Haller Base

Haller Base Haller-Basis
Lunar research station
Haller Base–Lunar Research Station
Haller Base facilities on the surface in 2008
Coat of arms
Haller Base
Sovereign state	Mascylla
Location on Luna	Jenssen crater, Soguichi Plateau
Administered by	Lunar Exploration Initiative of the MAOA and Air Force
Established	9 November 1987
Retired	15 February 2009
Named for	Emil G. Haller
Population  (1987 / 2008)
• Total	3 / 6
Type of operation
• Crew	All year-round
Operation
• Status	Inoperational
Dimensions	Length: 74 m (242.8 ft) Width: 30 m (98.4 ft) Height: 17 m (55.8 ft)
Facilities	9 buildings and facilities List Sahalinov Landing Site Accommodation and crew quarters Falkenhall Main Service Block Base Node Module Adapter 1, 2, and 3 Aufgang H-2B Crew Compartment and Science Module H-3 Science Module H-4 Utility Node Module H-5E Unpressurized Multipurpose Module Main Airlock Module Biomedical and astrophysical research facilities Communications and computer systems

Haller Base, officially the Haller Base–Lunar Research Station (Hesurian: Haller-Basis Lunare Forschungsstation), is a Mascyllary research station on the sloped rim of the Jenssen crater in the Soguichi Plateau, on the surface of Luna, the second planet of the world's binary planet system. It was operated under the Lunar Exploration Initiative (MLEI) jointly of the MAOA and Air Force from 1987 to 2009 and is considered to be the furthermost point of Mascyllary jurisdiction and only one on Luna. The base is named in honour of rocketry pioneer and polar explorer Emil Haller who was a significant contributor to the foundation of the MAOA and its early human spaceflight projects.

Haller Base is the first modular planetary station and first large man-made structure on Luna, and was assembled by over multiple subsequent manned missions from 1987 to 1999. The original base, less than a fifth of the completed station's volume and named Falkenhall, landed as part of the Sigma-Haller Expedition on 9 November 1987 by the space agencies of Mascylla and Dulebia as part of the Sigma program. With the Haller 87 and Haller 88 missions, the base became the first continuously inhabited research station on Luna and still maintains the longest duration of continuous human presence in space at 4,018 days. Since, the station has hosted up to 82 astronauts, the largest number for any Lunar research station, and has repeatedly been partially rebuilt and expanded upon. By 2008, Haller Base encompassed five pressurized modules, and two unpressurized components, the H-5E Unpressurized Multipurpose Module and the power-supplying photovoltaic array on the surface.

The station was purposefully constructed and ultimately served as a research laboratory which enabled crews to conduct scientific experiments on human biology, microgravity and radiation physics, astronomy, meteorology and space physics, as well as study the effects of long-term stay in space on humans. While the base operations and crew were militaristic in nature, it allowed scientific endeavours such as international collaborations with other countries to access the station. Haller 87 sustained three crew members, but the station's population continued to grow through its operation, with a peak six crew members of Haller 2000 and later 04 simultaneously on the station. In service from 1987 to 2009, Haller Base continued human presence on Luna, before it was agreed upon by the MLEI to retire the station in February 2009 mainly due to its aging hardware, damages sustained by meteorological phenomena and regolith exposure. The station has since been unoccupied and plans to either repurpose it for another settlement or preserve it as a protected area have been put forward.

Structural history

Original base (1987–1989)

Construction and Sigma-Haller Expedition

The initial first component of the station, the pressurized Falkenhall Main Service Block (Hauptbetriebsblock; MSB) module and its adjacent solar arrays measuring 4,000 m² of operable area, were manufactured at the Gräbler Spaceflight Center near Rothenau, Aldia, beginning in 1982. The name Falkenhall was ultimately chosen by MAOA in reference to the oldest continuously inhabited urban settlement in modern-day Mascylla, having been founded by 600 BC. The modules were delivered on ship to the Spacecraft Processing Facility and Main Flight Operations Building at Cape Weimud Space Center in Akawhk in August of 1987 for final inspections, processing and preparation for launch. The module was designed with three docking ports suitable for berthing operations, three autonomous arrays of solar cells measuring 4.5 by 1.3 meters (14.7 by 4.3 feet) mounted on its roof, six nickel-cadmium batteries with a capacity of 4 kilowatts of power, ten externally mounted fuel tanks holding 8.8 tonnes of propellant, and is outfitted with early communications and control equipment. Falkenhall has a dry mass of 21,492 kilograms (47,382 lb), is 8.2 meters (26.9 ft) long and 4.1 (13.5 ft) meters wide.

