Name | UVI-BurstCube |
---|---|
Type | CubeSat |
Units or mass | 3U |
Status | not launched, expected in 2023 |
Organisation | University of the Virgin Islands |
Institution | University |
Entity | Academic / Education |
Nation | US |
Oneliner |
The objective is to detect gamma ray bursts that correspond to collapsing neutron stars and black holes. |
Description |
Gamma ray bursts (GRBs) are energetic electromagnetic events produced by merging neutron stars and black holes. There are two types of GRBs: short-duration gamma ray bursts (sGRBs) that last less than 2 seconds and long-duration gamma ray bursts (lGRBs) that range from 2 second to a few hundred seconds. For BurstCube's and UVI-GREAT's mission, the interest will be in sGRBs, which are believed to be related to gravitational waves (GWs). GWs provide scientist with a new to observe the universe aside from electromagnetic radiation. UVI-GREAT would complement BurstCube and Fermi in the detection of GRBs enabling near complete sky coverage by providing 2 pi FOV. To detect the gamma burst from extragalactic sources, the instrument will be built using cesium iodide scintillators, silicon photo-multipliers and a DRS4 evaluation board on a 3U CubeSat. The radiation sources used in the instrument testing include Americium-241, Cobalt-60, Cesium-137, and Bismuth-207. Will collaborate closely with colleagues at NASA-Goddard Space Flight Center (GSFC) who are also building versions of the same Gamma-Ray Burst detection satellite that we have here at UVI (BurstCube). |
Sources | [1] [2] [3] |
Photo sources | [1] |
Last modified: 2023-06-09
Detailed UVI-BurstCube entry in the Database
Full Nanosats Database (much more data)