Hidden Faces, now open at Nitroglobus Roof Gallery curated by Dido Haas, is an exhibition of photography by Monique Beebe. While no stranger to Second Life – she has been involved in the platform for the last decade – Hidden Faces marks the first public exhibition of her photography.
On display are twelve self-studies by Monique (or Moni, as she signs herself), offered in the familiar large format at Nitroglobus, which reveal the reason behind the exhibition’s title: in not one of them does the artist fully reveal her face. The most we see in those where her face may be partially exposed is the curve of cheek, soft line of jaw, sweep of nose and flare of nostrils and most particularly, the fullness of lips.
These glimpses are tantalising, sensual, and in at least one case – Thinking (seen at the top of this article) – edged with pensiveness. They draw us into the pictures in a physical way, the desire to reach out and caress a cheek, cup and gently lift a chin, to see the eyes that remain hidden, is powerful to the point of mesmerizing.
Each of the poses offered is equally as sensual, with a couple probably NSFW. In many Moni is dressed in little more than her underwear or in sheer slips and tops; her poses nuanced, the dark backdrop to each piece further heightening its sensual feel. In two of those where her face isn’t visible at all, their sensual nature is carried in other ways: the lace ribbons tied around wrists, the drape of pearls down a naked back…
But there is more here has well. While Moni may be shy about revealing herself fully in the spotlight of an art exhibition, but because the images are so personal – both to her and in our reaction to them, they imbue a feeling of closeness with her without in any way casting us into the role of voyeur. Rather, the suggestion is that these are intimate moments being willingly shared with us, because we are trusted.
Hidden Faces is a beautiful portfolio of work specifically created for this exhibition by an artist who may well be new to the SL exhibition circuit, but whose work is fully deserving of being seen by a wider audience. As such, I hope we’ll be able to see more of her work displayed at galleries in-world in the future. In the meantime, Hidden Faces will remain open through until late March.
On Wednesday, February 22nd, US space agency NASA, working with a team of European astronomers, confirmed no fewer than seven extra-solar planets are orbiting a star some 39 light years away – with three of them within the so-called “Goldilocks zone” of habitability.
The star in question is TRAPPIST-1, named for the instruments used in its discovery, the Transiting Planets and Planetesimals Small Telescope (TRAPPIST), and more formally known as 2MASS J23062928-0502285. Regular readers of my Space Sunday column might remember that I referred to the system back in November 2016, whilst discussing the James Webb Space Telescope and the hunt of exoplanets. The NASA announcement, which coincides with the publication of a new paper by the TRAPPIST team, adds dramatic new information to the distant star system.
The first two of the planets orbiting the star were located in May 2016, after the TRAPPIST team had studied the results of a continuous series of observations of the star between September and December 2015 using the telescope, located at the European Southern Observatory’s (ESO) La Silla Observatory in Chile.
What was intriguing about the two world was that not only were both within the so-called “Goldilocks zone” of their parent planet, where conditions might be “just right” for life to start, but both were roughly comparable to Earth in size, and therefore likely solid bodies, and spectral analysis suggested both have atmospheres.
A third planet, TRAPPIST-1d was also discovered the the same time, but it was behaving oddly. This prompted a further extended period of observation between September and October 2016, using both the ESO’s ground-based Very Large Telescope, and the Spitzer Space Telescope. This work revealed at “TRAPPIST-1d” was not one, but three worlds, again, all roughly in the Earth-sized category. Spitzer’s data additionally revealed two more planets of roughly the same size, taking the total to seven. Following this, Hubble turned its attention on the planets, looking for signs of hydrogen and helium – the chemical signatures that would indicate if any of them might be gas giants. It found none, further confirming they are likely rocky in nature.
The size, mass and density of these telluric worlds were obtained by measuring the periodic dips in TRAPPIST-1’s luminosity as a result of each of the planets passing in front of it. This allowed the international team studying the system to further assess whether each world was rocky, icy, or gaseous and determine which might be habitable.
TRAPPIST-1 is an ultra-cool red dwarf star only slightly larger than the planet Jupiter, and about 2,000 times dimmer than the sun.
Such stars, designated Class M, are the most frequent type of star in the Universe – making up an estimated 70% of stars in our galaxy alone. However, they do not radiate energy like our own sun, instead they are very volatile; all activity within them is entirely convective in nature, giving rise to massive stellar flares.
Given TRAPPIST-1 is so small, all of its planets orbit in very close proximity to it – closer than Mercury is to the Sun (the nearest orbits its parent star once every 1.5 terrestrial days, and the outermost, about once every 20 terrestrial days). This makes them very vulnerable to violent outbursts by the star, and could affect their surface conditions and their ability to retain an atmosphere.
This close proximity also means all of the planets are tidally locked – they always have the same side facing their sun. Thus they all are likely to have extremes of temperature, and those with an atmosphere are likely to have quite extreme weather as well. However – and conversely – it also means they could have the potential for liquid water to exist on their surfaces.
The innermost of the three planets in the habitable zone, TRAPPIST-1e, is very close in size to Earth, and receives about the same amount of light as Earth does, and may well have similar day time temperatures. The middle planet of the three, TRAPPIST-1f, meanwhile, might be a water rich world, also roughly the same size as Earth. It has a 9-day orbit, and receives about the same amount of light from its sun as Mars does from our own.