Launch of the modified Atlant-3L carrying the Sigma-Haller Expedition from Akawhk, 6 November 1987

The module Falkenhall during the Haller 87 Expedition in December 1987, photographed by Thomas Knopp; note LM-15 Hährnig in the distance and the deployed solar arrays and parabolic antenna on the module's roof.

Falkenhall was launched on 6 November 1987 on a purpose-built and modified version of the Atlant-3 rocket from Cape Weimud in Akawhk; the mission was incorporated into the Sigma program as the Sigma-Haller Expedition, crewed by a joint Dulebian-Mascyllary crew of Mission Commander Janus Heine. After the initial launch and the first two stage separations, the payload ascended to a 500 km (311 mi) high parking orbit. Eight hours later, the crew of the Sigma-Haller Expedition was launched to the cargo stage waiting in orbit on an Atlant-4G, and performed a subsequent space rendezvous. The spacecraft complex was manned for re-configuration and trans-lunar flight preparations before firing the CSM third upper stage for trans-lunar injection on 7 November.

On 9 November, the two-stage Falkenhall module and its cargo load, referred to as LM-13 Dnepr, separated from the Sigma Command and Service Module (Kommando- und Betriebsmodul; CSM) Antares, having ferried it to lunar orbit, and descended to Luna's surface; Dnepr touched down at the ridges of Jenssen crater of the Soguichi Plateau at 05:22 UTC. The three astronauts of the resident crew stayed on the newly established lunar base before returning to the CSM in low orbit; the base module served as the launch pad for the ascent stage, similar in operation to the Sigma Lunar Module (Lunarmodul; LM), which then docked with CSM-98 Antares again and was subsequently discarded. After 6 days of stay and the 4 days of travel following the trans-Aurorum injection, the crew of the Sigma-Haller Expedition returned to Aurorum on 18 November.

Complications and modification

The ascent stage of Dnepr inadvertently polluted the photovoltaic arrays with whirled up lunar regolith, which caused Falkenhall to suffer a blackout one day after Sigma-Haller's departure. Contact to the automatic systems of the station remained severed until the Haller 87 Expedition was able to clean and re-orientate the solar arrays while moving them 700 meters (2,297 feet) away from the designated but improvised landing and take-off site, two weeks later in December of 1987. During the Haller 88 Expedition in July of 1988, a repurposed descent propulsion system similarly used in the LM descent stage was utilized to blow away possibly hazardous or inhibiting regolith from the designated site and heat the material to fuse it into a durable and hardened platform. After installing edge and status lighting, LM-17 Heiserer of the Haller 89 Expedition was the first to land on the Sahalinov Landing Site (Sahalinow-Landungsplatz; SLS); in 1994, a second SLS including seven additional external fuel storage tanks were constructed 30 meters (98.4 ft) away from the first SLS.

Added modules (1989–1999)

Assembly

The LSAM was crucial for the assembly and construction of Haller Base due to its heavy-payload and large crew capacity (LM-20 Hoffnung during the Haller 92 Expedition, with astronaut Simon Müller next to it for size comparison, 30 May 1992

The construction of Haller Base was a major and ultimately multi-national undertaking in space and lunar architecture. The initial assembly began in November 1988 during the Haller 89 Expedition when two Base Node Module Adapters (Basisknotenmoduladapter; BNMAs) were attached to the passive Falkenhall module by two astronauts performing extra-vehicular activities, serving as nodes for future additions. Over the course of Haller Base's assembly, astronauts used some 1,100 hours of EVA operations as well as the Mobile Servicing Robotic Unit (Mobiles Betriebsrobotikeinheit; MSRU) as the base expanded in size and complexity. Similarly, since the Haller 92 Expedition, Haller Base was serviced and supplied by an evolved and heavy-payload five-astronaut version of the 1980s Sigma LM, the Lunar Surface Access Module (Lunares Modul für Oberflächenerkundung; LSAM); because the first active LSAM was LM-19 Fischadler, it is sometimes referred to as Fischadler (meaning "Osprey") by itself.

