Publications
Articles
1. Podolak, M.,
and A. G. W. Cameron (1974). Models of the giant planets. Icarus 22, 123 -
148.
2. Podolak, M.,
and A. G. W. Cameron (1974). Possible formation of meteoric chondrules
and inclusions in the precollapse Jovian protoplanetary atmosphere. Icarus 23, 326 -
333.
3. Podolak, M.,
and A. G. W. Cameron (1975). Further investigations of Jupiter models. Icarus 25, 627 -
634.
4. Podolak, M.
(1976). Methane rich
models of Uranus. Icarus 27, 473 - 477.
5. Podolak, M.
(1977). The abundance of water and rock in Jupiter as derived from interior
models. Icarus 30, 155 - 162.
6. Podolak, M.,
and R. E. Danielson (1977). Axel dust on Saturn and Titan. Icarus 30, 479 -
492.
7. Podolak, M.
(1978). Models of
Saturn's interior: Evidence for phase separation. Icarus 33, 342 -
350.
8. Podolak, M.,
and L. P. Giver (1979). On inhomogeneous scattering models of Titan's atmosphere. Icarus 37, 361 -
376.
9. Bar-Nun, A., and M. Podolak
(1979). The
photochemistry of hydrocarbons in the atmosphere of Titan. Icarus 38, 115 -
122.
10. Podolak, M.,
and A. Bar-Nun (1979). A constraint on the distribution of Titan's atmospheric aerosols. Icarus 39, 272 -
276.
11. Podolak, M.,
N. Noy, and A. Bar-Nun (1979). Photochemical aerosols in
Titan's atmosphere. Icarus 40, 193 - 198.
12. Noy, N., A.
Bar-Nun, and M. Podolak (1979). Acetylene photopolymers in
Jupiter's stratosphere. Icarus 40, 199 - 204.
13.
Otterman, J., S. Ungar, Y. Kaufman, and M. Podolak (1980). Atmospheric effects
on radiometric imaging from satellites.
Remote Sensing of Environment 9, 115 - 129.
14. Otterman, J.,
Y. Kaufman, M. Podolak, and S. Ungar
(1980). Dependence of
the global irradiance on aerosol properties and surface reflectivity. Solar Energy 24, 279 - 286.
15. Podolak, M.,
and E. Podolak (1980). A numerical study of
aerosol growth in Titan's atmosphere.
Icarus 43, 74 - 83.
16. Noy, N., M. Podolak, and A. Bar-Nun (1981). Photochemistry of phosphine and Jupiter's great red spot. J. Geophys. Res.
86, 11985 - 11988.
17. Podolak, M.,
and R. Reynolds (1981). On the structure and composition of Uranus and Neptune. Icarus 46, 40 -
50.
18. Eviatar, A.,
and M. Podolak (1983). Titan's gas and plasma
torus. J. Geophys.
Res. 88, 833 - 840.
19. Podolak, M.,
A. Bar-Nun, N. Noy, and L. P. Giver (1984). Inhomogeneous models of Titan's aerosol
distribution. Icarus
57, 72 - 82.
20. Podolak, M.,
and R. Reynolds (1984). Consistency
tests of cosmogonic theories from models of Uranus and
Neptune. Icarus
57, 102 - 111.
21. Podolak, M.
(1984). Is the polarization data
consistent with constant flux models of Titan's atmosphere? Icarus 58, 325 -
330.
22. Bar-Nun, A., N. Noy,
and M. Podolak (1984). An upper limit to the
abundance of lightning-produced amino acids in the Jovian water clouds. Icarus 59, 162 -
168.
23. Podolak, M.
(1984). The rotation
of the Uranian system. Phil. Trans. Roy. Soc.
A 313, 141 - 146.
24. Eviatar, A.,
A. Bar-Nun, and M. Podolak (1985). Europan surface phenomena. Icarus 61, 185 - 191.
25. Herman, G., and M. Podolak
(1985). Numerical
simulation of comet nuclei. I. Water ice comets. Icarus 61, 252 -
266.
