In this task, you're given a question, along with three passages, 1, 2, and 3. Your job is to determine which passage can be used to answer the question by searching for further information using terms from the passage. Indicate your choice as 1, 2, or 3.

Question: Who finished second on the first season of the show that Simpson and his wife won? Passage 1:Beckett made his debut in county cricket for Cheshire against Staffordshire in the 1978 Minor Counties Championship. He made nine further Minor Counties Championship appearances for the county, the last of which came against Durham in 1979. It was in 1979 that Beckett was selected to play for Minor Counties North in the 1979 Benson & Hedges Cup, making a single List A appearance against Nottinghamshire. The following season he joined Lancashire, making his debut for the county in a List A match against Worcestershire in the 1980 Gillette Cup. He made six further List A appearances for Lancashire, the last of which came against Gloucestershire in the 1981 John Player League. In his seven List A matches for the county, he scored 77 runs at an average of 12.83, with a high score of 30. With the ball, he took 2 wickets at a bowling average of 18.00, with best figures of 2/23. He made no appearances in first-class cricket for Lancashire.
 Passage 2:On June 21, 2012, Simpson married Canadian figure skater Jamie Salé, whom he had "known for years from the Edmonton skating scene". They had been paired as partners in late 2009 for the first season of the CBC show Battle of the Blades, which they won. Simpson and Salé have one daughter, Samantha Rae Simpson, born on July 7, 2013. Through this marriage, Simpson is also a stepfather to Salé's son Jesse Pelletier (born September 30, 2007), from her first marriage to skating partner David Pelletier. He also has three children from a previous marriage, including son Dillon, who was drafted by the Edmonton Oilers in the 4th round of the 2011 NHL Entry Draft and is currently a defenseman for the Bakersfield Condors.
 Passage 3:HD 225218 is a quadruple star system in the northern constellation of Andromeda. The primary component, HD 225218 A, is a giant star with a stellar classification of B9III, an apparent magnitude of 6.16, and is a candidate Lambda Boötis star. It has a fainter, magnitude 9.65 companion, HD 225218 B, at an angular separation of 5.2″ along a position angle of 171°. The primary itself has been identified as a binary star system through interferometry, with the two components separated by 0.165″. The pair, HD 225218 Aa and Ab, orbit each other with a period of about 70 years and an eccentricity of 0.515. Component B is likewise a spectroscopic binary.
2