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Hall of MeteoritesThe Hall of Meteorites is located in a smaller exhibition hall on the first floor of the Historical Bu...
19/11/2023

Hall of Meteorites
The Hall of Meteorites is located in a smaller exhibition hall on the first floor of the Historical Building of the National Museum. It is connected to the neighbouring Hall of Minerals and the Hall of Luminescence, or the Windows into Prehistory – Quaternary.

In addition to the meteorites which are predominant in the room, the exhibition also includes tektites, both foreign and Czech moldavites, as well as terrestrial rocks and impactites (rocks altered by the impact of a large meteorite). All exhibits are installed in the original restored showcases from 1893 with a refurbished interior. The showcases are placed continuously at the walls around most of the perimeter of the exhibition hall. In the middle of the room, there is a dominant, also original – historical, hexagonal showcase with examples of large meteorites. On the top of it is a bronze bust of Karel Vrba, the founder of the National Museum's meteorite collection. The central showcase is dominated by a 69 kg complete individual meteorite Canyon Diablo, it also contains slabs and cuttings of Toluca, Mount Joy, Gibeon, Tamarugal meteorites and a large piece of sandstone with an overgrown moldavite from the Vrábče sandpit.

The subdominant feature of the hall is the pedestal with the Argentine meteorite Campo del Cielo, which weighs impressive 83 kg. The meteorite is placed freely on the pedestal, i.e. uncovered, so that visitors can touch it. Another separate element of the room is a horizontal showcase with 155 selected backlit examples of Czech and Moravian moldavites from 29 sites.

Out of the 530 items in the museum collection 440 specimens of meteorites are on display as part of the exhibition. The two introductory showcases contain mainly texts and pictures introducing the issue of meteorites, impactites and tektites. In addition, they are dedicated to two historically observed falls of meteorites, namely Ensisheim (France 1492) and Mauerkirchen (Austria 1768). Both of these meteorites are also presented in the form of physical specimens.

The next ten showcases present meteorites arranged systematically, i.e. undifferentiated meteorites (“immature”: carbonaceous and ordinary chondrites) and then differentiated meteorites (“mature”: achondrites, mesosiderites, pallasites and siderites) respectively. Among the chondrites, the visitor should not miss the outstanding example of the famous carbonaceous chondrite Orgueil, which impacted in France in 1864. Four examples of Martian meteorites or two lunar meteorites should not escape the visitor's attention either. Among the pallasites, four meteorites of Krasnoyarsk will certainly be of interest. Throughout the exhibition, the exhibited stones are interspersed with explanatory labels with texts and pictures.

One showcase is dedicated to meteorites with a pedigree, i.e. those that have a calculated orbit in the solar system and a place of impact on Earth. The leading experts on this issue are traditionally Czech astronomers, starting with Zdeněk Ceplecha and his followers Pavel Spurný and Zdeněk Borovička. A total of ten meteorite specimens are on display in this showcase, and more should be added in the near future thanks to the planned new acquisitions into the museum collection and also a loan from the Astronomical Institute of the CAS.

Two showcases are dedicated exclusively to Czech meteorites (a total of 49 pieces), which come from a total of 18 areas such as Elbogen, Blansko, Tábor or Lysá nad Labem. One showcase is then dedicated to impactites (a total of 23 specimens). Suevites, kärnäites, shatter cones, desert glasses, irgizites and other impact rocks can be seen here.

In the following two showcases, 81 samples of the largest and also the most beautiful Czech and Moravian moldavites from the collection of the National Museum are untraditionally displayed on pedestals. Among them is, for example, a moldavite from Strpí (111 g) or a Moravian moldavite from Kožichovice (235 g) (there is a total of 236 moldavites in the entire exhibition). The oldest documented moldavite in the collection of the National Museum is also on display. It comes from Dolní Chrášťany and is perched with a large open bubble on the edge of a flat pebble with which it was allegedly found. In 1891, this moldavite was acquired by Josef Kořenský at the General Land Centennial Exhibition in Prague who donated it to the National Museum.

Two showcases are also dedicated to foreign tektites, among which indochinites predominate, but there are also philippinites, a javaite, billitonites, australites, tasmanites, bediasites and georgiaites. Terrestrial rocks are on display in the last three showcases. These were created by the gradual transformation of the original primordial matter, which we encounter today in the form of meteorites – chondrites. Selected rock specimens are presented here, on which certain geological processes can be clearly demonstrated, in several cases these processes are briefly outlined in the accompanying text labels.