Elements

Fore view of the 1999 control and operations room of the Aufgang CCSM module

Aft view of the control and operations room

On 30 July 1989, the H-2B Crew Compartment and Science Module (Truppenabteil und Wissenschaftsmodul; CCSM) was launched into orbit and then delivered to Luna via the Haller 90 Expedition. The H-2B–Sagittarius vehicle performed the descent and docking to the Falkenhall-BNMA complex part-automatically and part-manually. Serving as the new operational centre of Haller Base, the H-2B module's computer system autonomously assumed control over the base from Falkenhall's systems, and was equipped with designated crew and sleeping quarters, a kitchen, multiple toilets and sanitary systems, and exercise equipment. Additionally, the scientific compartment of the large cylindric module, measuring 13.3 meters (43.6 ft) in diameter, supplemented the Falkenhall life-support systems with CO₂ scrubbers, dehumidifiers, wastewater treatment systems, and oxygen generators. It also comprises the central command and operations room of the base. Mission Commander Felix Ahrndt later recalled the happiness and gratitude of subsequent Haller Expedition astronauts who stayed in the base before the expansions in 2011, commenting: "By this point Falkenhall was, well, "overcrowded" would be an understatement. It was like a tan of sardines, speaking from experience and talking to other Haller astronauts, and everyone talked about how happy they were that they now could take more than eight steps in any direction. H-2B was like a cathedral in comparison to the old Falkenhall lady." In 1991, H-2B was officially renamed to Aufgang (meaning "Dawn").

Over the next four years, Haller Base continued to expand. During the 1991 Haller 92 Expedition, the H-3 Science Module (Wissenschaftsmodul) was delivered to Luna as the primary new facility for research payloads, scientific experiments and medical life-support operations. The 23.1-tonne (50,927 lb) heavy research and experimental laboratory is identical in layout and design to the H-2B Aufgang module and was permanently berthed to it on 29 January 1992, and has since been the location of active research on Haller Base, encompassing studies and experiments relating to medicine, biotechnology, materials science, and other fields of physics. Aufgang was used frequently by international teams of scientists and for scientific research contributions of participating states, most notably Lavaria and Dulebia, in the form of experiments and delivered technology.

In 1994, the Haller 94 Expedition contributed the Main Airlock Module (Hauptluftschleusenmodul; MAM) to the base, intended to relieve Falkenhall's forward airlock system of potentially damaging over-use; before the addition of the MAM, EVAs could only be performed through the forward door of the first module, and an almost fatal accident during the Haller 93 Expedition on 2 September 1993 involving astronaut Lukas Krausmann highlighted the frequently used airlock's strain. It provided the base's capability of EVA operations on the lunar surface and was attached to Haller Base inbetween the Aufgang and H-3 modules. In order to alleviate the issue of the rapidly deteriorating performance of airlocks due to regolith exposure, the airlock, being 4.2 meters (13.7 ft) in diameter and 7.9 meters (25.9 ft) long, comprises two separate passageways, one from which astronauts can exit the base, and a smaller hatch for equipment storage and to clean used EVA suits of regolith, as well as nitrogen to mitigate post-spacewalk decompression sickness.

Two additional BNMAs and a more compact version of the H-2B and H-3 modules serving as a central node for the newer Haller Base complex, the H-4 Utility Node Module (Nutzknotenmodul; UNM), were delivered on the Haller 96, 97 and 98 Expeditions. The UNM accommodates additional sleeping quarters and sanitary systems for astronauts, and more importantly, houses vital electrical power storage units, areas for cargo holds, and controls for the base's electronic system; the addition of the UNM was in response to the base's rapidly increasing power consumption and ineffective control of power-generating capabilities from Aufgang, as was the installation of another 980 m² (10,549 sq ft) of photovoltaic arrays outside Haller Base in 1997. During the Haller 98 Expedition in 1998, Haller Base was outfitted with 197 plates of a composite secondary hull consisting of stainless steel, kevlar and aluminium alloy to protect it from micrometeoroids.

Haller Base in 2001, with the vast majority of its modules visible: the H-3 Science Module (far left), BNMA 3 (left), MAM and H-4 UNM (centre), H-5E UMPM (above H-4), Aufgang H-2B CCSM (right), and Falkenhall MSB (far right).

