F1 World Championship points standings after the 2022 Belgian GP
Updated F1 drivers' and constructors' world championship standings following the 2022 Belgian Grand Prix.
2022 FORMULA 1 DRIVERS' WORLD CHAMPIONSHIP | |||||
Pos | Driver | Nat. | Team | Wins | Points |
1 | Max Verstappen | NED | Oracle Red Bull Racing | 9 | 284 |
2 | Sergio Perez | MEX | Oracle Bull Racing | 1 | 191 |
3 | Charles Leclerc | MON | Scuderia Ferrari | 3 | 185 |
4 | Carlos Sainz | ESP | Scuderia Ferrari | 1 | 171 |
5 | George Russell | GBR | Mercedes AMG Petronas Formula One Team | 0 | 170 |
6 | Lewis Hamilton | GBR | Mercedes AMG Petronas Formula One Team | 0 | 146 |
7 | Lando Norris | GBR | McLaren F1 Team | 0 | 76 |
8 | Esteban Ocon | FRA | BWT Alpine F1 Team | 0 | 64 |
9 | Fernando Alonso | ESP | BWT Alpine F1 Team | 0 | 51 |
10 | Valtteri Bottas | FIN | Alfa Romeo F1 Team Orlen | 0 | 46 |
11 | Kevin Magnussen | DAN | Haas F1 Team | 0 | 22 |
12 | Sebastian Vettel | GER | Aston Martin Aramco Cognizant Formula One Team | 0 | 20 |
13 | Daniel Ricciardo | AUS | McLaren F1 Team | 0 | 19 |
14 | Pierre Gasly | FRA | Scuderia AlphaTauri | 0 | 18 |
15 | Mick Schumacher | GER | Haas F1 Team | 0 | 12 |
16 | Yuki Tsunoda | JPN | Scuderia AlphaTauri | 0 | 11 |
17 | Guanyu Zhou | CHN | Alfa Romeo F1 Team Orlen | 0 | 5 |
18 | Lance Stroll | CAN | Aston Martin Aramco Cognizant Formula One Team | 0 | 4 |
19 | Alexander Albon | THA | Williams Racing | 0 | 4 |
20 | Nico Hulkenberg | GER | Aston Martin Aramco Cognizant Formula One Team | 0 | 0 |
21 | Nicholas Latifi | CAN | Williams Racing | 0 | 0. |
2022 FORMULA 1 CONSTRUCTORS' WORLD CHAMPIONSHIP | |||
Pos | Team | Wins | Points |
1 | Oracle Red Bull Racing | 10 | 475 |
2 | Scuderia Ferrari | 4 | 357 |
3 | Mercedes AMG Petronas Formula One Team | 0 | 316 |
4 | BWT Alpine F1 Team | 0 | 115 |
5 | McLaren F1 Team | 0 | 95 |
6 | Alfa Romeo F1 Team Orlen | 0 | 51 |
7 | Haas F1 Team | 0 | 34 |
8 | Scuderia AlphaTauri | 0 | 29 |
9 | Aston Martin Aramco Cognizant Formula One Team | 0 | 24 |
10 | Williams Racing | 0 | 4 |