Kenya national football team

The Kenya national football team represents Kenya in international football. It is controlled by the Football Kenya Federation, the governing body of football in Kenya, and competes as a member of the Confederation of African Football (CAF) and the Council for East and Central Africa Football Associations (CECAFA), a sub-confederation of CAF that has jurisdiction in East and Central Africa. The team is colloquially known as the Harambee Stars and plays its home games primarily at the Nyayo National Stadium in the country's capital, Nairobi. The team has never qualified for a FIFA World Cup finals.

History

Kenya has appeared in five Africa Cup of Nations tournaments, never reaching second round. The team entered its first FIFA World Cup qualification in 1974. As of 2010, they have not qualified for the final tournament.

2004 FIFA suspension

FIFA suspended Kenya from all football activities for three months in 2004, due to the interference of the government in football activities. The ban was reversed after the country agreed to create new statutes.

NTV (Kenya)

NTV came into being on May 12, 2005. A new face from the previous Nation TV station under the Nation Media Group arm that has been in existence since 1999.

It is a popular TV Station in Kenya along with Kenya Television Network, Kenya Broadcasting Corporation among others.

Youtube

In September 2007, NTV went online with its content on YouTube. Within the first month it received over 325,000 views, three honors, and an average of 4,000 views for every video uploaded. In mid-2012, NTV went live on YouTube. Following this move, the blogosphere was awash with accolades with NTV's US correspondent (BMJ) Ben Mutua Jonathan Muriithi terming it a techno-revolution for mass media among Kenyans across the globe.

Programming

Ali Mandhry hosts a cooking show on NTV Kenya, Tamu Tamu: Kenyan Cuisine with a Twist the first Kenyan cookery show on an outdoor setup showcasing the beautiful Cultures.

List of programs broadcast by NTV (Kenya)

References

Sierra Leone

Coordinates: 8°30′N 11°30′W / 8.500°N 11.500°W / 8.500; -11.500

Sierra Leone (ⁱ/sɪˈɛərə lɪˈoʊni, -lɪˈoʊn/), officially the Republic of Sierra Leone, is a country in West Africa. It is bordered by Guinea on the north, Liberia in the south-east, and the Atlantic Ocean in the south-west. Sierra Leone has a tropical climate, with a diverse environment ranging from savannah to rainforests. Sierra Leone has a total area of 71,740 km² (27,699 sq mi) and an estimated population of 6 million (2011 United Nations estimate).Freetown is the capital, largest city, and its economic and political centre. Bo is the second largest city. The other major cities in the country with a population above 100,000 are Kenema, Makeni and Koidu Town. Sierra Leone is divided into four geographical regions: the Northern Province, Eastern Province, Southern Province and the Western Area, which are further divided into fourteen districts.

About sixteen ethnic groups inhabit Sierra Leone, each with their own language and customs. The two largest and most influential are the Temne and the Mende people. The Temne are predominantly found in the north of the country, while the Mende are predominant in the south-east. Although English is the official language spoken at schools and government administration, the Krio language is the most widely spoken language in the country and unites all the different ethnic groups in the country, especially in their trade and social interaction with each other.

Double tap

A double tap is a shooting technique where two shots are fired in rapid succession at the same target with the same sight picture (different from the controlled pair, where a second sight picture is acquired for the second shot). Instruction and practice of the double-tap improves overall accuracy as shooters often do not have the gun fully extended on the first shot meaning the second of a double-tap is usually the better. The term hammer is sometimes used to describe a double tap in which the firearm's sights are not reacquired by the shooter between shots.

History

The origin of the double tap technique is credited to William Ewart Fairbairn and Eric A. Sykes, British police chiefs working in Shanghai during the 1930s who developed the technique in order to overcome the limitations of full metal jacketed (FMJ) ammunition. FMJ ammunition is commonly used by militaries for feeding reliability, adherence to the Hague Convention regarding non-expanding ammunition, and improved penetration. FMJ rounds can fail to cause sufficient damage, requiring more hits and better shot placement. In Ian Dear’s book Sabotage and Subversion about British Special Operations Executive (SOE) and United States Office of Strategic Services (OSS) forces, Fairbairn is reported to have instructed SOE personnel in the double tap from 1944 to 1945 at the SOE training school directed by Fairbairn and Sykes near Arisaig in Scotland. The term "double tap" is now used to describe the broader technique of firing two rounds quickly and accurately to disable an opponent. The tactic is still used today by firearms handlers, police tactical teams, military personnel, counter-terrorist combat units, and other Special Operations Forces personnel.

Star

A star is a luminous sphere of plasma held together by its own gravity. The nearest star to Earth is the Sun. Other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, and the brightest stars gained proper names. Extensive catalogues of stars have been assembled by astronomers, which provide standardized star designations.

For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Once the hydrogen in the core of a star is nearly exhausted, almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime and, for some stars, by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, luminosity, and spectrum respectively. The total mass of a star is the principal determinant of its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities, known as a Hertzsprung–Russell diagram (H–R diagram), allows the age and evolutionary state of a star to be determined.