The final expansion of the base to this date, the H-5E Unpressurized Multipurpose Module (Druckloses Mehrzweckmodul; UMPM), was brought to Luna in March of 1999 by the Haller 2000 Expedition. The UMPM was vertically mounted on top of the zenith docking port of the H-4 UNM, requiring 18 separate EVAs over the span of 48 hours and two specialized aerial work platforms. Once completed, the UMPM raised the total height of Haller Base to 17 meters (55.8 ft), and was added with the scientific experiments and devices intended for the module in the Haller 2000 and 01 Expeditions: the Wilhelm G. Neumayer Astronomical Observatory (Astronomisches Observatorium Wilhelm G. Neumayer; WiGNAO), Atmospheric and Lunaological Research Observatory (Atmosphärisches und Lunaologisches Forschungsobservatorium; ALRO), Angular Cosmic Interferometer (Kosmisches Winkelinterferometer; ACI), Lunar Muon and Neutrino Detector Array (Lunares Myon- und Neutrinodetektorfeld; LUMONDA), and Lunar Magnetic Spectrometer (Lunares Magnetospektrometer; LMS). WiGNAO is an astrophysical observatory equiped with an iliosar telescope, x-ray, extreme ultraviolet and Hα spectroheliographs, and a coronagraph intended for space weather prediction and x-ray astronomy; ALRO, also being an observatory, was used for observational astronomy, as well as imaging spectroscopy, energetic neutral atom imagery and mass spectrometry of Luna's surface and faint atmosphere. ACI observed the power spectrum, polarization and temperature anisotropies of the cosmic microwave background (CMB) to survey galaxy clusters, whereas LUMONDA was a high-energy neutrino observatory and the LMS magnetic spectrometer investigated antimatter amounts in cosmic rays.

Completed state (1999–present)

Haller Base (center) at the slope edges of the Jenssen crater in 2004, with the Sahalinov Landing Site (upper right corner)

By February of 2009, Haller Base consisted of five pressurized and two unpressurized modules. Following the announcement of the program's retirement, the last resident crew onboard the base, the Haller 09 Expedition, celebrated its continuous operation and deactivated its life-support system upon the crew's departure on 15 February. The numerous scientific experiments in the UMPM continued to be used by scientists on Aurorum and relay research data for another four years, until the base's central computer was commanded to go on stand-by in 2013. While Haller Base has not been in activation ever since, as of 2022, the photovoltaic arrays and electronic systems are still considered to be fully operational if activity were to be resumed. However, in 2019, multiple micrometeoroids damaged the parabolic communications antennae on Aufgang's outer hull, thus impairing direct communication to and from Aurorum.

International cooperation

Commemorative plaque of the LBJUIA, signed on October 22 1988

Participating states of the programme:

  Head state (Mascylla)

  Signatories of the LBJUIA (including the Republic of Dulebia)

  Participating states which contributed at least one astronaut

The Mascyllary Lunar Exploration Initiative included a formal provision, the Lunar Base Joint Use Intergovernmental Agreement (LBJUIA), which allowed members and citizens from interested countries (eight in total) to participate in crewed spaceflights to Haller Base and contribute scientific experiments or other payloads to regular Expeditions. However, the LBJUIA does not govern nor specify the legal foundations of the programme and the base itself, and because no other to-date convention of international law governing formal jurisdiction on Luna is in effect, Haller Base is de facto a stateless property on territory akin to international waters; simultaneously, it is generally accepted to be subject to Mascyllary legal jurisdiction (the only country to de jure govern territory outside Aurorum, but not exercise sovereignty), despite the lack of any formal convention or agreement.

Participating countries

• People's Republic of Dulebia (1987–1990)
• Dulebia
• Falland
• Lavaria
• Sarrac
• Telmerian Union
  • Lilienburg
  • Temaria
  • Valtriva
  • Valimia

Astronauts

Various Berean and Pamiran astronauts visited Haller Base over the course of the LBJUIA's existence and its operation, in order:

