North Melbourne vs Hawthorn 13-May-1933 Lineups

Saturday 13-May-1933

Final Round 3

North Melbourne Coach: Dick Taylor

75 10.15

67 10.7

Hawthorn Coach: Arthur Rademacher

The team sheet

Who takes the field

Attacking this way

Home team

North Melbourne

Recorded positions

Positions recorded for this match.

Exact positions unavailableAvailable players are listed below.

Position unavailable 19

2 Ben Whittam — 27 Bob Mathews — 20 Charlie Cameron — 14 Charlie Gaudion — 35 Dick Taylor — 23 Jack Haskett — 18 Jack Lynch — 12 Jack Smith — 3 Jack Wrout — 8 Jim Adamson — 2 Jim Bicknell — 1 John Lewis — 25 Johnny Edwards — 16 Les Allen — 13 Neville Huggins — 4 Selwyn Baker — 5 Syd Barker — 28 Ted Cusack — 26 Ted Llewellyn —

Away team

Hawthorn

Recorded positions

Positions recorded for this match.

Exact positions unavailableAvailable players are listed below.

Position unavailable 19

14 Alex Lee — 18 Bert Carey — 20 Bert Hyde — 12 Bert Mills — 47 Bob Hammond — 23 Bob Murdoch — 4 Clarrie Lonsdale — 31 Ernie Loveless — 28 Geoff Farrelly — 24 George Bennett — 21 Jack Ryan — 26 Jack Zander — 6 Keith Sharpley — 16 Leo Murphy — 2 Norm Collins — 29 Roy Rodda — 8 Stan Spinks — 9 Stuart Stewart — 19 Ted Pool —

Quarter Scores

Team	1Q	2Q	3Q	4Q	Total
NTH	1.5	2.6	4.2	3.2	75
HAW	2.1	3.0	2.2	3.4	67

Match Leaders

Goals

2 tied leaders

Jim BicknellNTH

Behinds

Not available yet

SuperCoach

Not available yet

Tackles

Not available yet

Team Stats

NTHHAW

Scoring / Attack

10Goals10

0Behinds0

3Behinds Rushed3

How the match finished

North Melbourne beat Hawthorn by 8 points, 75–67.

North Melbourne took a 10-point lead into the last quarter. Hawthorn cut that back to 8 by the final siren, scoring 22 points to 20 in the final term.

This match record does not include scoring sequence.

Match records and coverage

This summary uses the recorded scores; it cannot explain tactics or individual moments. Period comparisons are included only when all recorded periods add up to the final score. Missing records are not counted as zero.

Understanding historical coverage