was a spherical 6.2-kilogram subcritical mass of plutonium 89 millimeters in diameter, manufactured during World War II by the United States nuclear weapon development effort, the Manhattan Project, as a fissile core for an early atomic bomb. A square base of metal blocks, with a smaller square of metal on the top in the center, a metal ball contained in its center. A ruler along one side of the base shows it is roughly 10.5 inches square. The core was prepared for shipment as part of the third nuclear weapon to be used in Japan, but when Japan surrendered, the core was retained at Los Alamos for testing and potential later use. It was involved in two criticality accidents at the Los Alamos Laboratory on August 21, 1945, and May 21, 1946, each resulting in a fatality. Both experiments were designed to demonstrate how close the core was to criticality with a tamper, but in each case, the core was accidentally placed into a critical configuration.

Pillars Of Creation Pillars of Creation is a photograph taken by the Hubble Space Telescope of elephant trunks of interstella
Pillars Of Creation Pillars of Creation is a photograph taken by the Hubble Space Telescope of elephant trunks of interstellar gas and dust in the Eagle Nebula, in the Serpens constellation, some 6,500–7,000 light-years (2,000–2,100 pc; 61–66 Em) from Earth. These elephant trunks had been discovered by John Charles Duncan in 1920 on a plate made with the Mount Wilson Observatory 60-inch telescope. They are named so because the gas and dust are in the process of creating new stars, while also being eroded by the light from nearby stars that have recently formed. Closer view of one pillar Taken on April 1, 1995, it was named one of the top ten photographs from Hubble by Space.com. The astronomers responsible for the photo were Jeff Hester and Paul Scowen from Arizona State University. The region was rephotographed by ESA's Herschel Space Observatory in 2011, again by Hubble in 2014 with a newer camera, and the James Webb Space Telescope in 2022.

Neutron Star A neutron star is the collapsed core of a massive supergiant star, which had a total mass of between 10 and 25 s
Neutron Star A neutron star is the collapsed core of a massive supergiant star, which had a total mass of between 10 and 25 solar masses (M☉), possibly more if the star was especially metal-rich. Except for black holes, neutron stars are the smallest and densest currently known class of stellar objects. Neutron stars have a radius on the order of 10 kilometres and a mass of about 1.4 M☉. They result from the supernova explosion of a massive star, combined with gravitational collapse, that compresses the core past white dwarf star density to that of atomic nuclei. Once formed, neutron stars no longer actively generate heat and cool over time; however, they may still evolve further through collision or accretion.

Difference between Fission and Fusion Fission and fusion are nuclear reactions that produce energy. These two nuclear process
Difference between Fission and Fusion Fission and fusion are nuclear reactions that produce energy. These two nuclear processes use the binding energy of the protons and neutrons in the nucleus of atoms to release an enormous amount of energy. The main difference is that fission is the splitting of a heavy, unstable nucleus into two smaller nuclei, while fusion reactions involve combining two light nuclei together Nuclear fusion is the process of combining atomic nuclei rather than splitting them to produce energy. This process occurs naturally in the centre of stars like the Sun and creates no long-term radioactive waste or greenhouse gases. In the other hand Nuclear fission involves the splitting of atoms to release the binding energy of the atomic nuclei. This energy is released as heat and radiation, with the heat being used by a nuclear power plant to boil water into steam to turn a turbine and drive generators to produce electricity. As the process uses uranium rather than fossil fuels.

A Hypernova A hypernova (sometimes called a collapsar) is a very energetic supernova thought to result from an extreme core-c
A Hypernova A hypernova (sometimes called a collapsar) is a very energetic supernova thought to result from an extreme core-collapse scenario. In this case, a massive star (>30 solar masses) collapses to form a rotating black hole emitting twin energetic jets and surrounded by an accretion disk. It is a type of stellar explosion that ejects material with an unusually high kinetic energy, an order of magnitude higher than most supernovae, with a luminosity at least 10 times greater. They usually appear similar to a type Ic supernova, but with unusually broad spectral lines indicating an extremely high expansion velocity. Hypernovae are one of the mechanisms for producing long gamma ray bursts (GRBs), which range from 2 seconds to over a minute in duration. They have also been referred to as superluminous supernovae, though that classification also includes other types of extremely luminous stellar explosions that have different origins.

Nuclear Fusion Nuclear fusion is a reaction in which two or more atomic nuclei, usually deuterium and tritium (hydrogen varia
Nuclear Fusion Nuclear fusion is a reaction in which two or more atomic nuclei, usually deuterium and tritium (hydrogen variants), are combined to form one or more different atomic nuclei and subatomic particles (neutrons or protons). The difference in mass between the reactants and products is manifested as either the release or absorption of energy. This difference in mass arises due to the difference in nuclear binding energy between the atomic nuclei before and after the reaction. Nuclear fusion is the process that powers active or main-sequence stars and other high-magnitude stars, where large amounts of energy are released.

Hercules–Corona Borealis Great Wall The Hercules–Corona Borealis Great Wall is the largest known superstructure in the univer
Hercules–Corona Borealis Great Wall The Hercules–Corona Borealis Great Wall is the largest known superstructure in the universe. It is a huge group of galaxies forming a giant sheet-like pattern which is about 10 billion light-years long, 7.2 billion light-years wide, and almost 1 billion light-years thick. It is about 10 billion light-years away in the constellations of Hercules and Corona Borealis, hence its name. It was discovered in November 2013 by mapping gamma-ray bursts. They are very luminous explosions of distant, massive stars, the most powerful explosions in the universe. A typical burst releases more energy in less than a tenth of a second than the Sun will in its whole life of 10 billion years.