Less than a century after Einstein’s development of General Relativity (GR), physicists still marvel at its geometrical beauty and the myriad observational tests it has passed. One of the best tested theories in the history of science (that’s right IDiots - it’s “just” a theory), General Relativity is mature enough that these days it is increasingly being used as a tool through which to make other scientific discoveries. One of the most successful examples of this is the use of gravitational microlensing to tell us about the presence of small mass distributions - particularly planets.
The bending of light around massive bodies, as predicted by Einstein and later confirmed by Eddington’s observations during the 1919 solar eclipse, is a basic result of GR. Taken to extremes, light from a distant object, passing precisely around a closer, massive object leads to the Einstein Ring phenomenon. More typically, what is observed is a brightening of the light from a distant object as a massive object passes across the line of sight. In the eclipse observations, the presence of a known object was used to measure the way in which light bent, and thus to test GR. But these days, GR is so well understood on these scales, that one may turn this technique on its head and use GR as a tool, interpreting the brightening of such a distant object as evidence for an intervening mass distribution.
For planet detection, the increase in light from a far away star as a closer one passes can happen in a subtle way, revealing the presence of another massive object orbiting the nearer star. This is what is being reported for the smallest object so far - a roughly Earth-sized one. As the BBC article puts it
If the foreground star has a planet orbiting it, it will distort the light even more, and will make the star behind it look even brighter. But this effect lasts for a much shorter period, giving astronomers just hours or days to detect it.
Dr Martin Dominik from the University of St Andrews is a co-leader of the PLANET collaboration, one of the microlensing networks used to detect the new planet.
“We first saw the usual brightening reaching a peak magnification on 31 July 2005. On 10 August, however, there was a small ‘flash’ lasting about half a day,” he said.
“By succeeding in catching this anomaly with two of the telescopes of our network and with careful monitoring, we were able to conclude that the lens star is accompanied by a low-mass planet.”
The planet they discovered is unusual compared to other recently discovered extrasolar planets
The planet, which goes by the name OGLE-2005-BLG-390Lb, takes about 10 years to orbit its parent star, a red dwarf which is similar to the Sun but cooler and smaller.
It is in the same galaxy as Earth, the Milky Way, but is found closer to the galactic centre.
[…]
Like Earth, it has a rocky core and probably a thin atmosphere, but its large orbit and cool parent star mean it is a very cold world.
Predicted surface temperatures are minus 220 degrees Celcius (-364F), meaning that its surface is likely to be layer of frozen liquid. It may therefore resemble a more massive version of Pluto.
Since I spend a great deal of my time thinking about and investigating the role that GR plays in the early universe, it is nice to be reminded by stories such as this of the important role that GR plays in relatively late-universe science; in this case as a tool.
You can always rely on Albert.

So I was sitting on the bus reading and annotating my lecture notes on electromagnetic inductance for a lecture I was going to give 15 minutes later. A woman got on wearing a very short strapless red dress and medium height heels. She had short curly black hair. She seemed familiar in a way, but I could not place why, and she passed me and sat somewhere at the back of the bus. I carried on reading my notes. A few stops later the woman stood up and stood near the back door waiting for the bus to stop for her. I looked at her again, and it hit me. “She’s dressed a bit like Betty Boop, how funny!”, I thought to myself.
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But the real Source is Tainan, in the South of the island. Getting -at the last minute- the opportunity to go there, I gave a seminar on the 23rd December to the String Theory group (essentially all of the Taiwan string community came…this was part three of a series of talks), shut down my computer, excused myself as best and genuinely apologetically as I could, and grabbed my bags and headed for the door. A while later, after fortifying myself with a bowl of beef noodles (what else?) at Taipei Main Station, I headed for the bus, and the four and a half hour journey from Taipei to Tainan. There’s a bewildering variety of bus stops, and several bus companies to figure out, and getting on little shuttle buses to go to the other place to get the main bus….. and lots of yelling of destinations which I could not understand….I will not claim that I figured this all out myself……the brother of the friend I was going to stay with was also travelling this way, and so he offered to accompany me. I was dreading the bus journey, to be honest. It is not that I can’t do long bus journeys - as a student, to save money on home visits, I regularly took the marathon nine hour one leaving from from London Victoria at midnight, headed to every busstop between London and Preston - but that it was a bit cold, I only had my jacket, and I was not as well prepared in my mind for it either… I was not really in the mood for it, but it was the only way to get there and I was certainly going to go and was prepared to put up with whatever hardship it entailed.
