| Cerro Murphy Observatory | |
| Organization: | Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences |
| Location: | Antofagasta Region, Chile |
| Altitude: | 2817m (9,242feet) |
| Established: | 2005 |
| Telescope1 Name: | jk15 |
| Telescope1 Type: | 1.5-m reflector |
| Telescope2 Name: | zb08 |
| Telescope2 Type: | 0.8-m reflector |
| Telescope3 Name: | jk06 |
| Telescope3 Type: | 0.6-m reflector |
| Telescope4 Name: | IRIS |
| Telescope4 Type: | 0.8-m near-infrared reflector |
| Telescope5 Name: | Potsdam telescope |
| Telescope5 Type: | 30-cm refractor |
Cerro Murphy Observatory (Spanish: Observatorio Cerro Murphy, OCM; Polish: Obserwatorium Cerro Murphy, OCM; German: Observatorium Cerro Murphy, OCM; full name since 2023 is Rolf Chini Cerro Murphy Observatory) is an international astrophysical project hosted by the ESO Paranal Observatory and operated by the Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences. The observatory is located on Cerro Murphy, which is a hill located 1km (01miles) to the southwest and 230m (760feet) below the summit of Cerro Armazones, a mountain in the Antofagasta Region of Chile, 120km (80miles) south of Antofagasta. OCM is located at 2817m (9,242feet) altitude and currently houses 5 telescopes, whose diameters range between 0.3 and 1.5 m.
The observatory was established in 2005, owned and operated jointly by the Ruhr University Bochum (RUB) and the Catholic University of the North (UCN) until 2020, when it was transferred to the Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences (CAMK), and is now run by the Araucaria Project. The largest Polish telescope, with a mirror of diameter of 2.5 m, is currently being built by Astro Systeme Austria (ASA) and will start operations at OCM in 2026.
Three other observatories nearby are: the Paranal Observatory operated by the European Southern Observatory (ESO), the ESO's Extremely Large Telescope (currently under construction), and the Cherenkov Telescope Array gamma-ray telescope (also under construction, hosted by ESO).
The land for the observatory was donated to UCN by the Chilean government and it was protected by law for exclusive scientific research, securing the astronomical observations from being affected by possible future mining activities. Initially it was the summit of Cerro Armazones that was considered as the future observatory site, but after the measurements of the wind speed, the decision was made to settle on a slightly lower side hill, which is not so windswept. This hill was named Cerro Murphy to acknowledge the support from Prof. Miguel Murphy at UCN.[1]
The creation and development of the observatory is credited to prof. Rolf Chini from the Ruhr University in Bochum, who has supervised and been involved in all the works in the observatory (from laying the foundations for the telescope rooms and the main building, to setting up the computer network and software to control the telescopes, to carrying out science projects) from the very beginning till the present day.
The construction of the observatory at Cerro Murphy started in 2005 with cutting the top of the hill to provide a small flat plateau. Originally, the observatory was designed for 3 telescopes: 1.5m (04.9feet) Hexapod-Telescope (HPT) and two smaller auxiliary telescopes. The HPT was installed in 2006, and soon after, on September 28, 2006, the official inauguration of the observatory – initially called the Observatory Cerro Armazones (OCA) – took place in the presence of the German Ambassador in Chile, the president of the Chilean Astronomical Society, the rectors of UCN and RUB, a number of authorities from both universities, and numerous colleagues from ESO, CTIO, and the German Aerospace Center (DLR).
In 2010, within the framework of an ESO/European project (EVALSO) Cerro Murphy was connected by a 1 Gbps glass fiber to the Paranal Observatory. This innovation allowed for remote control of the telescopes from Bochum and provided a fast data transfer from Chile to Germany (60 GB per night). Up to that time, the observers had to take their data home on hard disks in their carry-on baggage.
On April 26, 2010, the ESO Council selected Cerro Armazones as the site for the planned ELT. In October 2011, an agreement was signed between the ESO and the Chilean government that includes the donation of 189 km2 of land around Cerro Armazones for the installation of the E-ELT as well as a concession for 50 years relating to the surrounding area.[2] As an inadvertent result of this agreement, the OCA became a telescope project hosted on ESO's land.
In 2017 the Leibniz Institute for Astrophysics in Potsdam (AIP) proposed to install a robotic 30 cm Zeiss refractor to support the satellite mission PLATO. This robotic telescope would stand in place of decommissioned HPT, which by 2017 had accumulated several technical problems, and could not be repaired due to a lack of replacement parts. In 2019 the Potsdam robotic telescope was installed at the observatory.
Also in 2017 an agreement was signed between the Ruhr University Bochum (RUB) and the Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences (CAMK) for the "use of observing time at the 0.8-m infrared telescope (IRIS)" by the Araucaria Project, led by Prof. Dr. habil. Grzegorz Pietrzyński. This marked the starting point for a fruitful collaboration between the two institutions, which eventually lead to the transfer of OCA to CAMK. The final contract between ESO, CAMK, and RUB was signed on January 17, 2020.
