What David Cone's 1988 Season Would Look Like in 2000

This page projects David Cone's production from the 1988 run environment into the 2000 one, so the two can be compared directly. His actual line was 2.22 ERA, 1.12 WHIP. Translated to 2000 conditions, that becomes 2.83 ERA, 1.25 WHIP. The translation rescales counting stats by the ratio of league run scoring between the two eras; it does not attempt to model park, travel or integration effects.

ERA (Earned Run Average):
Earned runs allowed per nine innings pitched: (ER × 9) ÷ IP. The primary measure of pitching effectiveness.
WHIP (Walks and Hits per Inning Pitched):
Baserunners allowed per inning: (BB + H) ÷ IP. Under 1.00 is elite.

Data updated

What would David Cone's 1988 season look like if he pitched in 2000 instead? Below, his real 1988 line sits beside a cross-era translation into 2000's run environment — and a live slider lets you drop that season into any year in MLB history.

David Cone — 1988 (real)

As actually pitched
2.22 ERA, 1.12 WHIP

Translated to 2000

Modeled estimate · 2000 run environment
2.83 ERA, 1.25 WHIP

Why the translated ERA is higher: 2000 was a higher-offense run environment than 1988 (league ERA 3.73 → 4.77).

What this translation does not account for

This is a model, not a prediction. It re-expresses only David Cone's rate stats against 2000's league run environment — and nothing else. It does not account for the depth of competition (integration, international talent, a vastly larger athlete pool), pitch velocity, modern pitch arsenals (sliders, splitters, sweepers), strength and conditioning, or in-game adjustments and advanced scouting.

So a higher translated line means 2000 was simply a higher-offense era — not a claim that David Cone would actually perform better against today's pitching.

Rate Stats: Real vs. Translated

These rate stats are re-expressed by holding David Cone's performance relative to his league constant and re-basing it on 2000's averages (the same idea behind OPS+/ERA+).

What David Cone's 1988 Season Would Look Like in 2000 — Rate Stats: Real vs. Translated
Stat1988 (real)2000 (modeled)
ERA 2.22 2.83
WHIP 1.12 1.25

Counting Stats (1988, as played)

What David Cone's 1988 Season Would Look Like in 2000 — Counting Stats (1988, as played)
Wins20
Losses3
Games35
Games Started28
Strikeouts213
Shutouts4
Complete Games8
Innings231.1

Why counting totals aren't translated: scaling a counting stat by the league environment ratio massively over-inflates era outliers — e.g. a 1920s slugger's home runs would balloon to absurd modern totals. So home runs, RBI, wins, strikeouts and the like are shown exactly as David Cone produced them.

Verdict

This is a model, not a prediction. In 2000, the highest-offense season of the steroid era — a run environment harder to pitch in than 1988's (league ERA 3.73 → 4.77) — one reasoned way to express David Cone's 1988 season is roughly a 2.83 ERA and 1.25 WHIP. That holds his dominance relative to his league constant and re-bases it on 2000's averages; it is not a claim that David Cone would actually post those numbers. His counting totals (20 W, 213 K) are shown exactly as he pitched them, because scaling counting stats across eras wildly inflates outliers.

Try Any Era — Live

Pick a player and slide across MLB history to re-translate their peak season into any season's run environment. Same model, recomputed instantly.

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David Cone in Other Eras

View David Cone's full profile → · Browse all era translations →

What David Cone's 1988 Season Would Look Like in 2000: Frequently Asked Questions

What would David Cone hit in the 2000?
Translated into the 2000 run environment, David Cone's line becomes 2.83 ERA, 1.25 WHIP.
What did David Cone actually do?
His real line was 2.22 ERA, 1.12 WHIP in 1988, compiled in the 1988 season.
How does the era translator work?
It rescales a player's counting statistics by the ratio of league-wide run scoring between the two eras, holding his playing time constant. It does not model park effects, travel, equipment or the integration of the leagues.