Attree, N., Jorda, L., Groussin, O., Mottola, S., Thomas, N., Brouet, Y., Kührt, E., Knapmeyer, M.,
Preusker, F., Scholten, F., Knollenberg, J., Hviid, S., Hartogh, P., & Rodrigo, R. (2019).
Constraining models of activity on comet 67P/Churyumov-Gerasimenko with Rosetta trajectory, rotation, and water production measurements. Astronomy and Astrophysics, 630, A18.
Auger, A.-T., et al. (2018). Meter-scale thermal contraction crack polygons on the nucleus of comet
67P/Churyumov-Gerasimenko. Icarus, 301, 173.
Avakyan, S. V., II’in, R. N., Lavrov, V. M., & Ogurtsov, G. N. (Eds.). (1998). Collision processes
and excitation of UV emission from planetary atmospheric gases: A handbook of cross sections.
Amsterdam: Gordon and Breach.
Bagnold, R. A. (1941). The physics of blown sand and desert dunes. New York: Methuen.
Baines, M. J., Williams, I. P., & Asebiomo, A. S. (1965). Resistance to the motion of a small sphere
moving through a gas. Monthly Notices of the Royal Astronomical Society, 130, 63.
Baker, V. R. (2001). Water and the martian landscape. Nature, 412, 228.
Balsiger, H., Altwegg, K., & Geiss, J. (1995). D/H and O-18/O-16 ratio in the hydronium ion and in
neutral water from in situ ion measurements in comet Halley. Journal of Geophysical Research,
100, 5827–5834.
Bardyn, A., Baklouti, D., Cottin, H., Fray, N., Briois, C., Paquette, J., Stenzel, O., Engrand, C.,
Fischer, H., Hornung, K., Isnard, R., Langevin, Y., Lehto, H., Le Roy, L., Ligier, N., Merouane,
S., Modica, P., Orthous-Daunay, F.-R., Rynö, J., Schulz, R., Silén, J., Thirkell, L., Varmuza, K.,
Zaprudin, B., Kissel, J., & Hilchenbach, M. (2017). Carbon-rich dust in comet 67P/ChuryumovGerasimenko measured by COSIMA/Rosetta. Monthly Notices of the Royal Astronomical
Society, 469, S712.
Baertschi, P. (1976). Absolute
18
O content of standard mean ocean water. Earth and Planetary
Science Letters, 31, 341.
Barucci, M. A., et al. (2016). Detection of exposed H 2 O ice on the nucleus of comet 67P/
Churyumov-Gerasimenko as observed by Rosetta OSIRIS and VIRTIS instruments. Astronomy
and Astrophysics, 595, A102.
Becker, K. H., & Haaks, D. (1973). Measurement of the natural lifetimes and quenching rate
constants of OH(2Σ+, v ¼ 0,1) and OD(2Σ+, v ¼ 0,i) Radicals. Zeitschrift Naturforschung,
Teil A, 28, 249–256.
Belton, M. J. S. (2015). The mass disruption of Jupiter Family comets. Icarus, 245, 8.
Belton, M. J. S., Wehinger, P., Wyckoff, S., & Spinrad, H. (1986). A precise spin period for
P/Halley. ESLAB Symposium on the Exploration of Halley’s Comet, 250, 599.
Belton, M. J. S., Julian, W. H., Anderson, A. J., & Mueller, B. E. A. (1991). The spin state and
homogeneity of comet Halley’s nucleus. Icarus, 93, 183.
Belton, M. J. S., et al. (2011). Stardust-NExT, Deep Impact, and the accelerating spin of 9P/Tempel
1. Icarus, 213, 345.
Belton, M. J. S., Thomas, P., Li, J.-Y., Williams, J., Carcich, B., A’Hearn, M. F., McLaughlin, S.,
Farnham, T., McFadden, L., Lisse, C. M., Collins, S., Besse, S., Klaasen, K., Sunshine, J.,
Meech, K. J., & Lindler, D. (2013). The complex spin state of 103P/Hartley 2: Kinematics and
orientation in space. Icarus, 222, 595.
Benkhoff, J., & Boice, D. C. (1996). Modeling the thermal properties and the gas flux from a
porous, ice-dust body in the orbit of P/Wirtanen. Planetary and Space Science, 44, 665–673.
Bensch, F., & Bergin, E. A. (2004). The pure rotational line emission of ortho-water vapor in
comets. I. Radiative transfer model. The Astrophysical Journal, 615, 531.
Bertini, I., et al. (2017). The scattering phase function of comet 67P/Churyumov-Gerasimenko
coma as seen from the Rosetta/OSIRIS instrument. Monthly Notices of the Royal Astronomical
Society, 469, S404.
Beutler, G. (2005). Methods of celestial mechanics: Vol. I. Physical, mathematical, and numerical
principles. In cooperation with Leos Mervart and Andreas Verdun. Astronomy and Astrophysics Library. Berlin: Springer. ISBN 3-540-40749-9.
Biele, J., Ulamec, S., Richter, L., Kührt, E., Knollenberg, J., Moehlmann, D., & Philae Team.
