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This tag is associated with 38 posts

Recap of the IAU Planet Formation Symposium

Highlights from the International Astronomical Union Symposium on “Exploring the Formation and Evolution of Planetary Systems”.

Transit Probabilities: Not As Simple As They Seem

Our simple formula for predicting the probability that an exoplanet will transit might miss something important.

The actual transit is not shown, as its depth would overwhelm much of the structure in the out-of-transit light curve.

Characterizing Planets with BEER

Faigler et al. apply their BEER algorithm to a collection of stars in the Kepler field and find a hot Jupiter missed by the Kepler Science Team, showing a new way to find and characterize planets without follow-up observations.

The Frequency of (Habitable?) Planets Around M dwarfs

The census of planets for smaller stars—M dwarfs—is now basically complete. In this paper, Courtney Dressing and Dave Charbonneau use this M dwarf advantage to determine the occurrence rate of small planets around M dwarfs.

Credit: Karen Teramura (UH Institute for Astronomy) with background photograph by Wei-Hao Wang

Three’s a Crowd: Potential Triple-Star Systems in the Kepler Field

By looking for variations in the observed periods for eclipsing binary stars, astronomers have found evidence that a sizable fraction of these systems are actually systems of three or more stars.

Figure 3 from Szabo et al. 2012

Lonely No More: Do Other Planets and Exomoons Keep Hot Jupiters Company?

The leading theory is that hot Jupiters tend to occur in single planet systems, but Szabo et al. find evidence that some hot Jupiters might reside in multi-planet systems. Are hot Jupiters actually lonely?

Is that a planet?

Is it a comet or a planet?

First light from a super Earth

Last year, I reported on how the mystery of 55 Cancri e was resolved. In this Letter, Demory et al. observe the secondary eclipses of 55 Cnc e (when the planet passes behind the star), allowing them to determine the planet’s temperature. At 3,800 degrees Fahrenheit: this super Earth is not looking like a good vacation spot. They are also able to explore possible compositions for the planet.

Starspots in the Spot Light

This paper discusses the observed anomalies caused by starspot occultations due to transiting exoplanets. They are useful in determining the obliquity of the star with respect to the orbital plane of the transiting planet.

Detecting Moons Around Exoplanets

Moons in other solar systems are common in science fiction. Are they common in the universe as well? Kipping et al. are using Kepler data to find out.

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