Answer:
 T= 6.78 10⁷ s
Step-by-step explanation:
One way to accomplish this problem is to use Kepler's third law, which relates the order of the planets to their orbital distance. 
 T² = (4π² / G 
 ) a³
) a³ 
Where T and a are the period and orbital radius, respectively 
 
Let's start by writing the data for Earth and the new planet 
 
 
 ² = (4π² / G
² = (4π² / G 
 ) ae³
) ae³ 
 T² = (4pi2 / G 
 ) a³
) a³ 
Let's solve with these equations 
 T² / 
 ²2 = a³ /
²2 = a³ / 
 ³
³ 
 T² = 
 ² (a /
² (a / 
 )³
)³
The land period is 1 year 
 Te = 1 year (365 days / 1 year) (24h / 1 day) (3600s / 1h) 
 Te = 3.15 10⁷ s 
 
Let's calculate 
 T² = (3.15 107)² (2.5 1011 / 1.5 1011) 3 
 T = RA 45.94 10¹⁴ s
 T= 6.78 10⁷ s