19/11/2023

Exhibition of Minerals and Elements

19/11/2023
Uranium Glass
19/11/2023

Uranium Glass

19/11/2023
Hall of LuminescenceThe chamber exhibition Hall of Luminescence, located on the first floor of the Historical Building o...
19/11/2023

Hall of Luminescence
The chamber exhibition Hall of Luminescence, located on the first floor of the Historical Building of the National Museum between the Hall of Meteorites and the Windows into Prehistory –Quaternary, presents a remarkable property of some minerals, namely their interaction with ultraviolet light. UV light is invisible to the human eye, but when it hits certain types of minerals, they start to emit light of different wavelengths which we can see. This phenomenon is presented in a dark room where normal lighting alternates with short-wave and long-wave UV radiation. Thanks to this, one can experience a surprising colourful spectacle.

Learn about the minerals and rocks that "glow" under ultraviolet light.

Fluorescent minerals: One of the most spectacular museum exhibits is a dark room filled with fluorescent rocks and minerals that are illuminated with ultraviolet light. They glow with an amazing array of vibrant colors - in sharp contrast to the color of the rocks under conditions of normal illumination. The ultraviolet light activates these minerals and causes them to temporarily emit visible light of various colors. This light emission is known as "fluorescence." The wonderful photograph above shows a collection of fluorescent minerals.

The color change of fluorescent minerals is most spectacular when they are illuminated in darkness by ultraviolet light (which is not visible to humans) and they release visible light. The photograph above is an example of this phenomenon.

What is a Fluorescent Mineral?
All minerals have the ability to reflect light. That is what makes them visible to the human eye. Some minerals have an interesting physical property known as "fluorescence." These minerals have the ability to temporarily absorb a small amount of light and an instant later release a small amount of light of a different wavelength. This change in wavelength causes a temporary color change of the mineral in the eye of a human observer.

Fluorescence in More Detail
Fluorescence in minerals occurs when a specimen is illuminated with specific wavelengths of light. Ultraviolet (UV) light, x-rays, and cathode rays are the typical types of light that trigger fluorescence. These types of light have the ability to excite susceptible electrons within the atomic structure of the mineral. These excited electrons temporarily jump up to a higher orbital within the mineral's atomic structure. When those electrons fall back down to their original orbital, a small amount of energy is released in the form of light. This release of light is known as fluorescence.

The wavelength of light released from a fluorescent mineral is often distinctly different from the wavelength of the incident light. This produces a visible change in the color of the mineral. This "glow" continues as long as the mineral is illuminated with light of the proper wavelength.

How Many Minerals Fluoresce in UV Light?
Most minerals do not have a noticeable fluorescence. Only about 15% of minerals have a fluorescence that is visible to people, and some specimens of those minerals will not fluoresce. Fluorescence usually occurs when specific impurities known as "activators" are present within the mineral. These activators are typically cations of metals such as: tungsten, molybdenum, lead, boron, titanium, manganese, uranium, and chromium. Rare earth elements such as europium, terbium, dysprosium, and yttrium are also known to contribute to the fluorescence phenomenon. Fluorescence can also be caused by crystal structural defects or organic impurities.

In addition to "activator" impurities, some impurities have a dampening effect on fluorescence. If iron or copper are present as impurities, they can reduce or eliminate fluorescence. Furthermore, if the activator mineral is present in large amounts, that can reduce the fluorescence effect.

Most minerals fluoresce a single color. Other minerals have multiple colors of fluorescence. Calcite has been known to fluoresce red, blue, white, pink, green, and orange. Some minerals are known to exhibit multiple colors of fluorescence in a single specimen. These can be banded minerals that exhibit several stages of growth from parent solutions with changing compositions. Many minerals fluoresce one color under shortwave UV light and another color under longwave UV light.

Fluorite: The Original "Fluorescent Mineral"
One of the first people to observe fluorescence in minerals was George Gabriel Stokes in 1852. He noted the ability of fluorite to produce a blue glow when illuminated with invisible light "beyond the violet end of the spectrum." He called this phenomenon "fluorescence" after the mineral fluorite. The name has gained wide acceptance in mineralogy, gemology, biology, optics, commercial lighting and many other fields.