In 2020-2023, the observatory underwent renewal and expansion: 3 new telescopes were built while old ones were decommissioned. This huge scientific and technical undertaking was made possible thanks to generous financial support from the Polish Ministry of Education and Science, and the European ERC Synergy scientific grant, awarded to Prof. Pietrzyński. This financial support facilitates the construction of a 2.5-m telescope, which will be the largest Polish telescope ever built. So far, the telescope pillar has been erected, while subsequent construction phases are expected in 2024-2026.
On 28 November 2023, the inauguration of the renovated observatory took place, which was the occasion to announce the renaming of the observatory from the Cerro Armazones Observatory (OCA) to the Rolf Chini Cerro Murphy Observatory, abbreviated as the Observatory Cerro Murphy (OCM). The name change highlights a new chapter in the observatory's history featuring scientific projects related to the calibration of the cosmic distance scale (the main specialisation of the Araucaria Project), and emphasises the contribution of Prof. Rolf Chini, who supervised and participated in all construction work at the observatory. The name change also removes ambiguity regarding the location of the observatory; in Chile it is customary for observatories to bear the names of the hills on which they stand, and the ELT is being built on the top of Cerro Armazones.
A new 2.5-m telescope is under construction at ASA, while its foundations and the telescope pillar have already been erected at OCM. Subsequent construction phases are expected in 2024-2026.
There are also plans to build the Thirty Millimetre Telescope (TMMT), which will be the smallest telescope in the world, equipped with a professional infrared camera. Its purpose will be to observe the brightest stars in the sky, which are saturated by larger telescopes.
The observatory is located in the Atacama Desert about 120km (80miles) south of the city of Antofagasta. Due to its harsh atmospheric conditions, such as dry air and extremely low rainfall, the Atacama Desert is the best place for astronomical observations in the world, providing over 330 starry nights per year.
OCM was built on a hill, named Cerro Murphy, located 1km (01miles) to the southwest and approximately 230m (760feet) below the summit of Cerro Armazones. Such proximity to the Armazones mountain makes OCM the most closely located astronomical facility to ESO's future Extremely Large Telescope (ELT), just after the Paranal Observatory, located 20 km to the west, where the ELT observations will be taking place. Due to their proximity to the ELT, OCM and Paranal share some facilities, like optic fibers for internet, roads, etc. About 10 km south-east of Paranal, there is a construction site for the southern part of the Cherenkov Telescope Array gamma-ray telescope (hosted by ESO).
OCM embodies the philosophy of a "green" observatory, committing to minimize its environmental footprint. By design, OCM facilities were limited to a main building with two adjacent telescope rooms, and a compact auxiliary building for solar batteries and an emergency generator. The main building comprises two bedrooms with bathrooms, a social room, a kitchen, and a control room with a separate computer room; it is suitable for two observers who, in addition to observing, carry out all maintenance activities, including cleaning and meal preparations.
OCM is powered by solar panels, located on the main building's roof and the slopes of the hill. Solar energy is stored in batteries and used at night to carry out observations, and on cloudy days to maintain essential functions of the observatory, e.g. computers and servers, internet connectivity, water pump, heating, etc. OCM had also 3 wind turbines, which took advantage of strong winds, and provided additional source of energy at night and on cloudy days. In 2023, the wind turbines were replaced with a new array of solar panels, which, together with the existing solar panels, can meet the energy requirements of the expanded observatory.
The Hexapod-Telescope performed – among other projects – a high-resolution radial velocity spectroscopic survey of about 250 O- and 540 B-type stars in the southern Milky Way. It was found that the vast majority of stars (>82%) with masses above 16 solar masses form close binary systems.[4]
VYSOS6 conducted a multi-epoch r- and i-band survey of the southern galactic disk with the prime aim to find new, low-mass pre-main sequence stars and to monitor their light curves. This survey yielded light curves for 16 million stars including about 70,000 variables. Surprisingly, 62,000 of them were new detections, which means that almost 90% of variable objects in the Milky way were unknown before this survey.[5] Part of the data were compiled into the largest astronomical image ever, covering 50 square degrees and consisting of 46 billion pixels with 196 GB (http://gds.astro.rub.de).
BEST II was used to conduct photometric observations of the CoRoT LRc2 field in 2007. From the acquired data containing about 100,000 stars, 426 new periodic variable stars were identified and 90% of them are located within the CoRoT exoplanetary CCD segments and may be of further interest for CoRoT additional science programs.[6]
Near-infrared observations of RR Lyrae variable stars and type II Cepheids in the Milky Way, carried out on the IRIS telescope by the members of the Araucaria Project, allowed to determine new period-luminosity and period-luminosity-metallicity relations for the RR Lyrae stars[7] and, for the first time ever, period-luminosity relations for type II Cepheids.[8] The period-luminosity relation is a canonical method to determine cosmic distances to galaxies and clusters hosting pulsating stars, and these new results refine the method, making it even more precise.