carbohydrate

UK: ˌkɑːbəʊˈhaɪdreɪt | US: ˌkɑːrboʊˈhaɪdreɪt

Definition
  1. n. A biological molecule consisting of carbon, hydrogen, and oxygen atoms, typically with a hydrogen-oxygen ratio of 2:1 (e.g., sugars, starches).

  2. n. (Nutrition) A macronutrient found in foods like grains, fruits, and vegetables, serving as a primary energy source.

Structure
carbo <carbon>hydrate <water>
Etymology

The term "carbohydrate" emerged in 19th-century chemistry, combining "carbo-" (from Latin carbo, meaning "coal" or "carbon") and "-hydrate" (from Greek hydor, "water"). Early chemists observed that these compounds (e.g., glucose) had a molecular formula resembling carbon ("carbo") combined with water ("hydrate"), e.g., C₆H₁₂O₆ = 6C + 6H₂O. Though modern chemistry reveals a more complex structure, the name reflects this historical observation.

Examples
  1. Whole grains are a rich source of complex carbohydrates.

  2. Athletes often consume carbohydrates before endurance events.

  3. Photosynthesis converts sunlight into carbohydrates in plants.

  4. A low-carbohydrate diet restricts foods like bread and pasta.

  5. Cellulose, a carbohydrate, provides structural support in plant cell walls.