• Wladimir Selyov – during the 1987 Sigma-Haller Expedition People's Republic of Dulebia
• Balduíno Miranda – during the 1992 Haller 92 Expedition Lavaria
• Corin Côté – during the 1996 Haller 96 Expedition Sarrac
• Kirill Antonov – during the 1997 Haller 97 Expedition Dulebia
• Tuomo Mäkinen – during the 1998 Haller 98 Expedition Valimia
• Estevão de Mascarenhas – during the 1999 Haller 99 Expedition Lavaria
• Radomil Borisov – during the 2000 Haller 2000 Expedition Dulebia
• Valquíria Costa – during the 2001 Haller 01 Expedition Lavaria
• Felix Kirchhöfer – during the 2002 Haller 02 Expedition Temaria
• Lidiya Vinogradova – during the 2004 Haller 04 Expedition Dulebia
• Claudette Tremblay – during the 2005 Haller 05 Expedition Sarrac
• Deodato Araújo – during the 2008 Haller 08 Expedition Lavaria

Operation

Expeditions typically stay for multiple months and in some cases for almost the duration of a full year in the base, thus isolating them for extended periods of time. This has presented researched and reported dangers to crew health and inter-personal relations, among other stresses of physical and psychological nature. During the Expeditions, Haller Base is completely self-sufficient through extensive storage of food, water, and the autonomous solar power supply; during lunar nights, a system of batteries supports power consumption while a 2002-installed small-scale radioisotope thermoelectric generator is intended for emergency use in the case of a blackout. When crews are not present, ground control as well as automated central computer systems located in the H-2B CCSM oversee basic utilities and operations in the base.

Crew stay

A package of food served on a tray, during the Haller 97 Expedition

Wide view of the Falkenhall MSB interior in 2003, with the galley (left) and three of the crew quarters' booths (right)

The station was originally supposed to remain in operation for a total of ten years, but instead operated for almost twice the intended span. As a result, the older components of Haller Base, most notably the Falkenhall module, were often compared to a cramped and visibly used-looking "labyrinth" with exposed technical equipment and hoses, as well as crowded with cargo; the modules added in the later development of the base were considerably more modern and new, as had been pointed out by crew members.

The operation of Haller Base was subject to a stringent timetable and schedule as provided by the ground operators. The time zone used in Haller Base was Eastern Berean Time (EBT; UTC+03:00). Due to the 3.5-day long lunar days and equally long lunar nights on the surface, certain measures were taken to re-create the temporal cycle as perceived on Aurorum, mainly for crew comfort and convenience, like covering windows during "night hours", dimming internal lighting, or adjusting light colour temperature. While the morning and mid-day were reserved for work, exercise to combat muscle atrophy and spaceflight osteopenia, and space food breaks, the evening could be used by crew members for recreational or other activities. Haller Base was supplied with a number of items to provide entertainment for astronauts in their spare time: books, films, a collection of pre-recorded music, and a guitar. Additionally, astronauts brought along their own personal belongings in a designated bag, which they stored in their crew quarters.

Astronauts stayed and slept in phonebox-sized soundproof booths, similar in appearance and style to bunk beds on board naval vessels. The crew quarters were equipped with secured trunks for personal belongings, shelves, reading lamps, laptops, and a small window; the actual bed could remain un-tethered and horizontal due to Luna's noteworthy gravity. Two designated galley areas are located next to the quarters, which are mostly located in the H-3 SM, as is the area for sanitary and hygienic utilities, including three space toilets and a shower. The galleys feature three food warmers similar to a microwave, two refrigerators, a locked safe for alcoholic beverages (such as cognac, vodka, and schnapps) only accessible to the Expedition Commander, and a water dispenser. Despite the fact that crumbly food can be safely eaten due to the lack of weightlessness, most foods eaten in the base do not create crumbs, as vacuum sealed, frozen, and freeze-dried packaged food could be stored for longer for the long durations of Expeditions. Nevertheless, it is custom for arriving astronauts to re-stock the base with fresh vegetables and fruits, as well as sweets.

Transportation and communication

The Lunar Roving Vehicle (LRV) was vital for EVA surface activities (astronaut Ursula Witt on an excursion during the Haller 92 Expedition, 12 November 1991).

The base has two landing areas for spacecraft, the Sahalinov Landing Sites (SLS; ICAO: ASLP), each 29.6 meters (97.1 feet) in diameter. Usually, these are reserved for the Expeditions' descent configurations of the LM from 1987 to 1992 and the heavy-version LSAM since 1992. In rare circumstances, parked vehicles might need to be removed or relocated to allow for resupply missions, automated cargo LSAMs, to land at Haller Base. Flights to and from the SLSs depend on the arrival and departures of the respective crews, but LSAMs have also been used to scout and explore nearby areas of interest surrounding the base, such was the case during the Haller 93, 96, 2000, and 05 Expeditions.