26. Podolak, M.,
and G. Herman (1985). Numerical
simulation of comet nuclei. II. The effect of the dust mantle. Icarus 61, 267 -
277.
27. Mekler, Y.,
and M. Podolak (1985). Estimation of cloud top
heights from satellite imagery.
Appl. Optics 24, 2419 - 2422.
28. Podolak, M.,
R. Young, and R. Reynolds (1985). The internal structures and relative rotation rates of Uranus and
Neptune. Icarus
62, 266 - 271.
29. Bar-Nun, A., and M. Podolak
(1985). The
contribution by thunderstorms to the abundance of CO, C2H2, and HCN on Jupiter. Icarus 64, 112 -
124.
30. Pollack, J. B., M. Podolak,
P. Bodenheimer, and B. Christofferson
(1986). Planetesimal dissolution in the
envelopes of the forming giant planets.
Icarus 67, 409 - 443.
31. Podolak, M.,
and R. T. Reynolds (1987). The rotation rate of Uranus, its internal structure and the process
of planetary accretion. Icarus 70, 31 - 36.
32. Prialnik, D.,
A. Bar-Nun, and M. Podolak (1987). Radiogenic heating of
comets by 26Al and implications for their time of formation. Astrophys. J. 319, 993 - 1002.
33. Podolak, M.,
J. B. Pollack, and R. T. Reynolds (1987).
The interaction of planetesimals
with protoplanetary atmospheres. Icarus 73, 163 -
179.
34. Podolak, M.,
and Bar-Nun, A. (1988). Moist convection
and the abundances of lightning produced CO, C2H2 and HCN on Jupiter. Icarus 75, 566 -
570.
35. Mekler, Y.,
and Podolak, M. (1989). Spectrophotometric observations of Comet Austin (1982g). Earth, Moon, and Planets 44, 39 - 46.
36. Podolak, M.,
Bunch, T. E., Cassen, P., Reynolds, R. T. and Chang,
S. (1990). Processing
of refractory meteorite inclusions (CAIs) in parent body atmospheres. Icarus 84, 254 -
260.
37. Mekler, Y.,
D. Prialnik, and M. Podolak
(1990). Evaporation
from a porous cometary nucleus. Astrophys. J. 356, 682 - 686.
38. Eviatar, A., Podolak, M., and Richardson, J. (1990). Molecular and atomic
hydrogen from Titan in the outer Kronian
magnetosphere. J. Geophys. Res. 95, 21,007 - 21,016.
39. Podolak, M.,
R. T. Reynolds, and R. Young (1990).
Post Voyager comparisons of the interiors of Uranus and Neptune. Geophys. Res. Let. 17, 1737 - 1740.
40. Bunch, T. E., P. Cassen,
M. Podolak, R. Reynolds, S. Chang, P. Schultz, D.
Brownlee, and J. Lissauer (1991). Are some chondrules
formed by impact processes? Observations and experiments. Icarus 91, 76 -
92.
41. Podolak, M.,
D. Prialnik, T. E. Bunch, P. Cassen,
and R. Reynolds (1993). Secondary processing of chondrules and
refractory inclusions (CAIs) by gasdynamic heating. Icarus 104, 97 -
109.
42. Prialnik, D.,
U. Egozi, A. Bar - Nun, M. Podolak,
and Y. Greenzweig (1993). On pore size and fracture in gas - laden
comet nuclei. Icarus
106, 499 - 507.
43. Mekler, Y.
and M. Podolak (1994). Formation of
amorphous ice in the protoplanetary nebula. Planet. and Space
Sci. 42, 865-870.
44. Podolak, M.,
A. Weizman, and M. Marley (1995). Comparative models of
Uranus and Neptune. Planet. and Space Sci. 43, 1517-1522.
45. Marley, M.S., P. Gomez, and M. Podolak (1995).
46. Prialnik, D.
and M. Podolak (1995). Radioactive heating of
porous icy bodies. Icarus 117, 420-430.
47. Weizman, A.,
D. Prialnik, and M. Podolak
(1996). Constraints of
the structure and composition of Mars from thermal evolution models. J. Geophys. Res.101, 2235-2245.
