What is UV Index?

June 12th, 2011 by admin No comments »

The UV Index, developed by the National Weather Service and EPA, indicates the strength of solar UV radiation on a scale from 1 (low) to 11+ (extremely high). You can use the UV Index to take appropriate sun-protective behaviors and avoid overexposure to UV radiation.

UV Index forecast map

The forecast map shows contour lines of predicted UV Index values during the solar noon hour. The map is created daily from National Weather Service forecast data. Click the buttons for Day 2, Day 3, or Day 4 to see the UV Index forecast for following days. You may notice a brief delay as each map loads. (To find the time of solar noon at your location, use the sunrise-sunset-solar noon calculator at the NOAA Web site.)

 

UV Index forecast map

UV Index forecast map

About UV Index

The ozone layer shields the Earth from harmful ultraviolet (UV) radiation. Ozone depletion, as well as seasonal and weather variations, cause different amounts of UV radiation to reach the Earth at any given time. The UV Index, developed by the National Weather Service and EPA, indicates the strength of solar UV radiation on a scale from 1 (low) to 11+ (extremely high).

Every day the National Weather Service calculates the predicted UV Index for the next day in each area of the U.S. This UV Index forecast is published in mid-afternoon (Eastern time zone) at the EPA Web site. If the level of solar UV radiation is predicted to be unusually high, and consequently the risk of overexposure is greater than normal, the forecast includes a UV Alert. (You can sign up below to receive e-mail notification of UV Alerts for your community.)

 

 

What is an Atom?

May 20th, 2011 by admin No comments »

Atoms are the extremely small particles of which we, and everything around us, are made. There are 92 naturally occurring elements and scientists have made another 17, bringing the total to 109. Atoms are the smallest unit of an element that chemically behaves the same way the element does.

When two chemicals react with each other, the reaction takes place between individual atoms–at the atomic level. The processes that cause materials to be radioactive–to emit particles and energy–also occur at the atomic level.

Atomic Structure

In the early 20th century, a New Zealand scientist working in England, Ernest Rutherford, and a Danish scientist, Niels Bohr, developed a way of thinking about the structure of an atom that described an atom as looking very much like our solar system. At the center of every atom was a nucleus, which is comparable to the sun in our solar system. Electrons moved around the nucleus in “orbits” similar to the way planets move around the sun.(While scientists now know that atomic structure is more complex, the Rutherford-Bohr model is still a useful approximation to begin understanding about atomic structure.)

nucleus contains protons and neutrons; together these are called “nucleons”

neutrons have no electrical charge, and like protons, are about 1800 times as heavy as an electron.
protons are positively charged particles. All atoms of an element (radioactive and non-radioactive) have the same number of protons.Protons and neutrons in the nucleus, and the forces among them, affect an atom’s radioactive properties.

electrons The particles that orbit the nucleus as a cloud are called electrons. They are negatively charged and balance the positive electrical charge of the protons in the nucleus.

Interactions with electrons in the outer orbits affect an atom’s chemical propertie

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What holds the parts of an atom together?

Opposite electrical charges of the protons and electrons do the work of holding the electrons in orbit around the nucleus. Electrons closer to the nucleus are bound more tightly than the outer electrons because of their distance from the protons in the nucleus. The electrons in the outer orbits, or shells, are more loosely bound and affect an atom’s chemical properties.

The nucleus is held together by the attractive strong nuclear force between nucleons: proton-to-proton, neutron-neutron, and proton-neutron. It is extremely powerful, but extends only a very short distance, about the diameter of a proton or neutron.

There are also electromagnetic forces, which tend to shove the positively-charged protons (and as a result the entire nucleus) apart. In contrast to the strong nuclear force, the electric field of a proton falls off slowly over distance extending way beyond the nucleus, binding electrons to it.

The balance between the strong nuclear force pulling the nucleus together and the positive charges of the protons pushing it apart is largely responsible for the properties of a particular kind of atom or nuclide. (a unique combination of protons, neutrons, and balance of energies.)

The delicate balance of forces among nuclear particles keeps the nucleus stable. Any change in the number, the arrangement, or energy of the nucleons can upset this balance and cause the nucleus to become unstable or radioactive. (Disruption of electrons close to the nucleus can also cause an atom to emit radiation.)

