In this paper, we study the linear stability of the elliptic rhombus solutions, which are the Keplerian homographic solution with the rhombus central configurations in the classical planar four-body problems. Using ω-Maslov index theory and trace formula, we prove the linear instability of elliptic rhombus solutions if the shape parameter u and the eccentricity of the elliptic orbit e satisfy
(
u
,
e
)
∈
(
1
/
3
,
u
2
)
×
0
,
f
^
(
27
4
)
−
1
/
2
∪
(
u
2
,
1
/
u
2
)
×
0
,
1
∪
(
1
/
u
2
,
3
)
×
0
,
f
^
(
27
4
)
−
1
/
2
where u
2 ≈ 0.6633 and
f
^
(
27
4
)
−
1
/
2
≈
0.4454
. Motivated on numerical results of the linear stability to the elliptic Lagrangian solutions in Martínez et al (2006 J. Differ. Equ.
226 619–651), we further analytically prove the linear instability of elliptic rhombus solutions for
(
u
,
e
)
∈
(
1
/
3
,
3
)
×
0
,
1
.