Answer:
<em>1</em><em>)</em><em> </em><em>P</em><em>late</em><em> </em><em>tectonic</em><em> </em><em>theory</em>
<em>2</em><em>)</em><em> </em><em>Lithospheric</em>
<em>3</em><em>)</em><em> </em><em>Plates</em>
<em>4</em><em>)</em><em> </em><em>Heat</em>
<em>5</em><em>)</em><em> </em><em>Less</em><em> </em><em>dense</em>
<em>6</em><em>)</em><em> </em><em>Conventional current</em>
<em>7</em><em>)</em><em> </em><em>Magma</em>
<em>8</em><em>)</em><em> </em><em>Ocean</em><em> </em><em>crust</em>
<em>9</em><em>)</em><em> </em><em>Slowly</em>
<em>10</em><em>)</em><em> </em><em>Drifting</em><em> </em><em>away</em><em> </em>
Answer: the part of the heating curve corresponds to showing how the temperature changes as a substance for a constant rate.
Explanation: Let me know if you need any details!
Answer:
Explanation:The main purpose of astronomical telescope is to make objects from outer space appear as bright, contrasty and large as possible. That defines its three main function: light gathering, resolution and magnification. These are the measure of its efficiency.
Answer:
F=G(m1m2)/Rsquare if radius is given
F=G(m1m2)/dsquare if distance is given
where,
f =gravitational force
G =gravitational constant
m1=mass of one object
m2=mass of another object
d=distance between two object from their center r=radius of earth/planet
Answer:
C. It helps scientists detect dark matter.
Explanation:
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