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Showing posts with label 2009. Show all posts
Showing posts with label 2009. Show all posts

Tuesday, January 5, 2010

X-Rays day

 

X-radiation (composed of X-rays) is a form of electromagnetic radiation. X-rays have a wavelength in the range of 10 to 0.01 nanometers, corresponding to frequencies in the range 3 × 1016 Hz to 3 × 1019 Hz and energies in the range 120 eV to 120 keV. They are shorter in wavelength than UV rays. In many languages, X-radiation is called Röntgen radiation after Wilhelm Conrad Röntgen, who is generally credited as their discoverer, and who had called them X-rays to signify an unknown type of radiation.
Wilhelm Conrad Röntgen is usually credited as the discoverer of X-rays because he was the first to systematically study them, though he is not the first to have observed their effects. He is also the one who gave them the name "X-rays", though many referred to these as "Röntgen rays" for several decades after their discovery.
X-rays were found emanating from Crookes tubes, experimental discharge tubes invented around 1875, by scientists investigating the cathode rays, that is energetic electron beams, that were first created in the tubes. Crookes tubes created electrons by ionization of the residual air in the tube by a high DC voltage of anywhere between a few kilovolts and 100 kV. This voltage accelerated the electrons coming from the cathode to a high enough velocity that they created X-rays when they struck the anode or the glass wall of the tube. Many of the early Crookes tubes undoubtedly radiated X-rays, because early researchers noticed effects that were attributable to them, as detailed below. Wilhelm Röntgen was the first to systematically study them, in 1895.
 
font: wikipedia (click to see full article)
Versão Portuguesa: Raios X
Versión Española:  Rayos X

Friday, December 18, 2009

Sir David Attenborough: The Truth About Climate Change

Wednesday, December 16, 2009

Wednesday, October 7, 2009

The Nobel Prize in Chemistry 2009

The Nobel Prize in Chemistry 2009
"for studies of the structure and function
of the ribosome"


Venkatraman Ramakrishnan (United Kingdom) - MRC Laboratory of Molecular Biology Cambridge, United Kingdom - b. 1952(in Chidambaram, Tamil Nadu, India)
Thomas A. Steitz (USA) - Yale University New Haven, CT, USA; Howard Hughes Medical Institute - b. 1940

Ada E. Yonath (Israel) - Weizmann Institute of Science Rehovot, Israel - b. 1939

Titles, data and places given above refer to the time of the award.

in nobelprize.com

Tuesday, October 6, 2009

Nobel Prize in Physics 2009

O Prémio Nobel da Física 2009

"para realizações inovadoras relacionadas com a transmissão da luz em fibras ópticas de comunicação"
"pela invenção do circuito semicondutos de imagem – o sensor CCD"
Charles K. KaoWillard S. BoyleGeorge E. Smith
Photo: Richard Epworth
Charles K. KaoWillard S. BoyleGeorge E. Smith
half 1/2 of the prizequarter 1/4 of the prizequarter 1/4 of the prize
Standard Telecommunication Laboratories
Harlow, United Kingdom; Chinese University of Hong Kong
Hong Kong, China
Bell Laboratories
Murray Hill, NJ, USA
Bell Laboratories
Murray Hill, NJ, USA
b. 1933
(in Shanghai, China)
b. 1924
(in Amherst, NS, Canada)
b. 1930
in nobelprize.com

Wednesday, September 30, 2009

LED bulbs

The new products use Panasonic's own heat dissipation technology to increase the bulb's energy-efficiency. Generally speaking, LED's luminous efficiency increases as temperature decreases. So it is important to lower and optimize the temperature of an LED package to achieve higher luminous efficiency. By applying alumite treatment to the surface, Panasonic successfully increased heat dissipation to lower the temperate of the LED package. Combining this technology with the design which tightly joins the LED package and the casing, the company has achieved the industry's highest energy efficiency in LED bulbs1).

Also, when used as a downlight, the 6.9 W standard type LED bulbs deliver the brightness equivalent to 60 W incandescent bulbs5). That means it can save up to 2,000 yen per year on energy bills. The 4.0 W standard and 5.5 W compact LED bulbs produce the output comparable to 40 W incandescents and the 7.6 W standard LED bulbs have the brightness of 60 W incandescents when used as a downlight6).

Panasonic also made the new LED bulbs the lightest2) in the industry by making the casing thinner and reducing the amount of aluminum used in the product. The standard size E26 base bulb weighs only 100 g and the compact size E17 base bulb weighs 50 g.

Further, Panasonic employed its own thermal analysis technology to optimize the heat dissipating configuration (heat sink) to create the most compact E26 base LED bulbs in terms of length and outer diameter. The new LED lamps, including the industry's first E17 base LED bulbs, will easily fit into existing fixtures with which other replacement bulbs did not physically match.

The E26 base LED bulbs have a long lifespan of up to 40,000 hours. That means they last for about 19 years when used for 5.5 hours a day. The E17 base LED bulbs have about 20,000 hour life span. The new LED bulbs also feature a durable glass globe using glass manufacturing technology Panasonic accumulated over the years. They emit virtually no UV or IR radiation. The 7.6 W standard type and the 5.5 W compact type LED bulbs are dimmable from 10 percent to 100 percent.

Notes:

1) The standard type LDA7D-A1 LED bulb, which produces the brightness equivalent to a 40 W incandescent lamp when used without fixtures, has luminous efficiency of 82.6 lm/W and standard type LDA4D-A1 LED bulb, which produces the brightness equivalent to a 30 W incandescent lamp when used without fixtures, has luminous efficiency of 85.0 lm/w, as of September 10, 2009.

2) As a standard type LED bulb, as of September 10, 2009.

3) In terms of length and outer diameter.

