The two numbers that decide whether a rooflight saves energy
The U-value is measured in watts per square metre per kelvin, W/m2K, and it counts how much heat passes through one square metre of the finished unit for every degree of difference between the room and the outside air. Lower is better. A single-glazed Victorian rooflight sits somewhere near 5.0. A double-glazed unit from the 1990s runs 2.8 to 3.0. A current manufactured roof window is 1.0 to 1.4, and a triple-glazed one can reach 0.6 to 0.8.
The g-value, sometimes written as the solar factor, is a fraction between zero and one. It is the proportion of the solar energy striking the glass that ends up as heat in the room, counting both the radiation that passes straight through and the part absorbed by the glass and then re-radiated inwards. Clear double glazing is around 0.6 to 0.7. A solar control unit is 0.25 to 0.35.
The two numbers pull in opposite directions for part of the year. A low g-value keeps a loft room usable in July and gives up some free winter heat in exchange. A high g-value collects that winter heat and makes the same room unbearable by four in the afternoon in August. Which trade is correct depends on the orientation of the slope, the room underneath, and how much glass is going in, and that judgement is made at survey rather than on a website.