The SLS landing pads are connected to the base through multiple improvised 900-meter (2953-feet) long routes used as regolith roads, termed the Thomas L. Knopp Lunar Highway (TKLH; Lunare Autobahn–Thomas L. Knopp). Ground transportation of crew and cargo is made possible by the Lunar Roving Vehicle (LRV; Lunares Lauffahrzeug), in use since the original Sigma program. Concepts of replacing the LRV with a pressurized modular cabin vehicle for long-term stay were discarded due to budgetory and practical restraints.

Communication of Haller Base is provided by the MAOA's VDÜS-2 and 4 satellites, and the VSKS-11 satellite of the Ministry of Defence of the Realm; these allow a date-transfer rate of some 60 Mbit per second, as well as broadband internet and satellite phone telecommunications access.

Expeditions

Designation	Patch	Crew (Expedition Commander)	Launch date	Landing date	Return date	Duration (days)	CSM	LM	Summary
Sigma-Haller Expedition		Janus Heine Peter-Hannes Wolf Wladimir Selyov	6 November 1987	9 November 1987	18 November 1987	6	CSM-98 Antares	LM-13 Dnepr	First over-all and crewed expedition, successful landing of the original Haller base compartment at Jenssen crater. Establishment of photovoltaic energy supply and preparation for Haller 87.
Haller 87 Expedition		Thomas Knopp Alexander Persching Karl Weisze	14 December 1987	17 December 1987	2 June 1988	168	CSM-99 Von Bauer	LM-15 Hährnig	Second expedition, first officially scientific expedition plan.
Haller 88 Expedition		Bartosz Maininger Daniel Bursch Reinhard Voß	9 July 1988	13 July 1988	23 November 1988	130	CSM-100 Borealis	LM-16 Unternehmen	Third expedition, established the first Sahalinov Landing Site.
Haller 89 Expedition		Walther Siewert Ursula Witt Josef Ohlsig	22 November 1988	25 November 1988	4 July 1989	221	CSM-101 Nordstern	LM-17 Heiserer	Fourth expedition, added two node modules for future expansion, Ursula Witt as the first female astronaut on Luna.
Haller 90 Expedition		Felix Ahrndt Hanno Foch Andreas Gerste	30 July 1989	2 August 1989	17 March 1990	230	CSM-103 Görche	LM-18 Sagittarius	Fifth expedition, docked H-2B crew compartment and science module to B node module.
Haller 91 Expedition		Harald Lesch Leopold Richter Hannah Gutenfeld Gregor Ellen Steffen Heese	28 May 1990	1 June 1990	7 March 1991	279	CSM-104 Erkunder	LM-19 Fischadler	Sixth expedition, first five-member expedition.
Haller 92 Expedition		Ursula Witt Simon Müller Christoph Osbeck Balduíno Miranda Moritz Peskycz	30 September 1991	5 October 1991	11 July 1992	280	CSM-105 Sextant	LSAM-20 Hoffnung	Seventh expedition, first expedition commanded by a woman and first international one with Balduíno Miranda, also the first Lavish citizen on Luna. Added the H-3 Science Module.
Haller 93 Expedition		Leopold Richter Heinz-Dieter Würsinger Lukas Krausmann Charlotte Reichenbach	1 December 1992	7 December 1992	17 September 1993	284	CSM-107 Aldebaran	LSAM-21 Brieselang	Eighth expedition, witnessed the Lukas Krausmann Falkenhall airlock incident.
Haller 94 Expedition		Hanno Foch Gregor Ellen Achim Hagedorn	12 September 1993	17 September 1993	30 July 1994	286	CSM-108 Föhn	LSAM-22 Spinne	Ninth expedition, established the second Sahalinov Landing Site and added the Main Airlock Module.
Haller 95 Expedition		Charlotte Reichenbach Steffen Heese Josef Ohlsig	12 August 1994	18 August 1994	4 July 1995	320	CSM-109 Antares II	LSAM-23 Dnepr II	Tenth expedition.
