For mass \( m_1 \), the force due to gravity is \( F_{g1} = m_1 \cdot g \). For mass \( m_2 \), the force due to gravity is \( F_{g2} = m_2 \cdot g \). Here, \( g \) is the acceleration due to gravity, which is approximately \( 9.8 \, \text{m/s}^2 \).
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