- Database
- Experimentalists
- Date
- 2015-01-01
- Provider
- IPAG
- Previous sample
- CO2 snow with 1.5% H2O ice
- Parent sample
- CO2 snow with 1.5% H2O ice
- Diameter
- 80.0 mm
- Sample changes
- CO2 sublimation: growth of top H2O layer. Surface area: 62+1.3−1.3%, thickness: 48+1.6−1.6µm, mean grain size: 279+30−43µm; 1µm frost: 5.72+0.95−1.52%
- Substrate material
- cooper
- Substrate comments
- cylindrical 80mm diameter, 60mm deep
- Comments
- sublimating CO2+H2O mixture deposited over martian analogue dust with an initial thickness of 55 mm decreasing with time
- Temperature
- 148.15 ± 0.5 K
- Type
- molecular gas
- Fluids
-
- CO2 100.0 %
- Fluid temperature
- 148.15 ± 0.5 K
- Fluid pressure
- 6.47 ± 0.03 mbar
- Source
- Halogen lamp
- Chronology
- before spectrum
- Family
- photons
- Type
- Vis photons
- Radiant flux
- 2250.0 ± 100.0 J.s-1.m-2
- Source
- Halogen lamp
- Chronology
- before spectrum
- Irradiation time
- 10.0 ± 0.25 min
- Comments
- the time is the total illumination time since start of experiment
- Radiant flux
- 2200.0 ± 100.0 J.s-1.m-2
- Radiant fluence
- 1320000.0 ± 93000.0 J.s-1.m-2
Particle
Radiance
Radiance
- Publications
- Number
- 3
- Arrangement
- heterogeneous H2O ice layer developing during sublimation on top of the CO2+H2O snow mixture deposited over a 5 mm thick flat layer of martian analogue dust
- Layers