(2009). The strength of cometary surface material: Relevance of Deep Impact results for Philae
References
451
Preusker, F., Scholten, F., Knollenberg, J., Hviid, S., Hartogh, P., & Rodrigo, R. (2019).
Constraining models of activity on comet 67P/Churyumov-Gerasimenko with Rosetta trajectory, rotation, and water production measurements. Astronomy and Astrophysics, 630, A18.
Auger, A.-T., et al. (2018). Meter-scale thermal contraction crack polygons on the nucleus of comet
67P/Churyumov-Gerasimenko. Icarus, 301, 173.
Avakyan, S. V., II’in, R. N., Lavrov, V. M., & Ogurtsov, G. N. (Eds.). (1998). Collision processes
and excitation of UV emission from planetary atmospheric gases: A handbook of cross sections.
Amsterdam: Gordon and Breach.
Bagnold, R. A. (1941). The physics of blown sand and desert dunes. New York: Methuen.
Baines, M. J., Williams, I. P., & Asebiomo, A. S. (1965). Resistance to the motion of a small sphere
moving through a gas. Monthly Notices of the Royal Astronomical Society, 130, 63.
Baker, V. R. (2001). Water and the martian landscape. Nature, 412, 228.
Balsiger, H., Altwegg, K., & Geiss, J. (1995). D/H and O-18/O-16 ratio in the hydronium ion and in
neutral water from in situ ion measurements in comet Halley. Journal of Geophysical Research,
100, 5827–5834.
Bardyn, A., Baklouti, D., Cottin, H., Fray, N., Briois, C., Paquette, J., Stenzel, O., Engrand, C.,
Fischer, H., Hornung, K., Isnard, R., Langevin, Y., Lehto, H., Le Roy, L., Ligier, N., Merouane,
S., Modica, P., Orthous-Daunay, F.-R., Rynö, J., Schulz, R., Silén, J., Thirkell, L., Varmuza, K.,
Zaprudin, B., Kissel, J., & Hilchenbach, M. (2017). Carbon-rich dust in comet 67P/ChuryumovGerasimenko measured by COSIMA/Rosetta. Monthly Notices of the Royal Astronomical
Society, 469, S712.
Baertschi, P. (1976). Absolute
18
O content of standard mean ocean water. Earth and Planetary
Science Letters, 31, 341.
Barucci, M. A., et al. (2016). Detection of exposed H 2 O ice on the nucleus of comet 67P/
Churyumov-Gerasimenko as observed by Rosetta OSIRIS and VIRTIS instruments. Astronomy
and Astrophysics, 595, A102.
Becker, K. H., & Haaks, D. (1973). Measurement of the natural lifetimes and quenching rate
constants of OH(2Σ+, v ¼ 0,1) and OD(2Σ+, v ¼ 0,i) Radicals. Zeitschrift Naturforschung,
Teil A, 28, 249–256.
Belton, M. J. S. (2015). The mass disruption of Jupiter Family comets. Icarus, 245, 8.
Belton, M. J. S., Wehinger, P., Wyckoff, S., & Spinrad, H. (1986). A precise spin period for
P/Halley. ESLAB Symposium on the Exploration of Halley’s Comet, 250, 599.
Belton, M. J. S., Julian, W. H., Anderson, A. J., & Mueller, B. E. A. (1991). The spin state and
homogeneity of comet Halley’s nucleus. Icarus, 93, 183.
Belton, M. J. S., et al. (2011). Stardust-NExT, Deep Impact, and the accelerating spin of 9P/Tempel
1. Icarus, 213, 345.
Belton, M. J. S., Thomas, P., Li, J.-Y., Williams, J., Carcich, B., A’Hearn, M. F., McLaughlin, S.,
Farnham, T., McFadden, L., Lisse, C. M., Collins, S., Besse, S., Klaasen, K., Sunshine, J.,
Meech, K. J., & Lindler, D. (2013). The complex spin state of 103P/Hartley 2: Kinematics and
orientation in space. Icarus, 222, 595.
Benkhoff, J., & Boice, D. C. (1996). Modeling the thermal properties and the gas flux from a
porous, ice-dust body in the orbit of P/Wirtanen. Planetary and Space Science, 44, 665–673.
Bensch, F., & Bergin, E. A. (2004). The pure rotational line emission of ortho-water vapor in
comets. I. Radiative transfer model. The Astrophysical Journal, 615, 531.
Bertini, I., et al. (2017). The scattering phase function of comet 67P/Churyumov-Gerasimenko
coma as seen from the Rosetta/OSIRIS instrument. Monthly Notices of the Royal Astronomical
Society, 469, S404.
Beutler, G. (2005). Methods of celestial mechanics: Vol. I. Physical, mathematical, and numerical
principles. In cooperation with Leos Mervart and Andreas Verdun. Astronomy and Astrophysics Library. Berlin: Springer. ISBN 3-540-40749-9.
Biele, J., Ulamec, S., Richter, L., Kührt, E., Knollenberg, J., Moehlmann, D., & Philae Team.
(2009). The strength of cometary surface material: Relevance of Deep Impact results for Philae
References
451