Compton Spectrometer and Imager

{{Infobox spaceflight

| name = Compton Spectrometer and Imager
(COSI)

| names_list = COSI
SMEX-17

| image = COSI higher quality.jpg

| image_caption = Artistic rendering of COSI

| image_size = 300px

| mission_type = Gamma-ray astronomy

| operator = University of California, Berkeley
NASA

| COSPAR_ID =

| SATCAT =

| website = https://cosi.ssl.berkeley.edu/

| mission_duration =

| spacecraft = COSI

| spacecraft_type =

| spacecraft_bus =

| manufacturer =

| launch_mass =

| payload_mass = < 400 kg

| dimensions =

| power =

| launch_date = August 2027 (planned)

| launch_rocket = Falcon 9

| launch_site = Cape Canaveral Space Force Station

| launch_contractor = SpaceX

| last_contact =

| decay =

| orbit_reference = Geocentric orbit

| orbit_regime = Low Earth orbit

| orbit_periapsis =

| orbit_apoapsis =

| orbit_inclination =

| orbit_period =

| apsis = gee

| instruments =

| telescope_area = 25% field of view of the sky

| telescope_name = Compton telescope

| instrument_type = Germanium detectors

| telescope_type =

| telescope_diameter =

| telescope_focal_length =

| telescope_wavelength =

| trans_band = Gamma Rays

| trans_frequency =

| trans_bandwidth = 0.2–5 MeV

| trans_capacity =

| trans_coverage =

| insignia = COSI logo.png

| insignia_caption = Logo of COSI with all the participating institutions.

| insignia_size = 150px

| programme = SMEX

| previous_mission = SMEX-16

| next_mission = SMEX-18

}}

The Compton Spectrometer and Imager (COSI) is a NASA SMEX astrophysics mission that will launch a soft gamma-ray telescope (0.2–5 MeV) in 2027.{{cite web |url=https://science.nasa.gov/mission/cosi |title=COSI |work=NASA |date=16 June 2023 |access-date=22 December 2023}}{{cite web |url=https://www.nasa.gov/press-release/nasa-selects-gamma-ray-telescope-to-chart-milky-way-evolution|title=NASA Selects Gamma-ray Telescope to Chart Milky Way Evolution|publisher=NASA|date=18 October 2021 |access-date=21 October 2021}} {{PD-notice}} It is a wide-field compact Compton telescope (CCT) that is uniquely suited to investigate the "MeV gap" (0.1–10 MeV).{{cite journal | arxiv=1907.07558 | last1=McEnery | first1=Julie | author2=Juan Abel Barrio | last3=Agudo | first3=Ivan | last4=Ajello | first4=Marco | last5=Álvarez | first5=José-Manuel | last6=Ansoldi | first6=Stefano | last7=Anton | first7=Sonia | last8=Auricchio | first8=Natalia | last9=Stephen | first9=John B. | last10=Baldini | first10=Luca | last11=Bambi | first11=Cosimo | last12=Baring | first12=Matthew | last13=Barres | first13=Ulisses | last14=Bastieri | first14=Denis | last15=Beacom | first15=John | last16=Beckmann | first16=Volker | last17=Bednarek | first17=Wlodek | last18=Bernard | first18=Denis | last19=Bissaldi | first19=Elisabetta | last20=Bloser | first20=Peter | last21=Blumer | first21=Harsha | last22=Boettcher | first22=Markus | last23=Boggs | first23=Steven | last24=Bolotnikov | first24=Aleksey | last25=Bottacini | first25=Eugenio | last26=Bozhilov | first26=Vladimir | last27=Bozzo | first27=Enrico | last28=Briggs | first28=Michael | last29=Buckley | first29=Jim | last30=Burns | first30=Eric | title=All-sky Medium Energy Gamma-ray Observatory: Exploring the Extreme Multimessenger Universe | journal=Bulletin of the American Astronomical Society | date=2019 | volume=51 | issue=7 | page=245 | bibcode=2019BAAS...51g.245M | display-authors=1 }} It provides imaging, spectroscopy, and polarimetry of astrophysical sources, and its germanium detectors provide excellent energy resolution for emission line measurements.{{cite arXiv | eprint=2308.12362 | last1=Tomsick | first1=John A. | last2=Boggs | first2=Steven E. | last3=Zoglauer | first3=Andreas | last4=Hartmann | first4=Dieter | last5=Ajello | first5=Marco | last6=Burns | first6=Eric | last7=Fryer | first7=Chris | last8=Karwin | first8=Chris | last9=Kierans | first9=Carolyn | last10=Lowell | first10=Alexander | last11=Malzac | first11=Julien | last12=Roberts | first12=Jarred | last13=Saint-Hilaire | first13=Pascal | last14=Shih | first14=Albert | last15=Siegert | first15=Thomas | last16=Sleator | first16=Clio | last17=Takahashi | first17=Tadayuki | last18=Tavecchio | first18=Fabrizio | last19=Wulf | first19=Eric | last20=Beechert | first20=Jacqueline | last21=Gulick | first21=Hannah | last22=Joens | first22=Alyson | last23=Lazar | first23=Hadar | last24=Neights | first24=Eliza | author25=Juan Carlos Martinez Oliveros | last26=Matsumoto | first26=Shigeki | last27=Melia | first27=Tom | last28=Yoneda | first28=Hiroki | last29=Amman | first29=Mark | last30=Bal | first30=Dhruv | title=The Compton Spectrometer and Imager | date=2023 | class=astro-ph.HE | display-authors=1 }}

The germanium detectors have an instantaneous field of view of more than 25% of the sky, and they are surrounded on the sides and bottom by active shields, which provide background rejection while also allowing for detection of gamma-ray bursts and other gamma-ray flares across the majority of the sky.

