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Periodic Table – Law of Triads

periodic table

Law of Triads

The development of the periodic table begins with German chemist Johann Dobereiner (1780-1849) who  grouped elements based on similarities.  Calcium (atomic weight 40), strontium (atomic weight 88), and barium (atomic weight 137) possess similar chemical prepares.  Dobereiner noticed the atomic weight of strontium fell midway between the weights of calcium and barium:
Ca   Sr   Ba     (40 + 137) ÷ 2 = 88
40     88     137

Was this merely a coincidence or did some pattern to the arrangement of the elements exist? Dobereiner  noticed the same pattern for the alkali metal triad (Li/Na/K) and the halogen triad (Cl/Br/I).
Li   Na  K         Cl   Br   I
7     23     39           35    80   127

In 1829 Dobereiner proposed the Law of Triads: Middle element in the triad had atomic weight that was the average of the other two members. Soon other scientists found chemical relationships extended beyond triads. Fluorine was added to Cl/Br/I group; sulfur, oxygen, selenium and tellurium were grouped into a family; nitrogen, phosphorus, arsenic, antimony, and bismuth were classified as another group.

Döbereiner’s classification scheme was improved and perfected by Mendeléev.

Law of Octaves

Law of Octaves

English chemist John Newlands (1837-1898), having arranged the 62 known elements in order of increasing atomic weights, noted that after interval of eight elements similar physical/chemical properties reappeared.  Newlands was the first to formulate the concept of periodicity in the properties of the chemical elements. In 1863 he wrote a paper proposing the Law of Octaves: Elements exhibit similar behavior to the eighth element following it in the table.

Mendeleev’s Periodic Table

Mendeleev's Periodic Table

Then in 1869, Russian chemist Dimitri Mendeleev (1834-1907) proposed arranging elements by atomic weights and properties (Lothar Meyer independently reached similar conclusion but published results after Mendeleev).  Mendeleev’s periodic table of 1869 contained 17 columns with two partial periods of seven elements each (Li-F & Na-Cl) followed by two nearly complete periods (K-Br & Rb-I).

In 1871 Mendeleev revised the 17-group table with eight columns (the eighth group consisted of transition elements). This table exhibited similarities not only in small units such as the triads, but showed similarities in an entire network of vertical, horizontal, and diagonal relationships. The table contained gaps but Mendeleev predicted the discovery of new elements.  In 1906, Mendeleev came within one vote of receiving the Nobel Prize in chemistry.

Mendeléev, Dmitri (1834-1907)
Russian chemist who arranged the 63 known elements into a periodic table  based on atomic mass,  which he published in Principles of Chemistry in 1869. This organization surpassed attempts at classification by Beguyer de Chancourtois and Newlands and was published a year before the work of Lothar Meyer. Mendeléev left space for new elements, and predicted three yet-to-be-discovered elements including eka-silicon and eka-boron. His table did not include any of the noble gases , however, which had not yet been discovered. His table placed elements in their correct position by atomic number, thus showing variance from atomic weight in a number of places.

Moseley’s Periodic Law

Moseley's Periodic Law

Soon after Rutherford’s landmark experiment of discovering the proton in 1911, Henry Moseley (1887-1915) subjected known elements to x-rays. He was able to derive the relationship between x-ray frequency and number of protons. When Moseley arranged the elements according to increasing atomic numbers and not atomic masses, some of the inconsistencies associated with Mendeleev’s table were eliminated. The modern periodic table is based on Moseley’s Periodic Law (atomic numbers). At age 28, Moseley was killed in action during World War I and as a direct result Britain adopted the policy of exempting scientists from fighting in wars.  Shown above is a periodic table from 1930:

The Beacon website:

At The Beacon, we have created a Periodic Table of Technology to teach about science and technology by showing how elements are used in everyday tech-use. The interactive guide is a supplement to the other learning resources.

See The Periodic Table of Technology website here.

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gastrulation

The three layers of the embryo are

  1. Endoderm 
  2. Ectoderm 
  3. Mesoderm

gastrulation

During gastrulation, three major cell lineages are being established. They are the Ectoderm, Mesoderm and Endoderm. Following gastrulation, various cell lineages are derrived from these three primary cell types. For example, the Ectoderm gives rise to the epidermis and its derrivatives such as nails, hair and teeth. On the other hand, the Ectoderm also gives rise to the Central Nervous System.