4) As a compact type LED bulb (E17 base) which produces the brightness equivalent to a 25 W mini-krypton when used without fixtures.

5) Direct lighting when used with the LB72630Z fixture by Panasonic Electric Works (PEW).

6) Direct lighting when used with PEW's LB72106 (4.0 W LED bulb), LB72630Z (7.6 W LED bulb) and LB74059 (5.5 W LED bulb) fixtures.


in Panasonic

Saturday, September 26, 2009

Moon has more water


"Using a NASA instrument housed on the Indian Chandrayyan-1 satellite, scientists have solved an Apollo-era mystery about water on the moon. The discovery could have profound implications for future human explorers on our nearest celestial neighbor."


image from astrobio.net (click in the link right up to see the full article and images).

Thursday, September 17, 2009

PhysicsCentral: Buzz Blog

PhysicsCentral: Buzz Blog

WASHINGTON — For the first time, physicists have photographed the structure of an atom down to its electrons.

The pictures, soon to be published in the journal Physical Review B, show the detailed images of a single carbon atom's electron cloud, taken by Ukrainian researchers at the Kharkov Institute for Physics and Technology in Kharkov, Ukraine.

Shared via AddThis

Tuesday, September 15, 2009

Fermi Problem - Classroom

 
Problema de Fermi:
“Supondo que não está numa grande sala de aula e o professor fecha a porta no início da aula, quanto tempo levará para que você e seus colegas esgotem o oxigénio?”

Você decide se os cálculos são razoáveis.
Vamos construir primeiro a nossa sala de aula. Terá 5 metros de largura e comprimento e 3 metros de altura. Na prática, as dimensões métricas de volume será:

5 metros por 5 metros por 3 metros = 75 metros cúbicos.

Um metro cúbico é 1 000 litros, então agora temos 75 000 litros de ar fresco.
O conteúdo de oxigénio do ar é de cerca de 21 por cento, e em cerca de 17,5 por cento deverá ser suficiente para sair correndo da sala gritando. Para passar de ar fresco e respirável para absolutamente sufocante, façamos a diferença entre ter 21 por cento dos 75 000 litros e 17,5 por cento dos 75 000 litros. Isso nos dá 2.625 litros de oxigénio de passagem.
O próximo passo será determinar quanto oxigénio é que um ser humano consome. Foi difícil encontrar uma fonte confiável, mas neste artigo sobre a instalação em 2006, de um novo sistema de criação de oxigénio na Estação Espacial Internacional, fornece uma pista:
Durante as operações normais, fornecerá 5 kg por dia; o suficiente para suportar seis membros da tripulação.

Assim, uma pessoa precisa de cerca de 900 g de oxigénio por dia, ou 0,9 kg. Mas quantos litros é? O oxigénio tem uma massa molar de 16 gramas, assim o gás oxigénio, ou O2, tem uma massa de 32 gramas por mole. Um mol de gás à pressão normal e temperatura ocupa 22,4 litros. Ou seja:

0,9 kg x (1000 g / 1 kg) x (1 mol O2 / 32 g O2) x (22,4 L / 1 O2 mole)

Isso dá um consumo de oxigénio de 630 litros diários por pessoa. Vamos começar numa taxa mais razoável:

(630 L / dia) x (1 dia / 24 horas) x (1 hora / 60 mins)

Agora, temos a taxa de consumo de oxigénio utilizável de 0,4375 litros por minuto. Estamos quase lá.

A seguir preenchemos a sala de aula com 34 alunos e 1 professor. Os 35 ocupantes consomem 15,3125 litros por minuto. Assim, para o cálculo final:

2625 L x (1 minuto / 15,3125 L)

O que levará cerca de 171 minutos, ou 2 horas e 51 minutos para a sala tornar-se insuportavelmente sufocante. Pode verificar que começará a sentir-se muito desconfortável cerca de uma hora e meia de duração da palestra, um bom argumento para as aulas serem mais curtas.
traduzido de:

Friday, August 7, 2009

Physics Buzz: How to Build a Spectrometer with Just Three Household Items

A PhysicsBuzz article show us how to build a spectrometer with simple stuff that we have at home!



"A CD has the very cool property of behaving like a reflective
diffraction grating. An ordinary diffraction grating is a grid of tiny,
evenly spaced opaque lines on an otherwise transparent material. Light can pass through the material but it has to bend around the lines, which are about the size of a wavelength of visible light." in PhysicsBuzz

----[Versão Portuguesa]----
Um artigo do PhysicsBuzz mostra como construir um espectrómetro com coisas simples que temos em casa!

"O CD tem a propiedade de comportar-se como uma rede de difracção por reflexão. Uma rede de difracção é como uma rede de pequenas linhas opacas, espaçadas uniformemente num material transparente. A luz pode passar através do material, mas tem que dobrar em redor das linhas, que são aproximadamente do tamanho de um comprimento de onda de a luz visível". in PhysicsBuzz
Para saber mais sobre como construir este espectrómetro, segue o endereço indicado.


---[Versión Española/Castelhana]----
Un artículo de PhysicsBuzz nos muestra cómo construir un espectrómetro con cosas simples que tenemos en casa!



"Un CD tiene la propiedad de comportarse como una red de difracción por reflexión. Una rejilla de difracción es como una red de pequeñas líneas opacas, espaciadas uniformemente, en un material transparente. La luz puede pasar a través del material, pero tiene que doblar en torno a las líneas, que son aproximadamente del tamaño de una longitud de onda de la luz visible". in PhysicsBuzz

Si quieres saber cómo construir, siga el enlace.

Friday, May 29, 2009

Featured Post

IBSE about Light Pollution

Here is my presentation that happened in the Discover the Cosmos Conference (Volos, Greece - 2013). The presentation was an Inquiry Base...

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