Bricks that are made of clay and laid in the sun for drying. Most commericial bricks are formed in a mold and baked in an oven.
That's exactly what they called it. Sun-Baked Bricks. I have that word in my vocabulary list, and I don't think there is a specific name for it
in the unesco building in paris
In the Kunstmuseum, Basle, Switzerland.
a canon
These phenomena, which are all related to the Sun's magnetic field, impact our near-Earth space environment and determine our "space weather" In the near future, the same as now.
Probable not.
What will happen in the future is that the sun will become a red giant and eventually explode.
The sun has been shining for about 4.6 billion years and is currently in the middle of its main-sequence phase, during which it fuses hydrogen into helium in its core. In about 5 billion years, it will exhaust its hydrogen fuel and start to expand into a red giant, eventually shedding its outer layers to form a planetary nebula. It will then cool and shrink into a white dwarf, eventually fading into a black dwarf over trillions of years.
The most probable outcome is that there would be a HUGE Ice Age. yet that will not happen
depends what space does in the future
The future tense of "shine" is "will shine." For example, "The sun will shine tomorrow."
no one ,,,went to the sun ,,, and i guranteed that in future also ,,no one can go ,,bcoz of high temperature of the sun
January, i wish you good luck on all your future endeavors :)
Sun Tsu wrote it, around 500BC. This is Chinese History, by the way, not European History
Possibly in the future!
The Wikipedia lists the mass as (1.98855±0.00025)E30 kilograms. The plus-minus, of course, refers to the probable error in the Sun's mass, as currently known. That means this mass is currently known with a probable error of about 0.01%.It is also necessary to realize that the mass of the sun is slowly but continuously decreasing. due mostly to the conversion of mass to energy in fusion (4.29E9 kilograms/second) but also the solar wind (~1E9 kilograms/second). Admittedly this mass loss is so small compared to the probable error in the total mass that it is usually ignored, but still it makes knowledge of "exact mass of the Sun" impossible.