V Valentino is a racing driver who last raced in PCA Club Racing. Valentino has recorded 0 wins and 0 podiums from 1 start.[1]
A Racer Rating of 915 ranks Valentino 32567th of 40,200 indexed drivers, on an Elo scale where the strongest reach the high 8,000s. It is built from every indexed race in the driver's file, decayed for time since their last race.
| 2010-05-30 | Watkins Glen International SP2 | DNF | β85 |
| Season | Series | Team | Races | Wins | Podiums | DNFs | Poles | Points | Pos | Gain/Loss | Rating |
|---|---|---|---|---|---|---|---|---|---|---|---|
| 2010 | βΈPCA Club Racing | 1 | 0 | 0 | 1 | 0 | 0 | P37 | β435 | 915 |
| # | Driver | Series | Rating |
|---|---|---|---|
| 32,557 | π³οΈ Robert Finlayson | NASA | 915 |
| 32,558 | π³οΈ Rodger Grantham | SCCA Majors | 915 |
| 32,559 | πΊπΈ Ronald Dale | NASA | 915 |
| 32,560 | π³οΈ Ryan Shand | NASA | 915 |
| 32,561 | π³οΈ S. Brown | PCA Club Racing | 915 |
| 32,562 | π³οΈ S. Virden | PCA Club Racing | 915 |
| 32,563 | π³οΈ Scott McDaniel | SVRA | 915 |
| 32,564 | π³οΈ Steve Henkle | SCCA Majors | 915 |
| 32,565 | π³οΈ Steve Kamisky | NASA | 915 |
| 32,566 | πΊπΈ T & T Holmes | PCA Club Racing | 915 |
| 32,567 | π³οΈ V Valentino | PCA Club Racing | 915 |
| 32,568 | π³οΈ Alanzo Taylor | NASA | 914 |
| 32,569 | π³οΈ Anita Weemaes | SVRA | 914 |
| 32,570 | π³οΈ Barrett Schwarzlose | SVRA | 914 |
| 32,571 | π³οΈ Bobby L. Byrd | NASA | 914 |
| 32,572 | π³οΈ Bruce Trenery | NASA | 914 |
| 32,573 | π³οΈ Bryan Clymer | NASA | 914 |
| 32,574 | π³οΈ Christopher Mosley | SCCA Regionals | 914 |
| 32,575 | π³οΈ Cliff Murray | SVRA | 914 |
| 32,576 | π³οΈ Cohn Fabney | NASA | 914 |
| 32,577 | π³οΈ D. Hill | NASA | 914 |
V Valentino is a racing driver who last raced in PCA Club Racing. Valentino has recorded 0 wins and 0 podiums from 1 start.[1]
A Racer Rating of 915 ranks Valentino 32567th of 40,200 indexed drivers, on an Elo scale where the strongest reach the high 8,000s. It is built from every indexed race in the driver's file, decayed for time since their last race.