48. Podolak, M.
and D. Prialnik (1996). On the structure and
evolution of comet P/Wirtanen. Planet. and Sp. Sci., 44, 655-664.
49. Pollack, J. B., O. Hubickyj,
P. Bodenheimer, J. J. Lissauer,
M. Podolak, and Y. Greenzweig,
(1996). Formation of
the giant planets by concurrent solid and gas accretion. Icarus 124, 62-85.
50. Elperin, T.,
N. Kleeorin, M. Podolak,
and
51. Weizman, A.,
D. Prialnik, and M. Podolak
(1997). Phase transitions and melting in
Mars. J. Geophys. Res., 102, 9205-9209.
52. Shoshani, Y.,
E. Heifetz, D. Prialnik, and M. Podolak
(1997). A model for
the changing pore structure and dust grain size distribution in a porous comet. Icarus, 126,
342-350.
53. Podolak, M.,
and Y. Mekler (1997).
Dirty ice grains in the protoplanetary
nebula. Planet.
Space Sci., 45, 1401-1406.
54. Shoshany, Y.,
M. Podolak, D. Prialnik,
and B. Berkowitz (1999). A monte carlo model for the flow of dust in a porous comet
nucleus, Icarus, 137, 348-354.
55. Prialnik, D.
and M. Podolak (1999). Changes in the structure of
comet nuclei due to radioactive heating.
Space Sci. Rev., 90, 169-178.
56. Podolak, M.,
J. I. Podolak, and M. Marley (2000). Further investigation of
random models of Uranus and Neptune, Planet. and
Sp. Sci., 48, 143-151.
57. Weizman, A.,
D. J. Stevenson, D. Prialnik, and M. Podolak (2001). Modeling the volcanism on Mars, Icarus,
150, 195-205.
58. Shoshany, Y.,
D. Prialnik, and M. Podolak
(2002).
59. Podolak, M.,
Y. Mekler, and D. Prialnik
(2002). Is the D/H ratio in the comet
coma equal to the D/H ratio in the comet nucleus? Icarus,
160, 208-211.
60. Cohen, M., D. Prialnik,
and M. Podolak (2003). A quasi-3D model for the
evolution of shape and temperature distribution of comet nuclei-application to
Comet 46P/Wirtanen. New
Astronomy, 8, 179-189.
61. Podolak, M.
(2003). The
contribution of small grains to the opacity of protoplanetary
atmospheres. Icarus,
165, 428-437.
62. Podolak, M.
(2003). The origin of
the solar system. Nakladem Polskiej
Akademii Umiejetnosci, 8,
11-23.
63. Podolak, M.,
Y. Mekler, and D. Prialnik
(2004). Comment on "Is the D/H
Ratio in the Comet Coma Equal to the D/H Ratio in the Comet Nucleus?" by
M. Podolak, Y. Mekler, and
D. Prialnik – rebuttal. Icarus, 168, 221-222.
64. Podolak, M.
(2004). Dust opacity and the contraction
of protoplanetary amospheres. Revista Mexicana de Astronomia y Astrofisica (Serie de Conferencias),
22, 104-107.
65.
Podolak, M., and S. Zucker (2004). A note on the snowline in protostellar
accretion disks. Meteoritics and
Planet. Sci., 39, 1859-1868.
66. Beer, E. H., M. Podolak,
and D. Prialnik (2006). The contribution of icy
grains to the activity of comets. Part I. Grain lifetime and
distribution. Icarus,
180, 473-486.
67. Lecar, M., M.
Podolak, D. Sasselov, and
E. Chiang (2006). On
the location of the snow line in a protoplanetary
disk. Astrophys. J., 640,
1115-1118.
68. Helled, R.,
M. Podolak, and A. Kovetz
(2006). Planetesimal capture in the disk
instability model. Icarus, 185, 64-75.
69. Iaroslavitz,
E., and M. Podolak (2007). Atmospheric mass deposition
by captured planetesimals. Icarus, 187,
600-610.
