Skip to main content

Table 3 Model parameters of numerical simulation with Tinit of 130 K. Note that “—” means the corresponding event does not occur.

From: Thermal evolution of icy planetesimals in the solar nebula

Model

R [km]

tafterCAI [Myr]

tice [Myr]

tdehydration [Myr]

Tpeak [K]

10–00A

10

0.0

0.14–0.20

560

10–05A

10

0.5

0.71–0.82

340

10–10A

10

1.0

260

50–10A

50

1.0

1.3–1.5

2.3–3.3

930

50–15A

50

1.5

2.1–2.6

530

50–20A

50

2.0

3.4<

273

50–24A

50

2.4

240

100–10A

100

1.0

1.3–1.5

2.3–3.3

1050

100–15A

100

1.5

2.1–2.6

640

100–20A

100

2.0

3.4<

273

100–24A

100

2.4

250

500–10A

500

1.0

1.3–1.5

2.3–3.3

1070

500–15A

500

1.5

2.1–2.6

650

500–20A

500

2.0

3.4<

273

500–24A

500

2.4

250

1000–10A

1000

1.0

1.3–1.5

2.3–3.3

1070

1000–15A

1000

1.5

2.1–2.6

650

1000–20A

1000

2.0

3.4<

273

1000–24A

1000

2.4

250