| Felipe Massa | Graham Hill | |
|---|---|---|
| Career | ||
| Championships | — | 2 |
| Career span | 2002–2017 | 1958–1975 |
| Seasons | 15 | 18 |
| Race starts | 269 | 176 |
| Teams | Sauber, Ferrari, Williams | Lotus, BRM, Brabham, Shadow, Lola |
| Wins & podiums era-dependent · not directly comparable across eras | ||
| Wins | 11 | 14 |
| Podiums | 41 | 36 |
| Poles | 16 | 13 |
| Fastest laps | 15 | 10 |
| Era-fair rates career rate · across all seasons | ||
| Win % | 4.1% | 8.0% |
| Podium % | 15.2% | 20.5% |
| Pole % | 5.9% | 7.4% |
| Reliability & consistency era-dependent · see explanation | ||
| DNF rate | 14.1% | 42.0% |
| Points-finish rate | 61.3% | 33.5% |
| Points scoring-era variable · not directly comparable | ||
| Career total | 1167 | 289 |
The share of race starts that ended without a classified finish. Formula: races not finished ÷ race starts × 100. Races the driver did not start are excluded from both sides. A disqualification counts as a finish that scored nothing, not a DNF. Why it sits apart from the era-fair rates: unlike a win or a podium, finishing meant something very different in different eras. Cars in the 1950s–70s broke constantly; modern cars almost always reach the flag. A high DNF rate in 1955 says far more about the machinery than the driver. Comparing two drivers within the same season is meaningful — they faced the same conditions. Across eras it's context, not a verdict.
The share of race starts that ended in a points-paying position. Formula: races finished in a scoring position ÷ race starts × 100, using that season's real points system. Why it's era-dependent: the number of positions that pay points has changed repeatedly — the top five scored in 1950, the top ten score today. A modern driver has roughly twice as many scoring positions available for the same relative performance, so a higher percentage doesn't necessarily mean a better driver. Like DNF rate, it's shown as context.