70. Beer, E., D. Prialnik,
and M. Podolak (2008). The contribution of grains
to the activity of comets II. The brightness of the coma.
Icarus, 195, 340-347.
71. Helled, R.,
M. Podolak, and A. Kovetz
(2008). Grain
sedimentation in a giant gaseous protoplanet. Icarus, 195,
863-870.
72. Movshovitz,
N. and M. Podolak (2008). Grain opacity in protoplanetary atmospheres. Icarus, 194,
368-378.
73. Levi, A. and M. Podolak (2009). Corona-like atmospheric escape from KBO’s I. Gas dynamics. Icarus, 202, 681-693.
74. Levi, A. and M. Podolak (2009). Corona-like atmospheric escape from KBO’s II. The behavior of aerosols. Icarus to appear.
Chapters in Books
1. Podolak, M.
(1982). The origin of Uranus:
Compositional considerations. In Uranus and the Outer
Planets. Proceedings of the
IAU/RAS Colloquium #60 (G. Hunt, ed.)
2. Podolak, M.,
and R. T. Reynolds (1985). What have we
learned from modeling giant planet interiors?
In Protostars and Planets II (D. Black and M.
Matthews, eds.)
3. Podolak, M.,
W. B. Hubbard, and D. J. Stevenson (1991). Models of Uranus'
interior and magnetic field. In
Uranus (J. Bergstralh, D. Miner, and M. Matthews, eds.)
4. Podolak, M.,
W. B. Hubbard, and J. B. Pollack (1993). Gaseous accretion
and the formation of giant planets.
In Protostars and Planets III (G. Levy, J. I. Lunine, and M. Matthews, eds.)
5. Hubbard, W. B., M. Podolak,
and D. J. Stevenson (1994). The interior of Neptune.
In Neptune and Triton (D. Cruickshank, ed.)
6. Podolak, M.
and D. Prialnik (1996). 26Al and liquid water
environments in comets. In Comets
and the Origin of Life (P. Thomas, C. H. Chyba, and
C. P. McKay, eds.)
7. Podolak, M.
and W. B. Hubbard (1998). Ice in the outer planets.
In Ice in the Solar System (B. Schmitt, C. deBergh,
and C. Festou, eds.) Kluwer Academic Publishers,
8. Prialnik, D.
and M. Podolak (1999). Changes in the structure of
comet nuclei due to radioactive heating.
In Composition and Origin of Cometary
Materials (K. Altwegg, P. Ehrenfreund,
J. Geiss, and W. Huebner, eds.)
Kluwer Academic Publishers,
9. Podolak, M.,
and D. Prialnik (2000). Conditions for the
production of liquid water in comet nuclei. In Bioastronomy
’99: a New Era in Bioastronomy (G. A. Lemarchand, K. J. Meech, eds.)
10. Brosch, N.,
L. S. Schijvarg, M. Podolak,
and M. R. Rosenkrantz (2001). Meteor observations from
Israel. In: Proceedings of the Meteoroids 2001 Conference, 6 - 10 August
2001,
11. Podolak, M.
(2003). The snowline
in protostellar disks. In Scientific Frontiers in Research
on Extrasolar Planets. (D. Deming and S. Seager, eds.) ASP Conference
Series, vol. 294,
12. Prialnik, D.,
J. Benkhoff, and M. Podolak
(2005). Modeling the
structure and activity of comet nuclei.
In Comets II.
(M. C. Festou, H. U. Keller, and H. A. Weaver,
eds.),
13. Podolak, M.
and D. Prialnik (2006). The conditions for liquid
water in cometary nuclei. In Comets and the Origin and Evolution of
Life (P. J. Thomas, R. D. Hicks, C. F. Chyba, and C.
P. McKay, eds.) Springer
14. Movshovitz, N. and M. Podolak (2008). Collisions between small dust particles reduce the formation time of giant planets. In Extreme Solar Systems (D. Fischer, F. A. Rasio, S. E. Thorsett, and A. Wolszczan, eds.) Am. Astron. Soc. Pacific, San Francisco, pp. 257-258.