Compressed Natural Gas (CNG) is often recommended as a clean fuel for buses. CNG is composed mainly of methane and is considered a cleaner alternative to traditional fuels such as diesel or gasoline. When used in buses, CNG can significantly reduce emissions of pollutants such as carbon monoxide (CO), nitrogen oxides (NOx), and particulate matter.

The use of CNG in buses is part of efforts to reduce air pollution and promote environmentally friendly transportation options. CNG is a compressed form of natural gas, and its combustion produces fewer harmful pollutants compared to conventional fuels. It's important to note that the adoption of clean fuels like CNG may also involve modifying or using specially designed engines and fuel systems in vehicles to accommodate the specific properties of the fuel.

Charcoal does not produce flames because it is nearly pure carbon and lacks the volatile hydrocarbons found in materials like wood. When wood is burned, it goes through several stages, including the release of volatile compounds that can ignite and produce flames. However, charcoal is created through a process called pyrolysis, which involves heating wood in the absence of oxygen.

During pyrolysis, the volatile components of wood, such as water, tars, and gases, are driven off, leaving behind mostly carbon. Charcoal is essentially the carbon-rich residue of wood after these volatile components have been removed. Since charcoal lacks these volatile substances, it doesn't produce flames when ignited.

When you burn charcoal, you'll observe a red or orange glow, but this is due to the incandescence of the carbon particles, not the combustion of volatile gases. The absence of flames in charcoal fires makes it a popular choice for certain cooking methods, such as grilling or barbecuing, where a steady and consistent heat source is desired without the flare-ups associated with flames.

No, not all substances catch fire at the same temperature. The temperature at which a substance catches fire and sustains combustion is known as its ignition temperature or kindling point. The ignition temperature varies widely among different materials due to differences in their chemical composition and physical properties.

Some materials have low ignition temperatures and can catch fire easily, while others require higher temperatures to ignite. For example:

1. Flammable Liquids:

   • Substances like gasoline and alcohol have relatively low ignition temperatures, and they can catch fire easily at or near room temperature.

2. Flammable Solids:

   • Materials like paper, wood, and certain fabrics have ignition temperatures that are generally lower than those of non-flammable materials. They can catch fire at moderate temperatures.

3. Metals:

   • Metals, in general, have high ignition temperatures. They often require extremely high temperatures for combustion. Instead of catching fire, metals may melt or oxidize under certain conditions.

4. Non-Flammable Materials:

   • Some materials, such as rocks, glass, and certain ceramics, are non-flammable and do not have a distinct ignition temperature under normal conditions.

It's important to note that the ignition temperature is not the only factor influencing whether a substance will catch fire. Other factors, such as the presence of oxygen, the concentration of flammable gases or vapors, and the availability of an ignition source, also play crucial roles in determining flammability.

Understanding the flammability characteristics of materials is essential for fire safety and prevention. Fire codes and safety regulations often take into account the properties of different materials to ensure that appropriate precautions are in place to minimize the risk of fires.

The Sun's heat and light originate from nuclear fusion reactions that occur in its core. The primary process responsible for the Sun's energy production is the fusion of hydrogen nuclei into helium through a series of nuclear reactions known as the proton-proton chain. Here's a simplified explanation:

1. Nuclear Fusion:

   • In the Sun's core, where temperatures and pressures are extremely high, hydrogen nuclei (protons) collide and fuse to form helium nuclei. This process releases a tremendous amount of energy in the form of gamma-ray photons.

   • The primary fusion reaction in the Sun is the conversion of four hydrogen nuclei (protons) into one helium nucleus. This process involves several intermediate steps, with the release of positrons, neutrinos, and other particles.

2. Energy Transport:

   • The energy generated in the Sun's core is initially in the form of high-energy gamma-ray photons. However, these photons undergo a process known as radiative diffusion, gradually making their way from the core toward the Sun's surface.

   • As they move outward through the layers of the Sun, the energy undergoes a series of absorption and re-emission processes until it reaches the Sun's surface.

3. Sun's Surface (Photosphere):

   • Once the energy reaches the Sun's surface, it is primarily emitted as visible light. The Sun's surface, called the photosphere, is the layer from which most of the sunlight we see is emitted.

4. Heat and Light Emission:

   • The Sun's heat and light result from the continuous nuclear fusion reactions occurring in its core. The energy released during these reactions eventually reaches the surface and is radiated into space as sunlight.

In summary, the Sun's heat and light are produced through nuclear fusion reactions in its core, where hydrogen is converted into helium, releasing a tremendous amount of energy. This energy gradually makes its way to the Sun's surface and is emitted as light, including the visible light that reaches Earth.