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Items: 1 to 20 of 99

1.

Organics and other molecules in the surfaces of Callisto and Ganymede.

McCord TB, Carlson RW, Smythe WD, Hansen GB, Clark RN, Hibbitts CA, Fanale FP, Granahan JC, Segura M, Matson DL, Johnson TV, Martin PD.

Science. 1997 Oct 10;278(5336):271-5.

2.

Near-infrared spectroscopy and spectral mapping of Jupiter and the Galilean satellites: results from Galileo's initial orbit.

Carlson R, Smythe W, Baines K, Barbinis E, Becker K, Burns R, Calcutt S, Calvin W, Clark R, Danielson G, Davies A, Drossart P, Encrenaz T, Fanale F, Granahan J, Hansen G, Herrera P, Hibbitts C, Hui J, Irwin P, Johnson T, Kamp L, Kieffer H, Leader F, Weissman P, et al.

Science. 1996 Oct 18;274(5286):385-8.

PMID:
8832878
3.

The Galilean satellites.

Showman AP, Malhotra R.

Science. 1999 Oct 1;286(5437):77-84. Review.

PMID:
10506564
4.

Laboratory studies of the newly discovered infrared band at 4705.2 cm-1 (2.1253 micrometers) in the spectrum of Io: the tentative identification of CO2.

Sandford SA, Salama F, Allamandola LJ, Trafton LM, Lester DF, Ramseyer TF.

Icarus. 1991;91:125-44.

PMID:
11538104
5.

The 2.5-5.0 micrometers spectra of Io: evidence for H2S and H2O frozen in SO2.

Salama F, Allamandola LJ, Witteborn FC, Cruikshank DP, Sandford SA, Bregman JD.

Icarus. 1990 Jan;83(1):66-82.

PMID:
11538411
6.

Hydrated salt minerals on Ganymede's surface: evidence of an ocean below.

McCord TB, Hansen GB, Hibbitts CA.

Science. 2001 May 25;292(5521):1523-5.

7.
8.

Gravitational evidence for an undifferentiated Callisto.

Anderson JD, Lau EL, Sjogren WL, Schubert G, Moore WB.

Nature. 1997 May 15;387(6630):264-6.

PMID:
9153389
9.

A new class of absorption feature in Io's near-infrared spectrum.

Trafton LM, Lester DF, Ramseyer TF, Salama F, Sandford SA, Allamandola LJ.

Icarus. 1991;89:264-76.

PMID:
11538100
10.

New horizons mapping of Europa and Ganymede.

Grundy WM, Buratti BJ, Cheng AF, Emery JP, Lunsford A, McKinnon WB, Moore JM, Newman SF, Olkin CB, Reuter DC, Schenk PM, Spencer JR, Stern SA, Throop HB, Weaver HA; New Horizons Team.

Science. 2007 Oct 12;318(5848):234-7.

11.

Detection of a deep 3-microm absorption feature in the spectrum of Amalthea (JV).

Takato N, Bus SJ, Terada H, Pyo TS, Kobayashi N.

Science. 2004 Dec 24;306(5705):2224-7.

12.

Is H2O present on Io? The detection of a new strong band near 3590 cm-1 (2.79 micrometers).

Salama F, Allamandola LJ, Sandford SA, Bregman JD, Witteborn FC, Cruikshank DP.

Icarus. 1994;107:413-7.

PMID:
11539181
13.

Induced magnetic fields as evidence for subsurface oceans in Europa and Callisto.

Khurana KK, Kivelson MG, Stevenson DJ, Schubert G, Russell CT, Walker RJ, Polanskey C.

Nature. 1998 Oct 22;395(6704):777-80.

PMID:
9796812
14.

Galileo's First Images of Jupiter and the Galilean Satellites

Belton MJS, Head JW III, Ingersoll AP, Greeley R, McEwen AS, Klaasen KP, Senske D, Pappalardo R, Collins G, Vasavada AR, Sullivan R, Simonelli D, Geissler P, Carr MH, Davies ME, Veverka J, Gierasch PJ, Banfield D, Bell M, Chapman CR, Anger C, Greenberg R, Neukum G, Pilcher CB, Beebe RF, Burns JA, Fanale F, Ip W, Johnson TV, Morrison D, Moore J, Orton GS, Thomas P, West RA.

Science. 1996 Oct 18;274(5286):377-85.

PMID:
17813508
15.

Distribution of rock, metals, and ices in Callisto.

Anderson JD, Schubert G, Jacobson RA, Lau EL, Moore WB, Sjogren WL.

Science. 1998 Jun 5;280(5369):1573-6.

16.

A tenuous carbon dioxide atmosphere on Jupiter's moon Callisto.

Carlson RW.

Science. 1999 Feb 5;283(5403):820-1.

17.
18.

Galilean satellites of jupiter: 12.6-centimeter radar observations.

Campbell DB, Chandler JF, Pettengill GH, Shapiro II.

Science. 1977 May 6;196(4290):650-3.

PMID:
17760059
19.

Detection of ozone on Saturn's satellites Rhea and Dione.

Noll KS, Roush TL, Cruikshank DP, Johnson RE, Pendleton YJ.

Nature. 1997 Jul 3;388(6637):45-7.

PMID:
9214500
20.

Chaotic motion of europa and ganymede and the ganymede-callisto dichotomy.

Tittemore WC.

Science. 1990 Oct 12;250(4978):263-7.

PMID:
17797308

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