History

COSI has its origins in the Nuclear Compton Telescope (NCT),{{Cite journal |last1=Chang |first1=Hsiang-Kuang |last2=Boggs |first2=Steven |last3=Chang |first3=Yuan-Hann |date=2007-01-01 |title=The Nuclear Compton Telescope (NCT): Scientific goals and expected sensitivity |url=https://www.sciencedirect.com/science/article/pii/S0273117707007752 |journal=Advances in Space Research |volume=40 |issue=8 |pages=1281–1287 |doi=10.1016/j.asr.2007.07.012 |bibcode=2007AdSpR..40.1281C |issn=0273-1177|url-access=subscription }} which was a prototype designed to study astrophysical sources of nuclear line emission and gamma-ray polarization. The NCT was a balloon-borne soft gamma-ray telescope, flying on several high-altitude balloon missions to test and refine its technology. Flights included launches from locations such as New Zealand and Antarctica.{{Cite web |date=2016-03-13 |title=Previous Campaigns |url=https://cosi.ssl.berkeley.edu/campaigns/previous-campaigns/ |access-date=2024-07-20 |website=COSI |language=en-US}}

File:COSI Balloon Stage.webp

COSI evolved from the advancements and lessons learned from the NCT missions. The improved design incorporated germanium cross-strip detectors to enhance sensitivity and resolution. This progression culminated in the development of a more sophisticated instrument capable of high-resolution spectroscopy, wide-field imaging, and gamma-ray polarization measurements. The successful demonstration of NCT's technology in balloon missions laid the groundwork for COSI to be selected as a NASA Small Explorer (SMEX) mission.{{Cite web |date=2020-12-04 |title=COSI |url=https://cosi.ssl.berkeley.edu/blog/ |access-date=2024-07-20 |website=COSI |language=en-US}}

Mission

"For more than 60 years, NASA has provided opportunities for inventive, smaller-scale missions to fill knowledge gaps where we still seek answers", said Thomas Zurbuchen, associate administrator for the agency's Science Mission Directorate in Washington, D.C. "COSI will answer questions about the origin of the chemical elements in our own Milky Way galaxy, the very ingredients critical to the formation of Earth itself".

The principal investigator is John Tomsick at the University of California, Berkeley. The mission will cost approximately US$145 million, with an additional launch cost of approximately US$69 million.{{Cite web |title=NASA Awards Launch Services Contract for Space Telescope Mission – NASA |url=https://www.nasa.gov/news-release/nasa-awards-launch-services-contract-for-space-telescope-mission/ |access-date=2024-07-02 |language=en-US}} The spacecraft is targeted to launch August 2027 on a SpaceX Falcon 9 rocket from Cape Canaveral Space Force Station. The COSI team spent decades developing their technology through flights on scientific balloons. In 2016, they sent a version of the gamma-ray instrument aboard NASA's super pressure balloon, which is designed for long flights and heavy lifts.

NASA's Explorers Program is the agency's oldest continuous program. It provides frequent, low-cost access to space using principal investigator-led space research relevant to the astrophysics and heliophysics programs. Since the 1958 launch of Explorer 1, which discovered Earth's radiation belts, the program has launched more than 90 missions. The Cosmic Background Explorer (COBE), another NASA Explorer mission, led to a Nobel Prize in 2006 for its principal investigators. NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the program for NASA.

Partnership

COSI is a collaboration between High Energy Astrophysics Group, Space Sciences Laboratory at UC Berkeley; Center for Astrophysics and Space Sciences, UCSD; Institute of Astronomy at National Tsing Hua University, Taiwan; Lawrence Berkeley National Laboratory; NASA Goddard Space Flight Center; U.S. Naval Research Laboratory; NASA Columbia Scientific Balloon Facility and [https://blogs.nasa.gov/superpressureballoon/ NASA Super Pressure Balloon Blog].{{Cite web |date=2016-03-11 |title=Balloon Team |url=https://cosi.ssl.berkeley.edu/team/ |access-date=2024-07-19 |website=COSI |language=en-US}}

References

External links

[https://cosi.ssl.berkeley.edu/ Project web site]
[https://cosi.ssl.berkeley.edu/instrument/design/ How the instrument functions]
[https://arxiv.org/abs/1908.04334 The Compton Spectrometer and Imager] Astro2020 APC White Paper (Tomsick et al)

Category:Space telescopes

Category:Explorers Program

Category:2027 in spaceflight