Freddie Vasa is a racing driver who last raced in NASA for Mazda Miata. Vasa has recorded 0 wins and 0 podiums from 1 start.[1]
A Racer Rating of 890 ranks Vasa 33379th 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.
| 2015-03-15 | MSR Cresson Spec Miata | P22 | −110 |
| Season | Series | Team | Races | Wins | Podiums | DNFs | Poles | Points | Pos | Gain/Loss | Rating |
|---|---|---|---|---|---|---|---|---|---|---|---|
| 2015 | ▸NASA | Mazda Miata | 1 | 0 | 0 | 0 | 0 | 0 | P103 | −460 | 890 |
| # | Driver | Series | Rating |
|---|---|---|---|
| 33,369 | 🏳️ Shureed Kabir | Skip Barber | 891 |
| 33,370 | 🏳️ T Markut | PCA Club Racing | 891 |
| 33,371 | 🏳️ Thor Gjerdrum | NASA | 891 |
| 33,372 | 🏳️ Victor Avigliano | SVRA | 891 |
| 33,373 | 🏳️ Akhil Akula | SCCA Regionals | 890 |
| 33,374 | 🏳️ Bennett Sikes | SCCA Regionals | 890 |
| 33,375 | 🏳️ Bjarni Jonsson | SCCA Regionals | 890 |
| 33,376 | 🏳️ Daniel Foresi | NASA | 890 |
| 33,377 | 🏳️ Diamond Doug Anderson | NASA | 890 |
| 33,378 | 🏳️ Eric Hurd | NASA | 890 |
| 33,379 | 🏳️ Freddie Vasa | NASA | 890 |
| 33,380 | 🏳️ George Peterson | PCA Club Racing | 890 |
| 33,381 | 🏳️ Jake Fazeli | NASA | 890 |
| 33,382 | 🏳️ Jason VonKluge | NASA | 890 |
| 33,383 | 🏳️ Jay Bosko | NASA | 890 |
| 33,384 | 🏳️ Jeff Winter | SVRA | 890 |
| 33,385 | 🇦🇷 Joaquín Cortina | TC Pista Mouras | 890 |
| 33,386 | 🏳️ John Loiodice | BMW CCA Club Racing | 890 |
| 33,387 | 🏳️ Kevin A Violette | PCA Club Racing | 890 |
| 33,388 | 🏳️ Kurt Leta | PCA Club Racing | 890 |
| 33,389 | 🏳️ Kurt Rotman | SCCA Regionals | 890 |
Freddie Vasa is a racing driver who last raced in NASA for Mazda Miata. Vasa has recorded 0 wins and 0 podiums from 1 start.[1]
A Racer Rating of 890 ranks Vasa 33379th 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.