A limitation of the radial velocity method used to detect Upsilon Andromedae b is that only a lower limit on the
mass can be found. The
true mass may be much greater depending on the
inclination of the orbit. Based on an analysis of the dynamic stability of the planetary system and the preference for
prograde orbital solutions, the planet's inclination should be in the range of °, resulting in a true mass of . This helped confirming that
hot Jupiters have distinct temperatures on the dayside (always faced to the host star) and the nightside (always facing away). The measured
phase curve of the planet together with measurements of the
orbital inclination allows an estimate of its radius, which is thought to be 1.8
Jupiter radii () based on the likely inclination values, making it one of the
largest known exoplanets. The cloud deck instead absorbs the star's radiation; between that and the hot, high-pressure gas surrounding the mantle, exists a
stratosphere of cooler gas. The outer shell of dark, opaque, hot cloud is assumed to consist of
vanadium and
titanium oxides, but other compounds like
tholins cannot be ruled out yet. The chemical elements in the atmosphere can be studied by finding their absorption lines in the thermal spectrum of the planet; given typical planet temperatures, the spectrum has its peak at infrared wavelengths. So far, only
water vapor has been detected in this planet, while
carbon monoxide and
methane are still under the detection limit. The planet (with
51 Pegasi b) was deemed a candidate for direct imaging by
Planetpol. Preliminary results from polarimetric studies indicate that the planet has a predominately blue color, is 1.36 times as large and 0.74 times as massive as Jupiter, meaning that the mean density is 0.36g/cm3. It has a
geometric albedo of 0.35 in visible light. In 2016–2017 the direct detection of the planetary thermal emission was claimed, but the detection was questioned in 2021. Similarly, the planet was not detected using high-resolution
inferterometric observations by the
CHARA array. == Host star ==