The amount of energy required to break up the nucleus into its parts is called the binding energy; it is often referred to as “cosmic glue.”

What is Radiation?

May 17th, 2011 by admin No comments »

Radiation has a wide range of energies that form the electromagnetic spectrum (illustrated below). The spectrum has two major divisions:

  • non-ionizing radiation
  • ionizing radiation

Radiation that has enough energy to move around atoms in a molecule or cause them to vibrate, but not enough to remove electrons, is referred to as “non-ionizing radiation.” Examples of this kind of radiation are sound waves, visible light, and microwaves.

Radiation that falls within the “ionizing radiation” range has enough energy to remove tightly bound electrons from atoms, thus creating ions. This is the type of radiation that people usually think of as ‘radiation.’ We take advantage of its properties to generate electric power, to kill cancer cells, and in many manufacturing processes.

The energy of the radiation shown on the spectrum below increases from left to right as the frequency rises.

 

Types of Radiation in the Electromagnetic Spectrum

Types of Radiation in the Electromagnetic Spectrum

 

Nonionizing Radiation

We take advantage of the properties of non-ionizing radiation for common tasks:

  • microwave radiation– telecommunications and heating food
  • infrared radiation –infrared lamps to keep food warm in restaurants
  • radio waves– broadcasting

Non-ionizing radiation ranges from extremely low frequency radiation, shown on the far left through the audible, microwave, and visible portions of the spectrum into the ultraviolet range.

Extremely low-frequency radiation has very long wave lengths (on the order of a million meters or more) and frequencies in the range of 100 Hertz (cycles per second) or less. Radio frequencies have wave lengths of between one and 100 meters and frequencies in the range of one million to 100 million Hertz. Microwaves that we use to heat food have wavelengths that are about one hundredth of a meter and have frequencies of about 2.5 billion Hertz.

Ionizing Radiation

Higher frequency ultraviolet radiation begins to have enough energy to break chemical bonds. X-ray and gamma ray radiation, which are at the upper end of magnetic radiation, have very high frequencies (in the range of 100 billion billion Hertz) and very short wavelengths of about 1 picometer (1 trillionth of a meter). Radiation in this range has extremely high energy. It has enough energy to strip off electrons or, in the case of very high-energy radiation, break up the nucleus of atoms.

Ionization is the process in which a charged portion of a molecule (usually an electron) is given enough energy to break away from the atom. This process results in the formation of two charged particles or ions: the molecule with a net positive charge and the free electron with a negative charge.

Each ionization releases approximately 33 electron volts (eV) of energy. Material surrounding the atom absorbs the energy. Compared to other types of radiation that may be absorbed, ionizing radiation deposits a large amount of energy into a small area. In fact, the 33 eV from one ionization is more than enough energy to disrupt the chemical bond between two carbon atoms. All ionizing radiation is capable, directly or indirectly, of removing electrons from most molecules.

Addressing Toxics, Hazardous Materials, and Waste

May 2nd, 2011 by admin No comments »
Pile of e-Waste / Electronic waste: A few olde...

Improper management and disposal of toxic substances poses a threat to local and global environments. Once released into the environment, many of these substances can travel long distances and affect ecosystems and human populations far from the point of use or disposal. In addition, toxic chemicals can accumulate in the environment and pose long-term threats to human health. EPA works to reduce the use and release of toxics that can cause harm to humans and ecosystems, by providing technical assistance and capacity building to developing countries and by providing technical input into international negotiations for the sound management of toxic substances and wastes.

Mercury

Gold Shops — artisanal and small-scale gold buying and refining facilities in the developing world — process a significant percentage of the world’s annual gold production, and are a major cause of air pollution from mercury. EPA’s low-cost, easily constructible Mercury Control System technology is reducing the harmful health effects of mercury air pollution from gold refining, for communities in the Amazon and worldwide.

E-Waste

Increasing waste from electronics (known as “e-waste”) is a significant problem. Meeting this challenge will require more sustainable management of electronics throughout the product lifecycle — from the design and manufacturing of the product, to its use and eventual recycling and disposal. To address this problem, President Barack Obama has established a task force to develop a national strategy for responsible electronic stewardship.