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Table 9.2 Properties of the known low-mass planets: super-Earths and mini-Neptunes.
Mass (M E )
Density (g/cm 3 )
Radius (R E )
Period (days)
Age (Gy)
Temp (K)
4.8 ± 0.8 c
1.68 ± 0.09 a
0.854 a
1.2-2.3 a
10 + 4 . 5
3.2
CoRoT-7b
1300-1800
6.9 ± 1.5 d
1.58 ± 0.10 b
8.0 ± 1.2 e
5.7 ± 2.5 f
2.5 ± 1.5 g
7.42 ± 1.21 h
4.56 + 1 . 17
1.26
8.9 + 3 . 2
2.9
Kepler-10b i
1 . 416 0 . 033
0 . 036
0.837
> 9
1500-2150
7.87 ± 0.65 j
2.08 + 0 . 16
0.17 j
0.74 j,k
5 j,k
4.8 + 1 . 9
1.3
55 Cnc-e
1400-1950
8.63 ± 0.35 k
2.00 ± 0.14 k
6.55 ± 0.98 m
2.678 ± 0.13 m
1.58 m
3-10 m
1.9 + 0 . 6
0.5
GJ 1214b
400-550
2.27 ± 0.08 n
Kepler-11b l
4.3 + 2 . 3
2.0
3.1 + 0 . 33
0.18
1.97 ± 0.19
10.3
8 ± 2
650-950
13.5 + 4 . 8
2.4 + 2 . 0
Kepler-11c l
3.15 ± 0.3
13.03
8 ± 2
600-900
6.1
1.4
Kepler-11d l
6.1 + 3 . 1
1.7
0.83 + 0 . 85
0.37
3.43 ± 0.32
22.7
8 ± 2
500-750
8.4 + 2 . 5
0.50 + 0 . 38
Kepler-11e l
4.52 ± 0.43
32
8 ± 2
450-650
1.9
0.21
2.3 + 2 . 2
1.2
0.71 + 1 . 2
0.45
Kepler-11f l
2.61 ± 0.25
46.7
8 ± 2
400-600
Kepler-18b o
4.8 + 3 . 5
2.7
6.9 ± 3.4
2.00 ± 0.10
3.5
10 ± 2.3
900-1300
1.91 + 0 . 12
6.9 + 5 . 3
Kepler-20b p
8.7 ± 2.2
3.7
> 6
850-1200
0.21
2.6
References: a Leger et al . 2009, b Bruntt et al . 2010, c Queloz et al . 2009, d Hatzes et al . 2010, e Ferraz-Mello et al . 2011,
f Boisse et al . 2011,
g Pont et al . 2011, h Hatzes et al . 2011,
i Batalha et al . 2010,
j Demory et al . 2011, k Winn et al . 2011,
l Lissauer et al . 2011, m Charbonneau
et al . 2009, n Carter et al . 2011, o Cochran et al . 2011, p Gautier et al . 2012.
The temperature range is calculated by assuming the planet re-radiates from its entire surface with an albedo of 0 and 0.75. The error bars
for the density are calculated as ρ min =
4 π
3
dM
( R + dR ) 3
M
4 π
3
dM
( R dR ) 3 .
M
+
and ρ max =
40000
HP-26b
500 K < T eq < 700 K
700 K < T eq < 900 K
900 K < T eq < 1100 K
1100 K < T eq < 1300 K
1300 K < T eq < 1500 K
1500 K < T eq < 1700 K
1700 K < T eq < 2200 K
K18-c
K11e
30000
HP-11b
GJ 436b
U
K11d
K4-b
N
K11c
20000
K20c
GJ 1214b
K11f
K18-b
55 Cnc-e
K20-b
K11-b
10000
C7-b
8000
K10-b
Fig. 9.3 Mass and Radius data for all transiting
exoplanets with masses below 10 M E color coded
according to the equilibrium temperature. Earth (E),
Uranus (U) and Neptune (N) are shown for reference.
Reproduced with permission of Elsevier. (See Color
Plate 7).
E
6000
5000
0.4
0.7
1
2
3
5
7
10
20
Mass [M Earth ]
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