Phase curve (astronomy)
In astronomy, a phase curve describes the brightness of a reflecting body as a function of its phase angle. The brightness usually refers the object's absolute magnitude, which, in turn, is its apparent magnitude at a distance of one astronomical unit from the Earth and Sun.
The phase curve is useful for characterizing an object's regolith and atmosphere. It is also the basis for computing the geometrical albedo and the Bond albedo of the body. In ephemeris generation, the phase curve is used in conjunction with the distances from the object to the Sun and the Earth to calculate the apparent magnitude.
Mercury
The phase curve of Mercury is very steep, which is characteristic of a body on which bare regolith is exposed to view. At phase angles exceeding 90° the brightness falls off especially sharply. The shape of the phase curve indicates a mean slope on the surface of Mercury of about 16°, which is slightly smoother than that of the Moon. Approaching phase angle 0° the curve rises to a sharp peak. This surge in brightness is called the opposition effect because for most bodies it occurs at astronomical opposition when the body is opposite from the Sun in the sky. The width of the opposition surge for Mercury indicates that both the compaction state of the regolith and the distribution of particle sizes on the planet are similar to those on the Moon.Early visual observations contributing to the phase curve of Mercury were obtained by G. Muller in the 1800s and by André-Louis Danjon in the mid-twentieth century. W. Irvine and colleagues used photoelectric photometry in the 1960s. Some of these early data were analyzed by G. de Vaucouleurs, summarized by D. Harris and used for predicting apparent magnitudes in the Astronomical Almanac for several decades. Highly accurate new observations covering the widest range of phase angles to date were carried out by A. Mallama, D. Wang and R. Howard using the Large Angle and Spectrometric Coronograph on the Solar and Heliospheric Observatory satellite. They also obtained new CCD observations from the ground. These data are now the major source of the phase curve used in the Astronomical Almanac for predicting apparent magnitudes.
The apparent brightness of Mercury as seen from Earth is greatest at phase angle 0° when it can reach magnitude −2.6. At phase angles approaching 180° the planet fades to about magnitude +5 with the exact brightness depending on the phase angle at that particular conjunction. This difference of more than 7 magnitudes corresponds to a change of over a thousand times in apparent brightness.
Venus
The relatively flat phase curve of Venus is characteristic of a cloudy planet. In contrast to Mercury where the curve is strongly peaked approaching phase angle zero that of Venus is rounded. The wide illumination scattering angle of clouds, as opposed to the narrower scattering of regolith, causes this flattening of the phase curve. Venus exhibits a brightness surge near phase angle 170°, when it is a thin crescent, due to forward scattering of sunlight by droplets of sulfuric acid that are above the planet's cloud tops. Even beyond 170° the brightness does not decline very steeply.The history of observation and analysis of the phase curve of Venus is similar to that of Mercury. The best set of modern observations and interpretation was reported by A. Mallama, D. Wang and R. Howard. They used the LASCO instrument on SOHO and ground-based, CCD equipment to observe the phase curve from 2 to 179°. As with Mercury, these new data are the major source of the phase curve used in the Astronomical Almanac for predicting apparent magnitudes.
In contrast to Mercury the maximal apparent brightness of Venus as seen from Earth does not occur at phase angle zero. Since the phase curve of Venus is relatively flat while its distance from the Earth can vary greatly, maximum brightness occurs when the planet is a crescent, at phase angle 125°, at which time Venus can be as bright as magnitude −4.9. Near inferior conjunction the planet typically fades to about magnitude −3 although the exact value depends on the phase angle. The typical range in apparent brightness for Venus over the course of one apparition is less than a factor of 10 or merely 1% that of Mercury.
Earth
The phase curve of the Earth has not been determined as accurately as those for Mercury and Venus because its integrated brightness is difficult to measure from the surface. Instead of direct observation, earthshine reflected from the portion of the Moon not lit by the Sun has served as a proxy. A few direct measurements of the Earth's luminosity have been obtained with the EPOXI spacecraft. While they do not cover much of the phase curve they reveal a rotational light curve caused by the transit of dark oceans and bright land masses across the hemisphere. P. Goode and colleagues at Big Bear Solar Observatory have measured the earthshine and T. Livengood of NASA analyzed the EPOXI data.Earth as seen from Venus near opposition from the Sun would be extremely bright at magnitude −6. To an observer outside the Earth's orbit on Mars our planet would appear most luminous near the time of its greatest elongation from the Sun, at about magnitude −1.5.
Mars
Since it orbits further from the Sun only about half of the Martian phase curve can be observed from Earth. There is an opposition surge but it is less pronounced than that of Mercury. The rotation of bright and dark surface markings across its disk and variability of its atmospheric state superimpose variations on the phase curve. R. Schmude obtained many of the Mars brightness measurements used in a comprehensive phase curve analysis performed by A. Mallama.Because the orbit of Mars is considerably eccentric its brightness at opposition can range from magnitude −3.0 to −1.4. The minimum brightness is about magnitude +1.6 when Mars is on the opposite site of the Sun from the Earth. Rotational variations can elevate or suppress the brightness of Mars by 5% and global dust storms can increase its luminosity by 25%.
Giant planets
The outermost planets are so distant that only small portions of their phase curves near 0° can be evaluated from the Earth. That part of the curve is generally fairly flat, like that of Venus, for these cloudy planets.The apparent magnitude of Jupiter ranges from −2.9 to −1.4, Saturn from −0.5 to +1.4, Uranus from +5.3 to +6.0, and Neptune from +7.8 to +8.0. Most of these variations are due to distance. However, the magnitude range for Saturn also depends on its ring system as explained below.