Welcome to SETI.org!
Allen Telescope Array
Skip Navigation Links
ATA: How It WorksExpand ATA: How It Works
ObservationsExpand Observations
Results from the ATAExpand Results from the ATA
MultimediaExpand Multimedia
Visiting the ATA
Media InformationExpand Media Information

Targeted Star Search

Selecting Target Stars

Life as we know it developed on a planet orbiting a G2 V star, the Sun. The cryptic “G2 V” designation is the Sun’s “spectral type.” Based on a star’s spectrum, astronomers group stars by temperature. From hottest to coolest, the spectral classes are O, B, A, F, G, K, and M. Each class is subdivided into ten and numbered from 0 to 9. The Sun is a G2 star. The “V” is the Roman numeral for five and designates the Sun’s luminosity class. Stars in luminosity classes I, II, and III are “giant” stars, very luminous and nearing the end of their life as a star. Class IV stars are “sub-giant” stars that are just entering “old age” and as the name implies, large but not giant. Stars in luminosity class V, like the Sun, burn only hydrogen in their cores and are relatively stable.

It is generally agreed that stars with spectral types from about F5 through K5 may be suitable hosts for habitable planets. Some recent studies indicate the some cooler stars, perhaps to spectral type M4, also may host habitable planets.

The HabCat Catalogs

In 2003, Margaret Turnbull and Jill Tarter published two lists of selected stars. The Nearby Habitable Systems (HabCat1) was created from the Hipparcos Catalogue by examining the information on distances, stellar variability, multiplicity, kinematics, and spectral classification for the 118,218 stars contained therein. They also made use of information from several other catalogs containing data for Hipparcos stars on X-ray luminosity, Ca II H and K activity, rotation, spectral types, kinematics, metallicity,

and Stromgren photometry. Combined with theoretical studies on habitable zones, evolutionary tracks, and third-body orbital stability, these data were used to remove unsuitable stars from HabCat, leaving a residue of stars that, to the best of our current knowledge, are potentially habitable hosts for complex life. The resulting HabCat1 catalog contains 17,133 well-selected “habstars”.

Since we need about one million target stars to fully utilize the capability of the ATA, a second catalog of stars was derived from the Tycho-2 Catalogue of 2.5 million stars. Unlike the Hipparcos stars, the Tycho stars did not have distance measurements. The approximately 250,000 stars of HabCat2 were selected primarily by their colors (brightness in blue and “visual” filters) and proper motion (motion across the sky).

You can download the HabCat1 list below. Here’s a peek at the first few entries and an explanation of the columns..

HIP

RA

RA

RA

Dec

Dec

Dec

v_mag

parllx

B-V

HD

BD


h

m

s

d

m

s


mas




6

0

0

4.3

3

56

47.4

12.31

18.8

1.336



7

0

0

5.4

20

2

11.8

9.64

17.74

0.74


B+19 5185

10

0

0

8.7

-50

52

1.5

8.59

10.76

0.489

224717


18

0

0

12.7

-4

3

13.5

11.03

19.93

1.567


B- 4 6001

24

0

0

18.2

-23

27

9.9

9.05

9.73

0.528

224746


HIP – Hipparcos Catalogue number

RA – Right Ascension (J2000) in hours, minutes, and seconds

Dec – Declination (J2000) in degrees, minutes, and seconds

v_mag – visual magnitude (apparent brightness)
a star with v_mag less than 6 is visible to the eye with a dark sky

parllx – parallax angle (in milliarcseconds) of motion of star due to Earth’s orbit around the Sun
Distance in parsecs = 1000/parallax
Distance in light years = 3262/parallax

B-V – Color Index, the difference in brightness measured in special Blue and Visual filters

HD – Henry Draper Catalogue number

BD – Bonner Durchmusterung Catalogue number

The HabCat1 list is in tab delimited text format.

LINK TO HABCAT text fileHERE

SETI Institute - 515 N. Whisman Road - Mountain View, CA 94043 - Phone 650.961.6633 - Fax 650-961-7099
Please send us your questions and comments

Copyright © 2008, SETI Institute - Unless otherwise indicated, the documents and graphics stored on this Web server, www.seti.org, are copyrighted. Links to these documents are permitted and encouraged. No copies may be made without permission.