Fluorescent Geodes?
You might be surprised to learn that some people have found geodes with fluorescent minerals inside. Some of the Dugway geodes, found near the community of Dugway, Utah, are lined with chalcedony that produces a lime-green fluorescence caused by trace amounts of uranium.

Practical Uses of Mineral and Rock Fluorescence
Fluorescence has practical uses in mining, gemology, petrology, and mineralogy. The mineral scheelite, an ore of tungsten, typically has a bright blue fluorescence. Geologists prospecting for scheelite and other fluorescent minerals sometimes search for them at night with ultraviolet lamps.

Geologists in the oil and gas industry sometimes examine drill cuttings and cores with UV lamps. Small amounts of oil in the pore spaces of the rock and mineral grains stained by oil will fluoresce under UV illumination. The color of the fluorescence can indicate the thermal maturity of the oil, with darker colors indicating heavier oils and lighter colors indicating lighter oils.

Fluorescent lamps can be used in underground mines to identify and trace ore-bearing rocks. They have also been used on picking lines to quickly spot valuable pieces of ore and separate them from waste.

Many gemstones are sometimes fluorescent, including ruby, kunzite, diamond, and opal. This property can sometimes be used to spot small stones in sediment or crushed ore. It can also be a way to associate stones with a mining locality. For example: light yellow diamonds with strong blue fluorescence are produced by South Africa's Premier Mine, and colorless stones with a strong blue fluorescence are produced by South Africa's Jagersfontein Mine. The stones from these mines are nicknamed "Premiers" and "Jagers."

In the early 1900s many diamond merchants would seek out stones with a strong blue fluorescence. They believed that these stones would appear more colorless (less yellow) when viewed in light with a high ultraviolet content. This eventually resulted in controlled lighting conditions for color grading diamonds. [6]

Fluorescence is not routinely used in mineral identification. Most minerals are not fluorescent, and the property is unpredictable. Calcite provides a good example. Some calcite does not fluoresce. Specimens of calcite that do fluoresce glow in a variety of colors, including red, blue, white, pink, green, and orange. Fluorescence is rarely a diagnostic property.

https://geology.com/articles/fluorescent-minerals/

பண்டைய உலக ஏழு அதிசயங்களில் ஒன்று:4600 வருடங்கள் பழமையான Giza Pyramid (எகிப்து)-----------------------------------------...
19/07/2023

பண்டைய உலக ஏழு அதிசயங்களில் ஒன்று:
4600 வருடங்கள் பழமையான Giza Pyramid (எகிப்து)
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பிரமிட்டை கட்டுவித்தவரின் சவப்பெட்டி வைக்கப்பட்டிருந்த அறையில் ஒரு நாள்
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எகிப்து நாட்டின் ,கிஸா எனும் பிரதேசத்தில் உள்ள Khufu Khafre, Menkaure என்றழைக்கப்படும் மூன்று பெரிய பிரமிட்களும் உலகின் பண்டைய ஏழு அதிசயங்களில் ஒன்றாகும் .

கிசா பிரமிட் வளாகத்தில் உள்ள மூன்று பிரமிடுளும் உலகில் மிகப் பழமையானதும் மற்றும் மிகப்பெரியதும் ஆகும் அதிலும் 'KUFU' என்றழைக்கப்படும் மிக உயரமான பிரமிட் சுமார் 4600 வருடங்களுக்கு முன்னர் பிர்அவ்ன் வம்சத்தின் 4 ஆவது வம்ச அரசரான 'KUFU' என்ற அரசரால் அவரின் இறந்த உடலை (Mummy) வைக்க கட்டுவிக்கப்பட்டுள்ளது .

*கட்டுவதற்கு எடுக்கப்பட்ட காலம் - 20 ஆண்டுகள்
*கட்டுமானப் பணிகளில் ஈடுபடுத்தப் பட்டோர் -1 இலட்சம் ஆண்கள்
*உயரம் 146.5 மீட்டர் (481 அடி)
*உள்ள கற்களின் (Lime stones ) எண்ணிக்கை - 2.3 மில்லியன் கற்கள்
*திணிவு 5.9 மில்லியன் டன்கள்
*கன அளவு சுமார் 2,500,000 கன மீட்டர்.

