  Recent Spitzer infrared (IR) observations of two transiting hot Jupiters
during their secondary eclipses have provided the first direct detection of
planets orbiting other stars (Charbonneau et al. 2005; Deming et al. 2005). We
here elaborate on some aspects of our detection of HD209458b at 24 microns, and
we compare to the detection of TrES-1 by Charbonneau et al. Spitzer will
eventually determine the IR spectral energy distribution of these and similar
hot Jupiters, opening the new field of comparative exoplanetology. For now, we
have only three Spitzer data points, augmented by upper limits from the ground.
We here interpret the available measurements from a purely observational
perspective, and we point out that a blackbody spectrum having T=1100K can
account for all current IR measurements, within the errors. This will surely
not remain true for long, since ongoing Spitzer observations will be very
sensitive to the IR characteristics of hot Jupiters.
