Hawthorn vs South Melbourne 16-May-1953 Lineups

Saturday 16-May-1953

Final Round 4

Hawthorn Coach: Jack Hale

53 7.11

63 9.9

South Melbourne Coach: Laurie Nash

The team sheet

Who takes the field

Attacking this way

Home team

Hawthorn

Recorded positions

Positions recorded for this match.

Exact positions unavailableAvailable players are listed below.

Position unavailable 20

12 Alf Hughes — 2 Bernie Considine — 34 Bill Collins — 8 Clive Philp — 32 Ian Egerton — 9 Ian McCann — 31 Jack Douglas — 10 John Kennedy — 23 John McCashney — 3 John OMahoney — 6 Kevin Coghlan — 14 Len Crane — 20 Mack Atkins — 28 Maurie Considine — 7 Neil Pearson — 5 Pat Cash — 18 Peter Kanis — 27 Roy Simmonds — 1 Ted Fletcher — 29 Wally Nash —

Away team

South Melbourne

Recorded positions

Positions recorded for this match.

Exact positions unavailableAvailable players are listed below.

Position unavailable 20

19 Alan McPherson — 8 Bill Gunn — 39 Bill Nolan — 9 Bob Giles — 38 Bruce Murray — 34 Don Scott — 27 Eddie Lane — 3 Frank Brew — 28 Ian Gillett — 29 Jack Garrick — 11 Jim Dorgan — 20 Jim Taylor — 21 John Svenson — 26 Keith Browning — 16 Kevin Hilet — 6 Nick Gelavis — 23 Ron Clegg — 25 Ron Digney — 35 Roy Cullinan — 36 Stan Smith —

Quarter Scores

Team	1Q	2Q	3Q	4Q	Total
HAW	1.3	1.2	4.2	1.4	53
SMO	3.2	4.2	1.2	1.3	63

Match Leaders

Goals

Wally NashHAW

Behinds

Not available yet

SuperCoach

Not available yet

Tackles

Not available yet

Team Stats

HAWSMO

Scoring / Attack

7Goals9

0Behinds0

0Behinds Rushed0

How the match finished

South Melbourne beat Hawthorn by 10 points, 63–53.

South Melbourne took a 11-point lead into the last quarter. Hawthorn cut that back to 10 by the final siren, scoring 10 points to 9 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. Quarter comparisons are included only when all four quarters add up to the final score. Missing records are not counted as zero.

Understanding historical coverage