| Boresight | RA | Dec | Roll | Ecliptic Longitude | Ecliptic Latitude |
|---|---|---|---|---|---|
| Spacecraft | 357.294 | -63.006 | -137.478 | 320.5 | -54.0 |
| Camera 1 | 329.486 | -31.617 | -68.884 | 320.5 | -18.0 |
| Camera 2 | 343.687 | -53.324 | -59.095 | 320.5 | -42.0 |
| Camera 3 | 21.858 | -70.243 | 155.167 | 320.5 | -66.0 |
| Camera 4 | 90.003 | -66.565 | -140.477 | 250.8 | -90.0 |
| All coordinates are degrees (J2000) | |||||
Map of TESS camera fields-of-view in ecliptic coordinates. Camera 1 is red, camera 2 is magenta, camera 3 is blue, camera 4 is green. The field of camera 4 looks distorted because it is centered on the ecliptic pole. The thin black line is the ecliptic; the thick black line is the galactic plane.
Map of TESS camera fields-of-view in celestial coordinates. Camera 1 is red, camera 2 is magenta, camera 3 is blue, camera 4 is green. The thin black line is the ecliptic; the thick black line is the galactic plane.
Targets for Sector 28
During Sector 28, 20,000 stars were observed at two-minute cadence, 1000 at 20-second cadence, and full-frame images are collected every 10 minutes.
The list of targets observed at two-minute cadence are given on the Target List page. The target list includes the camera and CCD on which the target can be found, TIC ID, RA, declination, and TESS magnitude.
Target Characteristics
The plots below show the distribution of stellar temperature, radius, and magnitude.
Earth and Moon Locations in the TESS Fields
Refer to Scattered Light page for an overview of these plots.