பண்டைய உலக ஏழு அதிசயங்களில் ஒன்று:2300 வருடங்கள் பழமையான அலெக்சாந்திரியாவின் கலங்கரை விளக்கம் (எகிப்து)-----------------...
17/07/2023

பண்டைய உலக ஏழு அதிசயங்களில் ஒன்று:
2300 வருடங்கள் பழமையான அலெக்சாந்திரியாவின் கலங்கரை விளக்கம் (எகிப்து)
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அலெக்சாந்திரியாவின் கலங்கரை விளக்கம் (அல்லது அலெக்சாந்திரியாவின் ஃபாரோஸ், கி.மு மூன்றாம் நூற்றாண்டில் (285க்கும் 247க்கும் இடைப்பட்ட காலத்தில்) எகிப்தின் அலெக்சாந்திரியாவின் மத்திய தரை கடல் பிரதேசத்தில் உள்ள பாரோஸ் தீவில் துறைமுகத்தை அடையாளம் காணும் விதமாகக் கட்டப்பட்ட கோபுரமாகும். பின்னர் இது கலங்கரைவிளக்கமாகவும் செயல்பட்டது.

115இலிருந்து 135 மீட்டர் வரை மதிப்பிடப்படும் இதன் உயரம் அந்நாளைய உலகின் மூன்றாம் (பிரமிட்கள் குஃபு மற்றும் காஃபரா அடுத்து) உயரமான கட்டிடமாகக் கருதப்படுகிறது.
பழங்கால உலகின் ஏழு அதிசயங்களில் இதுவும் ஒன்றாகும். இந்தக் கலங்கரை விளக்கம் கி.பி. 956,1303 மற்றும் 1323 ஆண்டுகளின் நிலநடுக்கங்களின் போது அழிபட்டது. 1480 ஆம் ஆண்டு அழிபட்ட கட்டிடத்தின் கற்களைக் கொண்டு அங்கு ஓர் கோட்டை (Citadel of Qaitbay) எழுப்பப்பட்ட பின் முழுமையாக பழமையான கட்டிடத்தின் இடிபாடுகள் அழிந்தன. 1994 இல் பிரான்சு தொல்பொருள் ஆய்வாளர்கள் அலெக்சாந்திரியாவின் கிழக்குத துறைமுக கடலின் அடியில் புராதன கலங்கரை விளக்கதத்தின் சில பகுதிகளை கண்டுபிடித்தனர்.

Citadel of Qaitbay இப்போது எகிப்தின் முக்கிய ஒரு சுற்றுலா தளமாகும்.

ஹரீஸ் ஸாலிஹ்
22.09.2017

The Haramain high-speed railway (Arabic: قطار الحرمين السريع, also known as the Western railway or Mecca–Medina high-spe...
08/12/2022

The Haramain high-speed railway
(Arabic: قطار الحرمين السريع, also known as the Western railway or Mecca–Medina high-speed railway, is a 453-kilometre-long (281 mi) high-speed rail line in Saudi Arabia. It links the Muslim holy cities of Medina and Mecca via King Abdullah Economic City and Jeddah, using 449.2 kilometres (279.1 mi) of main line and a 3.75-kilometre (2.33 mi) branch connection to King Abdulaziz International Airport (KAIA), in Jeddah. The line is designed for a top speed of 300 km/h (190 mph). Construction on the project began in March 2009, was officially inaugurated on 25 September 2018,[5] and opened to the public on 11 October 2018. The railway is expected to carry 60 million passengers a year, including around 3-4 million Hajj and Umrah pilgrims, helping to relieve traffic congestion on the roads. It does not connect with the Mecca Metro. On March 31, 2021 the first trip to Madinah was launched and the operations between Makkah and Madinah will resume after they were postponed from March 20, 2020 due to the COVID-19 pandemic.

The Haramain high-speed railway (Arabic: قطار الحرمين السريع, also known as the Western railway or Mecca–Medina high-speed railway, is a 453-kilometre-long (...

ரஸூல் (ஸல்) அவர்களின் வீட்டுக்குச் சென்று "ரவ்தா ஷரீப்" இல்  ஒரு பொழுது روضة الجنة في المسجد النبوي10.11.2022
23/11/2022

ரஸூல் (ஸல்) அவர்களின் வீட்டுக்குச் சென்று "ரவ்தா ஷரீப்" இல் ஒரு பொழுது
روضة الجنة في المسجد النبوي
10.11.2022

Masjid An Nabavi and Rawda Shareef ரஸூல் (ஸல்) அவர்களின் வீட்டுக்குச் சென்று "ரவ்தா ஷரீப்" இல் ஒரு பொழுது روضة الجنة في المسجد النبوي10.11.2022

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