LCOGT is soliciting proposals for key projects: large, coherent observing programs designed to take maximum advantage of the unique capabilities of the LCOGT network to address important astrophysical problems. The goal of key projects is to produce the highest-impact science that can be done with the Network.
In 2016A, LCOGT Network has nine 1-meter telescopes and two 2-meter telescopes available for science observations. The SBIG cameras installed on some of the 1m telescopes are being replaced with Sinistro cameras during the (current) 2015B semester. The distribution of Sinistros and SBIGs will be announced before the start of the 2016A semester. The 2m telescopes are equipped with Spectral imagers and FLOYDS low-dispersion spectrographs. Up to 3000 hours of 1m time and 400 hours of 2m time will be allocated, depending on whether new key projects are approved.
Here's an update on recent LCOGT activities.
A team of astronomers have used the LCOGT network to detect light scattered by tiny particles (called Rayleigh scattering), through the atmosphere of a Neptune-size transiting exoplanet. This suggests a blue sky on this world which is only 100 light years away from us. The result was published in the Astrophysical Journal on November 20 (and is available on ArXiV).
Transits occur when an exoplanet passes in front of its parent star, reducing the amount of light we receive from the star by a small fraction. When the orbit of an exoplanet is aligned just right for transits to occur, astronomers can measure the planet’s size at different wavelengths in order to generate a spectrum of its atmosphere. The spectrum then reveals the substances present in the planet’s atmosphere, and therefore its composition. This measurement is most often performed using infrared light, where the planet is brightest and most easily observed. During the last few years, researchers have been probing the atmospheres of several small exoplanets with large ground and space-based telescopes, but have found it challenging to determine their composition using this method. This is either because the planets have clouds (which obscure the atmosphere) or because the measurements were not sufficiently precise.
It's no trick, but certainly a treat that on 31 October 2015 at 10:00 am PDT the near-Earth object (NEO) 2015 TB145 (nicknamed “spooky” by some) will pass within ~490,000 km or ~305,000 miles from Earth (roughly 1.3 times farther away than the Moon). Using our global network of telescopes at LCOGT, we have been monitoring 2015 TB145 for the past 2.5 weeks since shortly after it was discovered by the Panoramic Survey Telescope & Rapid Response System (Pan-STARRS) survey in Haleakala, Maui, Hawaii on 10 October 2015. Using our 1.0-m telescope in Cerro Tololo, Chile, we were one of the first groups to provide follow-up observations of 2015 TB145. These observations helped to improve the NEO's orbit and confirm that it will be whizzing past the Earth on Halloween.
The movie shows images taken from our 1.0-m telescopes in Southerland, South Africa and Cerro Tololo, Chile taken during seven 15 minute windows spaced roughly 1 hour apart. During this time, roughly 7 hours altogether, 2015 TB145 travels a distance across the sky of about 2.3 times the diameter of the Moon.
2015 TB145 is about 400 m in diameter (roughly 0.25 mile). At this size, if you were to skewer 2015 TB145 with the empire state building, only a small portion of the spire on top would stick out! It is roughly twenty times as large as the asteroid that hit Chelyabinsk, Russia on 15 February 2013. 2015 TB145 has a zero probability of hitting the Earth on Halloween, but keeping a watchful eye on all NEOs that come close to the Earth is important for determining the probability that future asteroids and comets could strike us and is an integral part of the work we do at LCOGT. Our ability to use multiple sites allows us to watch multiple objects at a time, and when keeping a close eye on one particular object these sites provide multiple opportunities to observe the object should one site develop bad weather or need to be used by another observing group.
2015 TB145 has a high eccentricity (highly elliptical) orbit with a three year orbital period that makes this Earth close approach quite rare since the NEO and Earth are rarely in the same place at the same time, making this a unique opportunity for astronomers to study this object. The observations from LCOGT telescopes will aid astronomers at NASA in aiming their Goldstone radio antennas at 2015 TB145, which will allow them to determine the object's shape using detailed radar images.
2015 TB145's unusual orbit also has astronomers curious as to whether it is an asteroid or a comet. Its highly elliptical orbit appears more like that of a comet, but 2015 TB145 does not show any signs of a bright coma or tail as it gets closer to the Sun as comets typically do. This could mean 2015 TB145 is an 'extinct' comet that has already lost all of its volatile material and now looks more like an asteroid. Its close proximity to the Earth will allow astronomers to take a closer look and hopefully answer this question. Overall, 2015 TB145 is proving to be quite a Halloween treat for astronomers!
Dear Users and Friends of LCOGT Network,
On 29 September 2015 the near-Earth object (NEO) 2015 SZ2 passed within roughly 500,00 km or 305,000 miles from Earth (that's only 1.3 times farther away than the Moon). At LCOGT, we monitored the NEO as it flew by. The movie shows images taken from our 1-m telescope in Chile during its closest approach, spanning about 45 minutes. Because of its very close proximity to the Earth, 2015 SZ2 traveled a distance across the sky of roughly 3.5 times the diameter of the Moon in that time!