The heat can be lost in several forms, in an atmosphere it is lost by convection, conduction and radiation. Convection is the heating of the air, causing hot air to rise and cool air to fall, creating convection 'cells'. Conduction is, of course, heat loss through contact with another, colder object, such as when you hold a glass of iced water, you feel the cold as your hand conducts heat through to the glass and water. Finally radiation is direct energy given off as infra-red radiation.Commander McLane wrote:I would like to ask that as a question to the people who know more about physics than I do. Would it really? Lose a lot of heat rapidly into what exactly? How would heat dissipate in vacuum? Objects on earth cool because their heat dissipates into the surrounding medium, be it air, water, earth, whatever. But in a vacuum there is by definition no surrounding medium. So my gut tells me that a hot object would not lose a lot of heat rapidly, but stay hot for a long time. Or am I wrong here?Captain Hesperus wrote:As the metal disintegrates, it'd lose a lot of heat rapidly into the stellar environment...
This radiation is usually the method of heat loss in space, several satellites use radiation to vent excess electricity from fixed solar panels to prevent overloading their onboard batteries by passing excess current through resistors, heating them and allowing them to radiate off the heat.
http://www.qrg.northwestern.edu/project ... space.html
Captain Hesperus