Gastrulation

“It is not birth, marriage, or death, but gastrulation, which is truly the most important time in your life.”
Lewis Wolpert (1986)

gastrulationDuring gastrulation, cell movements result in a massive reorganization of the embryo from a simple spherical ball of cells, the blastula, into a multi-layered organism. During gastrulation, many of the cells at or near the surface of the embryo move to a new, more interior location.

The primary germ layers (endoderm, mesoderm, and ectoderm) are formed and organized in their proper locations during gastrulation. Endoderm, the most internal germ layer, forms the lining of the gut and other internal organs. Ectoderm, the most exterior germ layer, forms skin, brain, the nervous system, and other external tissues. Mesoderm, the the middle germ layer, forms muscle, the skeletal system, and the circulatory system.

Scientists

Pander, Christian (1794-1865) was the Russian zoologist who studied the chick embryo. He discovered the three layers that form in the early development of the embryo, and is considered the father of embryology. Pander’s work was extended by Baer.

Remak, Robert (1815-1865) was the German physician who is the founder of electrotherapy. He also reduced the four germ layers of Baer to three and gave them their modern names of ectoderm, mesoderm, and endoderm. Remak devised a cellular interpretation of vertebrate development.

© 1996-2007 Eric W. Weisstein

Origin of EMBRYO

Medieval Latin embryon-, embryo, from Greek embryon,from en-bryein to swell; akin to Greek bryon catkin

First Known Use: 1548

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Atmospheric layers of the sun

The Sun is a ball of gas, so it does not have a well-defined surface. When we speak of the surface of the Sun, we normally mean the photosphere.

  1. The photosphere is the lowest layer of the Sun’s three main atmospheric layers. It is the layer from which the Sun’s visible light emanates. Just above the photosphere lies the chromosphere.
  2. The Chromosphere is the layer of the Sun lying just above the photosphere. It is less than 20,000 km thick and separates the photosphere, at about 6000 degrees K, from the much hotter corona, at temperatures in the millions of degrees Kelvin.
  3. The Corona is the Sun’s faint (and hot) outer atmosphere, extending from  about 20,000 km above the photosphere to at least several solar radii, although its boundary is not defined. The temperature of the corona is about 1.5 million Kelvin.

Source: Alexander, P. EOS, Bull. Amer. Geophys. U. 73, 433, 1992.

Golub, L. and Pasachoff, J. M. The Solar Corona. Cambridge, England: Cambridge University Press, 1997.

Stern, D. and Peredo, M. “The Sun’s Corona.” http://www-spof.gsfc.nasa.gov/Education/wcorona.html.

© 1996-2007 Eric W. Weisstein


The Photosphere:

SunThe photosphere is the visible surface of the Sun that we are most familiar with. Since the Sun is a ball of gas, this is not a solid surface but is actually a layer about 100 km thick (very, very, thin compared to the 700,000 km radius of the Sun). When we look at the center of the disk of the Sun we look straight in and see somewhat hotter and brighter regions. When we look at the limb, or edge, of the solar disk we see light that has taken a slanting path through this layer and we only see through the upper, cooler and dimmer regions. This explains the “limb darkening” that appears as a darkening of the solar disk near the limb.

A number of features can be observed in the photosphere with a simple telescope (along with a good filter to reduce the intensity of sunlight to safely observable levels). These features include the dark sunspots, the bright faculae, andgranules. We can also measure the flow of material in the photosphere using the Doppler effect. These measurements reveal additional features such assupergranules as well as large scale flows and a pattern of waves and oscillations.

The Sun rotates on its axis once in about 27 days. This rotation was first detected by observing the motion of sunspots in the photosphere. The Sun’s rotation axis is tilted by about 7.25 degrees from the axis of the Earth’s orbit so we see more of the Sun’s north pole in September of each year and more of its south pole in March.

Since the Sun is a ball of gas it does not have to rotate rigidly like the solid planets and moons do. In fact, the Sun’s equatorial regions rotate faster (taking about 24 days) than the polar regions (which rotate once in more than 30 days). The source of this “differential rotation” is an area of current research in solar astronomy.

Read and see more about the sun at http://solarscience.msfc.nasa.gov/surface.shtml

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