Haller 96 Expedition		Sylvia Trauth Lukas Krausmann Dirk-Philip Scheffel Corin Côté	29 June 1995	4 July 1995	20 March 1996	260	CSM-111 Rohrn	LSAM-24 Ambition	Eleventh expedition, added the BNMA 2. First Sarracese citizen on Luna with Corin Côté.
Haller 97 Expedition		Robert Behr Florentin Lehmann Hannah Gutenfeld Christoph Osbeck Kirill Antonov	1 April 1996	8 April 1996	11 January 1997	278	CSM-112 Werner	LSAM-26 Astrolabium	Twelth expedition, added the BNMA 3 and additional photovoltaic arrays on the lunar surface.
Haller 98 Expedition		Simon Müller Achim Hagedorn Oliver Werfel Tuomo Mäkinen	3 November 1997	7 November 1997	17 August 1998	283	CSM-113 Sigurd	LSAM-27 Erkunder II	Thirteenth expedition, added the H-4 Utility Node Module. First Valimian citizen in space and on Luna with Tuomo Mäkinen.
Haller 99 Expedition		Dirk-Philip Scheffel Hannah Gutenfeld Estevão de Mascarenhas	6 October 1998	10 October 1998	21 September 1999	346	CSM-114 Sirius	LSAM-28 Esforço	Fourteenth expedition.
Haller 2000 Expedition		Janik Lischke Manuela Letzel Daniel Bursch Fabian Hopfer Radomil Borisov Konrad Goedde	20 December 1999	23 December 1999	7 May 2000	136	CSM-115 Lena	LSAM-29 Union	Fifteenth expedition, added the H-5E Unpressurized Multipurpose Module, Wilhelm G. Neumayer Astronomical Observatory, and Atmospheric and Lunaological Research Observatory.
Haller 01 Expedition		Florentin Lehmann Robert Behr Valquíria Costa Gregor Ellen	8 July 2000	12 July 2000	17 February 2001	220	CSM-116 Beteigeuze	LSAM-30 Fortuna	Sixteenth expedition, added the Angular Cosmic Interferometer, Lunar Muon and Neutrino Detector Array, and Lunar Magnetic Spectrometer.
Haller 02 Expedition		Manuela Letzel Oliver Werfel Felix Kirchhöfer	21 June 2001	25 June 2001	23 April 2002	302	CSM-120 Ergreifer	LSAM-31 Erkunder III	Seventeenth expedition, first Temarian citizen in space and on Luna with Felix Kirchhöfer.
Haller 03 Expedition		Laurenz Kiesling Daniel Bursch Konrad Goedde Heinz-Dieter Würsinger	29 September 2002	2 October 2002	9 June 2003	250	CSM-121 Liga	LSAM-32 Entdecker	Eighteenth expedition.
Haller 04 Expedition		Fabian Hopfer Sylvia Trauth Robert Behr Achim Hagedorn Carsten Wallner Lidiya Vinogradova	30 November 2003	2 December 2003	30 May 2004	180	CSM-122 Agretta	LSAM-33 Halie	Nineteenth expedition, first Dulebian woman on Luna with Lidiya Vinogradova.
Haller 05 Expedition		Konrad Goedde Oliver Werfel Katharina Heep Claudette Tremblay Gregor Ellen	24 January 2005	27 January 2005	29 December 2005	336	CSM-123 Leopold Brasich	LSAM-34 Augúste Marchial	Twentieth expedition, first Sarracese woman in space and on Luna with Claudette Tremblay.
Haller 06 Expedition		Heinz-Dieter Würsinger Matthias Nothnagel Laurenz Kiesling	21 March 2006	25 March 2006	18 November 2006	238	CSM-124 Nordstern II	LSAM-35 Fortuna II	Twenty-first expedition.
Haller 07 Expedition		Gregor Ellen Manuela Letzel Casper Haushofer	13 February 2007	16 February 2007	6 September 2007	202	CSM-125 Nachtigall	LSAM-36 Von Grübbe	Twenty-second expedition.
Haller 08 Expedition		Matthias Nothnagel Hannah Gutenfeld Josef Ohlsig Deodato Araújo	1 September 2007	4 September 2007	10 March 2008	178	CSM-126 Baranson	LSAM-37 Weißhaupt	Twenty-third expedition.
Haller 09 Expedition		Casper Haushofer Carsten Wallner Steffen Heese Charlotte Reichenbach Sylvia Trauth	27 February 2008	2 March 2008	6 March 2009	369	CSM-127 Alpha	LSAM-38 Omega	Twenty-fourth and last expedition to-date (as of 2022). Longest mission to-date and only one to take place over more than a full year.