Step 1: The Bohr model with a finite-mass nucleus depends on the reduced mass \(\mu = \dfrac{m_1 m_2}{m_1 + m_2}\). For hydrogen the proton is very heavy, so \(\mu_H \approx m_e\).
Step 2: Positronium is an electron bound to a positron, both of mass \(m_e\). Its reduced mass is
\[\mu_p = \frac{m_e \cdot m_e}{m_e + m_e} = \frac{m_e}{2}.\]
Step 3: The Bohr radius scales as \(r_n \propto \dfrac{1}{\mu}\). Since \(\mu_p = \tfrac{1}{2}\mu_H\), the positronium orbit is twice as large:
\[r_p = 2\,r_H.\]
Step 4: The binding energy scales as \(E_n \propto \mu\). Since \(\mu_p = \tfrac{1}{2}\mu_H\), the positronium energy is half that of hydrogen in magnitude:
\[E_p = \frac{E_H}{2}.\]
Step 5: Combining both results:
\[\boxed{r_p = 2r_H,\quad E_p = \frac{E_H}{2}}\]