Rocky World Discovered Through Microlensing

by Paul Gilster on January 25, 2006

The most Earth-like planet yet found has been discovered by a team of astronomers in a collaborative effort that involved 73 scientists in 12 countries. When astronomers use the term ‘Earth-like’ in this context, they’re referring to planets whose mass is closer to Earth’s than previous discoveries. They’re also talking about surface conditions, for OGLE-2005-BLG-390Lb seems to have a rocky surface, and is only five times as massive as Earth.

And what a fascinating find from the standpoint of technique. This is no relatively nearby gas giant found through observing the radial velocity changes it caused in its star’s path through space. Instead, the new world, some 20,000 light years away, was found through microlensing, where the gravity of an intervening star magnifies the light of a more distant star. Close study of the brightening phenomenon can reveal defects that are the telltale sign of a companion object.

In this case, as the star and its planet passed in front of the background star, the light curve showed the clear signature of a planetary body, as seen in the image below. OGLE-2005-BLG-390Lb is not the first planet found through microlensing, but the previous two have been gas giants larger than Jupiter.

Microlensing graph

Image (click to enlarge): Data obtained by PLANET/RoboNet, OGLE, and MOA on the microlensing event OGLE-2005-BLG-390 together with a model light curve, showing the planetary deviation on its falling part, lasting about a day. Also shown are best-fitting models with a single lens and a binary source (long-dashed) and a single-source-single-lens light curve (short-dashed). Each point represents the brightness in a single image and the data are colour-coded in order to indicate the telescope. The regular cycle of colors shows how observing is taken over by the next telescope in turn as the night ends at each site. An enlargement of the planetary deviation is shown as an inset in the top right. Credit: European Southern Observatory.

But back to the new planet: it orbits a red dwarf star five times less massive than the Sun in roughly ten years. Astronomers working on the project calculate its surface temperatures at 220 degrees Centigrade below zero, and suspect that the world has a thin atmosphere and a rocky surface buried deeply beneath frozen oceans. On that score, the Solar System analogue to OGLE-2005-BLG-390Lb may not be Earth so much as Pluto.

A heartening conclusion now being drawn from this work is that smaller, frozen worlds like this are more common than Jupiter-class gas giants, which have tended to be, overwhelmingly, the kind of worlds found by radial velocity searches. “Indeed if Jupiter-like planets were as widespread, the microlensing method should have found dozens of them by now,” said David Bennett (University of Notre Dame, USA), a PLANET team member. PLANET, one of the groups behind the find, is a network of one-meter class telescopes stretching from Chile to Australia and South Africa.

The paper, soon to appear in the January 26 Nature, is J.-P. Beaulieu, D. P. Bennett, P. Fouqué et al., “Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing” (abstract here). A Nature.com article is available, while audio and video podcasts on the discovery are online.

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ljk May 14, 2008 at 13:17

High magnification events by MOA in 2007

Authors: Philip Yock

(Submitted on 13 May 2008)

Abstract: Gravitational microlensing events of high magnification provide exceptional sensitivity to the presence of low-mass planets orbiting the lens star, including planets with masses as low as that of Earth. The essential requirement for the detection of such planets in these events is that the FWHM of the light curve be monitored continuously, or as nearly continuously as possible.

The dependence of planet detectability on the magnification caused by microlensing, on the planet mass and planet location, and on the size of the source star, may be understood in terms of simple geometrical properties of microlensing that have been known since 1964.

Planetary signals of low-mass planets are found to be approximately independent of the magnification caused by microlensing. This implies that planets can be detected in events over a wide range of magnifications, from moderately high values ~ 100 to very high values ~ 1000. The former values are likely to yield more clear-cut separations of the stellar and planetary features on the light curve, but they require larger telescopes to obtain precision photometry.

During 2007, twenty-four events with magnification exceeding 50 were detected by the MOA collaboration, of which about half were also detected by the OGLE collaboration. A quarter of the events received essentially continuous coverage of their FWHMs by follow-up collaborations, another quarter received partial coverage, and the remaining half received little coverage.

Final analysis of these events is still underway, but casual inspection of the light curves reveals some possible planetary detections amongst them. During 2008 it is hoped that fuller coverage of events of high magnification will be obtained with the addition of further telescopes to existing follow-up networks.

Comments: 13 pages, 17 figures, Manchester Microlensing Conference, January 2008. To be published in the proceedings

Subjects: Astrophysics (astro-ph)

Cite as: arXiv:0805.1775v1 [astro-ph]

Submission history

From: Philip Yock [view email]

[v1] Tue, 13 May 2008 04:07:02 GMT (304kb)

http://arxiv.org/abs/0805.1775

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